The ATLAS Collaboration
Acknowledgements.tex
% Acknowledgements for papers with collision data
% Version 06-Mar-2017

% Standard acknowledgements start here
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We thank CERN for the very successful operation of the LHC, as well as the
support staff from our institutions without whom ATLAS could not be
operated efficiently.

We acknowledge the support of ANPCyT, Argentina; YerPhI, Armenia; ARC, Australia; BMWFW and FWF, Austria; ANAS, Azerbaijan; SSTC, Belarus; CNPq and FAPESP, Brazil; NSERC, NRC and CFI, Canada; CERN; CONICYT, Chile; CAS, MOST and NSFC, China; COLCIENCIAS, Colombia; MSMT CR, MPO CR and VSC CR, Czech Republic; DNRF and DNSRC, Denmark; IN2P3-CNRS, CEA-DSM/IRFU, France; SRNSF, Georgia; BMBF, HGF, and MPG, Germany; GSRT, Greece; RGC, Hong Kong SAR, China; ISF, I-CORE and Benoziyo Center, Israel; INFN, Italy; MEXT and JSPS, Japan; CNRST, Morocco; NWO, Netherlands; RCN, Norway; MNiSW and NCN, Poland; FCT, Portugal; MNE/IFA, Romania; MES of Russia and NRC KI, Russian Federation; JINR; MESTD, Serbia; MSSR, Slovakia; ARRS and MIZ\v{S}, Slovenia; DST/NRF, South Africa; MINECO, Spain; SRC and Wallenberg Foundation, Sweden; SERI, SNSF and Cantons of Bern and Geneva, Switzerland; MOST, Taiwan; TAEK, Turkey; STFC, United Kingdom; DOE and NSF, United States of America. In addition, individual groups and members have received support from BCKDF, the Canada Council, CANARIE, CRC, Compute Canada, FQRNT, and the Ontario Innovation Trust, Canada; EPLANET, ERC, ERDF, FP7, Horizon 2020 and Marie Sk{\l}odowska-Curie Actions, European Union; Investissements d'Avenir Labex and Idex, ANR, R{\'e}gion Auvergne and Fondation Partager le Savoir, France; DFG and AvH Foundation, Germany; Herakleitos, Thales and Aristeia programmes co-financed by EU-ESF and the Greek NSRF; BSF, GIF and Minerva, Israel; BRF, Norway; CERCA Programme Generalitat de Catalunya, Generalitat Valenciana, Spain; the Royal Society and Leverhulme Trust, United Kingdom.

The crucial computing support from all WLCG partners is acknowledged gratefully, in particular from CERN, the ATLAS Tier-1 facilities at TRIUMF (Canada), NDGF (Denmark, Norway, Sweden), CC-IN2P3 (France), KIT/GridKA (Germany), INFN-CNAF (Italy), NL-T1 (Netherlands), PIC (Spain), ASGC (Taiwan), RAL (UK) and BNL (USA), the Tier-2 facilities worldwide and large non-WLCG resource providers. Major contributors of computing resources are listed in Ref.~\cite{ATL-GEN-PUB-2016-002}.
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atlas_authlist.tex
% ATLAS Collaboration author list
% Data extracted on 05-Dec-2016 for paper reference STDM-2016-01
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{\Large The ATLAS Collaboration}

\bigskip

M.~Aaboud$^\textrm{\scriptsize 137d}$,
G.~Aad$^\textrm{\scriptsize 88}$,
B.~Abbott$^\textrm{\scriptsize 115}$,
J.~Abdallah$^\textrm{\scriptsize 8}$,
O.~Abdinov$^\textrm{\scriptsize 12}$,
B.~Abeloos$^\textrm{\scriptsize 119}$,
R.~Aben$^\textrm{\scriptsize 109}$,
O.S.~AbouZeid$^\textrm{\scriptsize 139}$,
N.L.~Abraham$^\textrm{\scriptsize 151}$,
H.~Abramowicz$^\textrm{\scriptsize 155}$,
H.~Abreu$^\textrm{\scriptsize 154}$,
R.~Abreu$^\textrm{\scriptsize 118}$,
Y.~Abulaiti$^\textrm{\scriptsize 148a,148b}$,
B.S.~Acharya$^\textrm{\scriptsize 167a,167b}$$^{,a}$,
S.~Adachi$^\textrm{\scriptsize 157}$,
L.~Adamczyk$^\textrm{\scriptsize 41a}$,
D.L.~Adams$^\textrm{\scriptsize 27}$,
J.~Adelman$^\textrm{\scriptsize 110}$,
S.~Adomeit$^\textrm{\scriptsize 102}$,
T.~Adye$^\textrm{\scriptsize 133}$,
A.A.~Affolder$^\textrm{\scriptsize 77}$,
T.~Agatonovic-Jovin$^\textrm{\scriptsize 14}$,
J.A.~Aguilar-Saavedra$^\textrm{\scriptsize 128a,128f}$,
S.P.~Ahlen$^\textrm{\scriptsize 24}$,
F.~Ahmadov$^\textrm{\scriptsize 68}$$^{,b}$,
G.~Aielli$^\textrm{\scriptsize 135a,135b}$,
H.~Akerstedt$^\textrm{\scriptsize 148a,148b}$,
T.P.A.~{\AA}kesson$^\textrm{\scriptsize 84}$,
A.V.~Akimov$^\textrm{\scriptsize 98}$,
G.L.~Alberghi$^\textrm{\scriptsize 22a,22b}$,
J.~Albert$^\textrm{\scriptsize 172}$,
S.~Albrand$^\textrm{\scriptsize 58}$,
M.J.~Alconada~Verzini$^\textrm{\scriptsize 74}$,
M.~Aleksa$^\textrm{\scriptsize 32}$,
I.N.~Aleksandrov$^\textrm{\scriptsize 68}$,
C.~Alexa$^\textrm{\scriptsize 28b}$,
G.~Alexander$^\textrm{\scriptsize 155}$,
T.~Alexopoulos$^\textrm{\scriptsize 10}$,
M.~Alhroob$^\textrm{\scriptsize 115}$,
B.~Ali$^\textrm{\scriptsize 130}$,
M.~Aliev$^\textrm{\scriptsize 76a,76b}$,
G.~Alimonti$^\textrm{\scriptsize 94a}$,
J.~Alison$^\textrm{\scriptsize 33}$,
S.P.~Alkire$^\textrm{\scriptsize 38}$,
B.M.M.~Allbrooke$^\textrm{\scriptsize 151}$,
B.W.~Allen$^\textrm{\scriptsize 118}$,
P.P.~Allport$^\textrm{\scriptsize 19}$,
A.~Aloisio$^\textrm{\scriptsize 106a,106b}$,
A.~Alonso$^\textrm{\scriptsize 39}$,
F.~Alonso$^\textrm{\scriptsize 74}$,
C.~Alpigiani$^\textrm{\scriptsize 140}$,
A.A.~Alshehri$^\textrm{\scriptsize 56}$,
M.~Alstaty$^\textrm{\scriptsize 88}$,
B.~Alvarez~Gonzalez$^\textrm{\scriptsize 32}$,
D.~\'{A}lvarez~Piqueras$^\textrm{\scriptsize 170}$,
M.G.~Alviggi$^\textrm{\scriptsize 106a,106b}$,
B.T.~Amadio$^\textrm{\scriptsize 16}$,
Y.~Amaral~Coutinho$^\textrm{\scriptsize 26a}$,
C.~Amelung$^\textrm{\scriptsize 25}$,
D.~Amidei$^\textrm{\scriptsize 92}$,
S.P.~Amor~Dos~Santos$^\textrm{\scriptsize 128a,128c}$,
A.~Amorim$^\textrm{\scriptsize 128a,128b}$,
S.~Amoroso$^\textrm{\scriptsize 32}$,
G.~Amundsen$^\textrm{\scriptsize 25}$,
C.~Anastopoulos$^\textrm{\scriptsize 141}$,
L.S.~Ancu$^\textrm{\scriptsize 52}$,
N.~Andari$^\textrm{\scriptsize 19}$,
T.~Andeen$^\textrm{\scriptsize 11}$,
C.F.~Anders$^\textrm{\scriptsize 60b}$,
G.~Anders$^\textrm{\scriptsize 32}$,
J.K.~Anders$^\textrm{\scriptsize 77}$,
K.J.~Anderson$^\textrm{\scriptsize 33}$,
A.~Andreazza$^\textrm{\scriptsize 94a,94b}$,
V.~Andrei$^\textrm{\scriptsize 60a}$,
S.~Angelidakis$^\textrm{\scriptsize 9}$,
I.~Angelozzi$^\textrm{\scriptsize 109}$,
A.~Angerami$^\textrm{\scriptsize 38}$,
F.~Anghinolfi$^\textrm{\scriptsize 32}$,
A.V.~Anisenkov$^\textrm{\scriptsize 111}$$^{,c}$,
N.~Anjos$^\textrm{\scriptsize 13}$,
A.~Annovi$^\textrm{\scriptsize 126a,126b}$,
C.~Antel$^\textrm{\scriptsize 60a}$,
M.~Antonelli$^\textrm{\scriptsize 50}$,
A.~Antonov$^\textrm{\scriptsize 100}$$^{,*}$,
D.J.~Antrim$^\textrm{\scriptsize 166}$,
F.~Anulli$^\textrm{\scriptsize 134a}$,
M.~Aoki$^\textrm{\scriptsize 69}$,
L.~Aperio~Bella$^\textrm{\scriptsize 19}$,
G.~Arabidze$^\textrm{\scriptsize 93}$,
Y.~Arai$^\textrm{\scriptsize 69}$,
J.P.~Araque$^\textrm{\scriptsize 128a}$,
A.T.H.~Arce$^\textrm{\scriptsize 48}$,
F.A.~Arduh$^\textrm{\scriptsize 74}$,
J-F.~Arguin$^\textrm{\scriptsize 97}$,
S.~Argyropoulos$^\textrm{\scriptsize 66}$,
M.~Arik$^\textrm{\scriptsize 20a}$,
A.J.~Armbruster$^\textrm{\scriptsize 145}$,
L.J.~Armitage$^\textrm{\scriptsize 79}$,
O.~Arnaez$^\textrm{\scriptsize 32}$,
H.~Arnold$^\textrm{\scriptsize 51}$,
M.~Arratia$^\textrm{\scriptsize 30}$,
O.~Arslan$^\textrm{\scriptsize 23}$,
A.~Artamonov$^\textrm{\scriptsize 99}$,
G.~Artoni$^\textrm{\scriptsize 122}$,
S.~Artz$^\textrm{\scriptsize 86}$,
S.~Asai$^\textrm{\scriptsize 157}$,
N.~Asbah$^\textrm{\scriptsize 45}$,
A.~Ashkenazi$^\textrm{\scriptsize 155}$,
B.~{\AA}sman$^\textrm{\scriptsize 148a,148b}$,
L.~Asquith$^\textrm{\scriptsize 151}$,
K.~Assamagan$^\textrm{\scriptsize 27}$,
R.~Astalos$^\textrm{\scriptsize 146a}$,
M.~Atkinson$^\textrm{\scriptsize 169}$,
N.B.~Atlay$^\textrm{\scriptsize 143}$,
K.~Augsten$^\textrm{\scriptsize 130}$,
G.~Avolio$^\textrm{\scriptsize 32}$,
B.~Axen$^\textrm{\scriptsize 16}$,
M.K.~Ayoub$^\textrm{\scriptsize 119}$,
G.~Azuelos$^\textrm{\scriptsize 97}$$^{,d}$,
M.A.~Baak$^\textrm{\scriptsize 32}$,
A.E.~Baas$^\textrm{\scriptsize 60a}$,
M.J.~Baca$^\textrm{\scriptsize 19}$,
H.~Bachacou$^\textrm{\scriptsize 138}$,
K.~Bachas$^\textrm{\scriptsize 76a,76b}$,
M.~Backes$^\textrm{\scriptsize 122}$,
M.~Backhaus$^\textrm{\scriptsize 32}$,
P.~Bagiacchi$^\textrm{\scriptsize 134a,134b}$,
P.~Bagnaia$^\textrm{\scriptsize 134a,134b}$,
Y.~Bai$^\textrm{\scriptsize 35a}$,
J.T.~Baines$^\textrm{\scriptsize 133}$,
M.~Bajic$^\textrm{\scriptsize 39}$,
O.K.~Baker$^\textrm{\scriptsize 179}$,
E.M.~Baldin$^\textrm{\scriptsize 111}$$^{,c}$,
P.~Balek$^\textrm{\scriptsize 175}$,
T.~Balestri$^\textrm{\scriptsize 150}$,
F.~Balli$^\textrm{\scriptsize 138}$,
W.K.~Balunas$^\textrm{\scriptsize 124}$,
E.~Banas$^\textrm{\scriptsize 42}$,
Sw.~Banerjee$^\textrm{\scriptsize 176}$$^{,e}$,
A.A.E.~Bannoura$^\textrm{\scriptsize 178}$,
L.~Barak$^\textrm{\scriptsize 32}$,
E.L.~Barberio$^\textrm{\scriptsize 91}$,
D.~Barberis$^\textrm{\scriptsize 53a,53b}$,
M.~Barbero$^\textrm{\scriptsize 88}$,
T.~Barillari$^\textrm{\scriptsize 103}$,
M-S~Barisits$^\textrm{\scriptsize 32}$,
T.~Barklow$^\textrm{\scriptsize 145}$,
N.~Barlow$^\textrm{\scriptsize 30}$,
S.L.~Barnes$^\textrm{\scriptsize 87}$,
B.M.~Barnett$^\textrm{\scriptsize 133}$,
R.M.~Barnett$^\textrm{\scriptsize 16}$,
Z.~Barnovska-Blenessy$^\textrm{\scriptsize 36a}$,
A.~Baroncelli$^\textrm{\scriptsize 136a}$,
G.~Barone$^\textrm{\scriptsize 25}$,
A.J.~Barr$^\textrm{\scriptsize 122}$,
L.~Barranco~Navarro$^\textrm{\scriptsize 170}$,
F.~Barreiro$^\textrm{\scriptsize 85}$,
J.~Barreiro~Guimar\~{a}es~da~Costa$^\textrm{\scriptsize 35a}$,
R.~Bartoldus$^\textrm{\scriptsize 145}$,
A.E.~Barton$^\textrm{\scriptsize 75}$,
P.~Bartos$^\textrm{\scriptsize 146a}$,
A.~Basalaev$^\textrm{\scriptsize 125}$,
A.~Bassalat$^\textrm{\scriptsize 119}$$^{,f}$,
R.L.~Bates$^\textrm{\scriptsize 56}$,
S.J.~Batista$^\textrm{\scriptsize 161}$,
J.R.~Batley$^\textrm{\scriptsize 30}$,
M.~Battaglia$^\textrm{\scriptsize 139}$,
M.~Bauce$^\textrm{\scriptsize 134a,134b}$,
F.~Bauer$^\textrm{\scriptsize 138}$,
H.S.~Bawa$^\textrm{\scriptsize 145}$$^{,g}$,
J.B.~Beacham$^\textrm{\scriptsize 113}$,
M.D.~Beattie$^\textrm{\scriptsize 75}$,
T.~Beau$^\textrm{\scriptsize 83}$,
P.H.~Beauchemin$^\textrm{\scriptsize 165}$,
P.~Bechtle$^\textrm{\scriptsize 23}$,
H.P.~Beck$^\textrm{\scriptsize 18}$$^{,h}$,
K.~Becker$^\textrm{\scriptsize 122}$,
M.~Becker$^\textrm{\scriptsize 86}$,
M.~Beckingham$^\textrm{\scriptsize 173}$,
C.~Becot$^\textrm{\scriptsize 112}$,
A.J.~Beddall$^\textrm{\scriptsize 20e}$,
A.~Beddall$^\textrm{\scriptsize 20b}$,
V.A.~Bednyakov$^\textrm{\scriptsize 68}$,
M.~Bedognetti$^\textrm{\scriptsize 109}$,
C.P.~Bee$^\textrm{\scriptsize 150}$,
L.J.~Beemster$^\textrm{\scriptsize 109}$,
T.A.~Beermann$^\textrm{\scriptsize 32}$,
M.~Begel$^\textrm{\scriptsize 27}$,
J.K.~Behr$^\textrm{\scriptsize 45}$,
A.S.~Bell$^\textrm{\scriptsize 81}$,
G.~Bella$^\textrm{\scriptsize 155}$,
L.~Bellagamba$^\textrm{\scriptsize 22a}$,
A.~Bellerive$^\textrm{\scriptsize 31}$,
M.~Bellomo$^\textrm{\scriptsize 89}$,
K.~Belotskiy$^\textrm{\scriptsize 100}$,
O.~Beltramello$^\textrm{\scriptsize 32}$,
N.L.~Belyaev$^\textrm{\scriptsize 100}$,
O.~Benary$^\textrm{\scriptsize 155}$$^{,*}$,
D.~Benchekroun$^\textrm{\scriptsize 137a}$,
M.~Bender$^\textrm{\scriptsize 102}$,
K.~Bendtz$^\textrm{\scriptsize 148a,148b}$,
N.~Benekos$^\textrm{\scriptsize 10}$,
Y.~Benhammou$^\textrm{\scriptsize 155}$,
E.~Benhar~Noccioli$^\textrm{\scriptsize 179}$,
J.~Benitez$^\textrm{\scriptsize 66}$,
D.P.~Benjamin$^\textrm{\scriptsize 48}$,
J.R.~Bensinger$^\textrm{\scriptsize 25}$,
S.~Bentvelsen$^\textrm{\scriptsize 109}$,
L.~Beresford$^\textrm{\scriptsize 122}$,
M.~Beretta$^\textrm{\scriptsize 50}$,
D.~Berge$^\textrm{\scriptsize 109}$,
E.~Bergeaas~Kuutmann$^\textrm{\scriptsize 168}$,
N.~Berger$^\textrm{\scriptsize 5}$,
J.~Beringer$^\textrm{\scriptsize 16}$,
S.~Berlendis$^\textrm{\scriptsize 58}$,
N.R.~Bernard$^\textrm{\scriptsize 89}$,
C.~Bernius$^\textrm{\scriptsize 112}$,
F.U.~Bernlochner$^\textrm{\scriptsize 23}$,
T.~Berry$^\textrm{\scriptsize 80}$,
P.~Berta$^\textrm{\scriptsize 131}$,
C.~Bertella$^\textrm{\scriptsize 86}$,
G.~Bertoli$^\textrm{\scriptsize 148a,148b}$,
F.~Bertolucci$^\textrm{\scriptsize 126a,126b}$,
I.A.~Bertram$^\textrm{\scriptsize 75}$,
C.~Bertsche$^\textrm{\scriptsize 45}$,
D.~Bertsche$^\textrm{\scriptsize 115}$,
G.J.~Besjes$^\textrm{\scriptsize 39}$,
O.~Bessidskaia~Bylund$^\textrm{\scriptsize 148a,148b}$,
M.~Bessner$^\textrm{\scriptsize 45}$,
N.~Besson$^\textrm{\scriptsize 138}$,
C.~Betancourt$^\textrm{\scriptsize 51}$,
A.~Bethani$^\textrm{\scriptsize 58}$,
S.~Bethke$^\textrm{\scriptsize 103}$,
A.J.~Bevan$^\textrm{\scriptsize 79}$,
R.M.~Bianchi$^\textrm{\scriptsize 127}$,
M.~Bianco$^\textrm{\scriptsize 32}$,
O.~Biebel$^\textrm{\scriptsize 102}$,
D.~Biedermann$^\textrm{\scriptsize 17}$,
R.~Bielski$^\textrm{\scriptsize 87}$,
N.V.~Biesuz$^\textrm{\scriptsize 126a,126b}$,
M.~Biglietti$^\textrm{\scriptsize 136a}$,
J.~Bilbao~De~Mendizabal$^\textrm{\scriptsize 52}$,
T.R.V.~Billoud$^\textrm{\scriptsize 97}$,
H.~Bilokon$^\textrm{\scriptsize 50}$,
M.~Bindi$^\textrm{\scriptsize 57}$,
A.~Bingul$^\textrm{\scriptsize 20b}$,
C.~Bini$^\textrm{\scriptsize 134a,134b}$,
S.~Biondi$^\textrm{\scriptsize 22a,22b}$,
T.~Bisanz$^\textrm{\scriptsize 57}$,
D.M.~Bjergaard$^\textrm{\scriptsize 48}$,
C.W.~Black$^\textrm{\scriptsize 152}$,
J.E.~Black$^\textrm{\scriptsize 145}$,
K.M.~Black$^\textrm{\scriptsize 24}$,
D.~Blackburn$^\textrm{\scriptsize 140}$,
R.E.~Blair$^\textrm{\scriptsize 6}$,
T.~Blazek$^\textrm{\scriptsize 146a}$,
I.~Bloch$^\textrm{\scriptsize 45}$,
C.~Blocker$^\textrm{\scriptsize 25}$,
A.~Blue$^\textrm{\scriptsize 56}$,
W.~Blum$^\textrm{\scriptsize 86}$$^{,*}$,
U.~Blumenschein$^\textrm{\scriptsize 57}$,
S.~Blunier$^\textrm{\scriptsize 34a}$,
G.J.~Bobbink$^\textrm{\scriptsize 109}$,
V.S.~Bobrovnikov$^\textrm{\scriptsize 111}$$^{,c}$,
S.S.~Bocchetta$^\textrm{\scriptsize 84}$,
A.~Bocci$^\textrm{\scriptsize 48}$,
C.~Bock$^\textrm{\scriptsize 102}$,
M.~Boehler$^\textrm{\scriptsize 51}$,
D.~Boerner$^\textrm{\scriptsize 178}$,
J.A.~Bogaerts$^\textrm{\scriptsize 32}$,
D.~Bogavac$^\textrm{\scriptsize 14}$,
A.G.~Bogdanchikov$^\textrm{\scriptsize 111}$,
C.~Bohm$^\textrm{\scriptsize 148a}$,
V.~Boisvert$^\textrm{\scriptsize 80}$,
P.~Bokan$^\textrm{\scriptsize 14}$,
T.~Bold$^\textrm{\scriptsize 41a}$,
A.S.~Boldyrev$^\textrm{\scriptsize 101}$,
M.~Bomben$^\textrm{\scriptsize 83}$,
M.~Bona$^\textrm{\scriptsize 79}$,
M.~Boonekamp$^\textrm{\scriptsize 138}$,
A.~Borisov$^\textrm{\scriptsize 132}$,
G.~Borissov$^\textrm{\scriptsize 75}$,
J.~Bortfeldt$^\textrm{\scriptsize 32}$,
D.~Bortoletto$^\textrm{\scriptsize 122}$,
V.~Bortolotto$^\textrm{\scriptsize 62a,62b,62c}$,
K.~Bos$^\textrm{\scriptsize 109}$,
D.~Boscherini$^\textrm{\scriptsize 22a}$,
M.~Bosman$^\textrm{\scriptsize 13}$,
J.D.~Bossio~Sola$^\textrm{\scriptsize 29}$,
J.~Boudreau$^\textrm{\scriptsize 127}$,
J.~Bouffard$^\textrm{\scriptsize 2}$,
E.V.~Bouhova-Thacker$^\textrm{\scriptsize 75}$,
D.~Boumediene$^\textrm{\scriptsize 37}$,
C.~Bourdarios$^\textrm{\scriptsize 119}$,
S.K.~Boutle$^\textrm{\scriptsize 56}$,
A.~Boveia$^\textrm{\scriptsize 32}$,
J.~Boyd$^\textrm{\scriptsize 32}$,
I.R.~Boyko$^\textrm{\scriptsize 68}$,
J.~Bracinik$^\textrm{\scriptsize 19}$,
A.~Brandt$^\textrm{\scriptsize 8}$,
G.~Brandt$^\textrm{\scriptsize 57}$,
O.~Brandt$^\textrm{\scriptsize 60a}$,
U.~Bratzler$^\textrm{\scriptsize 158}$,
B.~Brau$^\textrm{\scriptsize 89}$,
J.E.~Brau$^\textrm{\scriptsize 118}$,
W.D.~Breaden~Madden$^\textrm{\scriptsize 56}$,
K.~Brendlinger$^\textrm{\scriptsize 124}$,
A.J.~Brennan$^\textrm{\scriptsize 91}$,
L.~Brenner$^\textrm{\scriptsize 109}$,
R.~Brenner$^\textrm{\scriptsize 168}$,
S.~Bressler$^\textrm{\scriptsize 175}$,
T.M.~Bristow$^\textrm{\scriptsize 49}$,
D.~Britton$^\textrm{\scriptsize 56}$,
D.~Britzger$^\textrm{\scriptsize 45}$,
F.M.~Brochu$^\textrm{\scriptsize 30}$,
I.~Brock$^\textrm{\scriptsize 23}$,
R.~Brock$^\textrm{\scriptsize 93}$,
G.~Brooijmans$^\textrm{\scriptsize 38}$,
T.~Brooks$^\textrm{\scriptsize 80}$,
W.K.~Brooks$^\textrm{\scriptsize 34b}$,
J.~Brosamer$^\textrm{\scriptsize 16}$,
E.~Brost$^\textrm{\scriptsize 110}$,
J.H~Broughton$^\textrm{\scriptsize 19}$,
P.A.~Bruckman~de~Renstrom$^\textrm{\scriptsize 42}$,
D.~Bruncko$^\textrm{\scriptsize 146b}$,
R.~Bruneliere$^\textrm{\scriptsize 51}$,
A.~Bruni$^\textrm{\scriptsize 22a}$,
G.~Bruni$^\textrm{\scriptsize 22a}$,
L.S.~Bruni$^\textrm{\scriptsize 109}$,
BH~Brunt$^\textrm{\scriptsize 30}$,
M.~Bruschi$^\textrm{\scriptsize 22a}$,
N.~Bruscino$^\textrm{\scriptsize 23}$,
P.~Bryant$^\textrm{\scriptsize 33}$,
L.~Bryngemark$^\textrm{\scriptsize 84}$,
T.~Buanes$^\textrm{\scriptsize 15}$,
Q.~Buat$^\textrm{\scriptsize 144}$,
P.~Buchholz$^\textrm{\scriptsize 143}$,
A.G.~Buckley$^\textrm{\scriptsize 56}$,
I.A.~Budagov$^\textrm{\scriptsize 68}$,
F.~Buehrer$^\textrm{\scriptsize 51}$,
M.K.~Bugge$^\textrm{\scriptsize 121}$,
O.~Bulekov$^\textrm{\scriptsize 100}$,
D.~Bullock$^\textrm{\scriptsize 8}$,
H.~Burckhart$^\textrm{\scriptsize 32}$,
S.~Burdin$^\textrm{\scriptsize 77}$,
C.D.~Burgard$^\textrm{\scriptsize 51}$,
A.M.~Burger$^\textrm{\scriptsize 5}$,
B.~Burghgrave$^\textrm{\scriptsize 110}$,
K.~Burka$^\textrm{\scriptsize 42}$,
S.~Burke$^\textrm{\scriptsize 133}$,
I.~Burmeister$^\textrm{\scriptsize 46}$,
J.T.P.~Burr$^\textrm{\scriptsize 122}$,
E.~Busato$^\textrm{\scriptsize 37}$,
D.~B\"uscher$^\textrm{\scriptsize 51}$,
V.~B\"uscher$^\textrm{\scriptsize 86}$,
P.~Bussey$^\textrm{\scriptsize 56}$,
J.M.~Butler$^\textrm{\scriptsize 24}$,
C.M.~Buttar$^\textrm{\scriptsize 56}$,
J.M.~Butterworth$^\textrm{\scriptsize 81}$,
P.~Butti$^\textrm{\scriptsize 109}$,
W.~Buttinger$^\textrm{\scriptsize 27}$,
A.~Buzatu$^\textrm{\scriptsize 56}$,
A.R.~Buzykaev$^\textrm{\scriptsize 111}$$^{,c}$,
S.~Cabrera~Urb\'an$^\textrm{\scriptsize 170}$,
D.~Caforio$^\textrm{\scriptsize 130}$,
V.M.~Cairo$^\textrm{\scriptsize 40a,40b}$,
O.~Cakir$^\textrm{\scriptsize 4a}$,
N.~Calace$^\textrm{\scriptsize 52}$,
P.~Calafiura$^\textrm{\scriptsize 16}$,
A.~Calandri$^\textrm{\scriptsize 88}$,
G.~Calderini$^\textrm{\scriptsize 83}$,
P.~Calfayan$^\textrm{\scriptsize 64}$,
G.~Callea$^\textrm{\scriptsize 40a,40b}$,
L.P.~Caloba$^\textrm{\scriptsize 26a}$,
S.~Calvente~Lopez$^\textrm{\scriptsize 85}$,
D.~Calvet$^\textrm{\scriptsize 37}$,
S.~Calvet$^\textrm{\scriptsize 37}$,
T.P.~Calvet$^\textrm{\scriptsize 88}$,
R.~Camacho~Toro$^\textrm{\scriptsize 33}$,
S.~Camarda$^\textrm{\scriptsize 32}$,
P.~Camarri$^\textrm{\scriptsize 135a,135b}$,
D.~Cameron$^\textrm{\scriptsize 121}$,
R.~Caminal~Armadans$^\textrm{\scriptsize 169}$,
C.~Camincher$^\textrm{\scriptsize 58}$,
S.~Campana$^\textrm{\scriptsize 32}$,
M.~Campanelli$^\textrm{\scriptsize 81}$,
A.~Camplani$^\textrm{\scriptsize 94a,94b}$,
A.~Campoverde$^\textrm{\scriptsize 143}$,
V.~Canale$^\textrm{\scriptsize 106a,106b}$,
A.~Canepa$^\textrm{\scriptsize 163a}$,
M.~Cano~Bret$^\textrm{\scriptsize 36c}$,
J.~Cantero$^\textrm{\scriptsize 116}$,
T.~Cao$^\textrm{\scriptsize 43}$,
M.D.M.~Capeans~Garrido$^\textrm{\scriptsize 32}$,
I.~Caprini$^\textrm{\scriptsize 28b}$,
M.~Caprini$^\textrm{\scriptsize 28b}$,
M.~Capua$^\textrm{\scriptsize 40a,40b}$,
R.M.~Carbone$^\textrm{\scriptsize 38}$,
R.~Cardarelli$^\textrm{\scriptsize 135a}$,
F.~Cardillo$^\textrm{\scriptsize 51}$,
I.~Carli$^\textrm{\scriptsize 131}$,
T.~Carli$^\textrm{\scriptsize 32}$,
G.~Carlino$^\textrm{\scriptsize 106a}$,
L.~Carminati$^\textrm{\scriptsize 94a,94b}$,
R.M.D.~Carney$^\textrm{\scriptsize 148a,148b}$,
S.~Caron$^\textrm{\scriptsize 108}$,
E.~Carquin$^\textrm{\scriptsize 34b}$,
G.D.~Carrillo-Montoya$^\textrm{\scriptsize 32}$,
J.R.~Carter$^\textrm{\scriptsize 30}$,
J.~Carvalho$^\textrm{\scriptsize 128a,128c}$,
D.~Casadei$^\textrm{\scriptsize 19}$,
M.P.~Casado$^\textrm{\scriptsize 13}$$^{,i}$,
M.~Casolino$^\textrm{\scriptsize 13}$,
D.W.~Casper$^\textrm{\scriptsize 166}$,
E.~Castaneda-Miranda$^\textrm{\scriptsize 147a}$,
R.~Castelijn$^\textrm{\scriptsize 109}$,
A.~Castelli$^\textrm{\scriptsize 109}$,
V.~Castillo~Gimenez$^\textrm{\scriptsize 170}$,
N.F.~Castro$^\textrm{\scriptsize 128a}$$^{,j}$,
A.~Catinaccio$^\textrm{\scriptsize 32}$,
J.R.~Catmore$^\textrm{\scriptsize 121}$,
A.~Cattai$^\textrm{\scriptsize 32}$,
J.~Caudron$^\textrm{\scriptsize 23}$,
V.~Cavaliere$^\textrm{\scriptsize 169}$,
E.~Cavallaro$^\textrm{\scriptsize 13}$,
D.~Cavalli$^\textrm{\scriptsize 94a}$,
M.~Cavalli-Sforza$^\textrm{\scriptsize 13}$,
V.~Cavasinni$^\textrm{\scriptsize 126a,126b}$,
F.~Ceradini$^\textrm{\scriptsize 136a,136b}$,
L.~Cerda~Alberich$^\textrm{\scriptsize 170}$,
A.S.~Cerqueira$^\textrm{\scriptsize 26b}$,
A.~Cerri$^\textrm{\scriptsize 151}$,
L.~Cerrito$^\textrm{\scriptsize 135a,135b}$,
F.~Cerutti$^\textrm{\scriptsize 16}$,
A.~Cervelli$^\textrm{\scriptsize 18}$,
S.A.~Cetin$^\textrm{\scriptsize 20d}$,
A.~Chafaq$^\textrm{\scriptsize 137a}$,
D.~Chakraborty$^\textrm{\scriptsize 110}$,
S.K.~Chan$^\textrm{\scriptsize 59}$,
Y.L.~Chan$^\textrm{\scriptsize 62a}$,
P.~Chang$^\textrm{\scriptsize 169}$,
J.D.~Chapman$^\textrm{\scriptsize 30}$,
D.G.~Charlton$^\textrm{\scriptsize 19}$,
A.~Chatterjee$^\textrm{\scriptsize 52}$,
C.C.~Chau$^\textrm{\scriptsize 161}$,
C.A.~Chavez~Barajas$^\textrm{\scriptsize 151}$,
S.~Che$^\textrm{\scriptsize 113}$,
S.~Cheatham$^\textrm{\scriptsize 167a,167c}$,
A.~Chegwidden$^\textrm{\scriptsize 93}$,
S.~Chekanov$^\textrm{\scriptsize 6}$,
S.V.~Chekulaev$^\textrm{\scriptsize 163a}$,
G.A.~Chelkov$^\textrm{\scriptsize 68}$$^{,k}$,
M.A.~Chelstowska$^\textrm{\scriptsize 92}$,
C.~Chen$^\textrm{\scriptsize 67}$,
H.~Chen$^\textrm{\scriptsize 27}$,
K.~Chen$^\textrm{\scriptsize 150}$,
S.~Chen$^\textrm{\scriptsize 35b}$,
S.~Chen$^\textrm{\scriptsize 157}$,
X.~Chen$^\textrm{\scriptsize 35c}$$^{,l}$,
Y.~Chen$^\textrm{\scriptsize 70}$,
H.C.~Cheng$^\textrm{\scriptsize 92}$,
H.J.~Cheng$^\textrm{\scriptsize 35a}$,
Y.~Cheng$^\textrm{\scriptsize 33}$,
A.~Cheplakov$^\textrm{\scriptsize 68}$,
E.~Cheremushkina$^\textrm{\scriptsize 132}$,
R.~Cherkaoui~El~Moursli$^\textrm{\scriptsize 137e}$,
V.~Chernyatin$^\textrm{\scriptsize 27}$$^{,*}$,
E.~Cheu$^\textrm{\scriptsize 7}$,
L.~Chevalier$^\textrm{\scriptsize 138}$,
V.~Chiarella$^\textrm{\scriptsize 50}$,
G.~Chiarelli$^\textrm{\scriptsize 126a,126b}$,
G.~Chiodini$^\textrm{\scriptsize 76a}$,
A.S.~Chisholm$^\textrm{\scriptsize 32}$,
A.~Chitan$^\textrm{\scriptsize 28b}$,
M.V.~Chizhov$^\textrm{\scriptsize 68}$,
K.~Choi$^\textrm{\scriptsize 64}$,
A.R.~Chomont$^\textrm{\scriptsize 37}$,
S.~Chouridou$^\textrm{\scriptsize 9}$,
B.K.B.~Chow$^\textrm{\scriptsize 102}$,
V.~Christodoulou$^\textrm{\scriptsize 81}$,
D.~Chromek-Burckhart$^\textrm{\scriptsize 32}$,
J.~Chudoba$^\textrm{\scriptsize 129}$,
A.J.~Chuinard$^\textrm{\scriptsize 90}$,
J.J.~Chwastowski$^\textrm{\scriptsize 42}$,
L.~Chytka$^\textrm{\scriptsize 117}$,
G.~Ciapetti$^\textrm{\scriptsize 134a,134b}$,
A.K.~Ciftci$^\textrm{\scriptsize 4a}$,
D.~Cinca$^\textrm{\scriptsize 46}$,
V.~Cindro$^\textrm{\scriptsize 78}$,
I.A.~Cioara$^\textrm{\scriptsize 23}$,
C.~Ciocca$^\textrm{\scriptsize 22a,22b}$,
A.~Ciocio$^\textrm{\scriptsize 16}$,
F.~Cirotto$^\textrm{\scriptsize 106a,106b}$,
Z.H.~Citron$^\textrm{\scriptsize 175}$,
M.~Citterio$^\textrm{\scriptsize 94a}$,
M.~Ciubancan$^\textrm{\scriptsize 28b}$,
A.~Clark$^\textrm{\scriptsize 52}$,
B.L.~Clark$^\textrm{\scriptsize 59}$,
M.R.~Clark$^\textrm{\scriptsize 38}$,
P.J.~Clark$^\textrm{\scriptsize 49}$,
R.N.~Clarke$^\textrm{\scriptsize 16}$,
C.~Clement$^\textrm{\scriptsize 148a,148b}$,
Y.~Coadou$^\textrm{\scriptsize 88}$,
M.~Cobal$^\textrm{\scriptsize 167a,167c}$,
A.~Coccaro$^\textrm{\scriptsize 52}$,
J.~Cochran$^\textrm{\scriptsize 67}$,
L.~Colasurdo$^\textrm{\scriptsize 108}$,
B.~Cole$^\textrm{\scriptsize 38}$,
A.P.~Colijn$^\textrm{\scriptsize 109}$,
J.~Collot$^\textrm{\scriptsize 58}$,
T.~Colombo$^\textrm{\scriptsize 166}$,
G.~Compostella$^\textrm{\scriptsize 103}$,
P.~Conde~Mui\~no$^\textrm{\scriptsize 128a,128b}$,
E.~Coniavitis$^\textrm{\scriptsize 51}$,
S.H.~Connell$^\textrm{\scriptsize 147b}$,
I.A.~Connelly$^\textrm{\scriptsize 80}$,
V.~Consorti$^\textrm{\scriptsize 51}$,
S.~Constantinescu$^\textrm{\scriptsize 28b}$,
G.~Conti$^\textrm{\scriptsize 32}$,
F.~Conventi$^\textrm{\scriptsize 106a}$$^{,m}$,
M.~Cooke$^\textrm{\scriptsize 16}$,
B.D.~Cooper$^\textrm{\scriptsize 81}$,
A.M.~Cooper-Sarkar$^\textrm{\scriptsize 122}$,
F.~Cormier$^\textrm{\scriptsize 171}$,
K.J.R.~Cormier$^\textrm{\scriptsize 161}$,
T.~Cornelissen$^\textrm{\scriptsize 178}$,
M.~Corradi$^\textrm{\scriptsize 134a,134b}$,
F.~Corriveau$^\textrm{\scriptsize 90}$$^{,n}$,
A.~Cortes-Gonzalez$^\textrm{\scriptsize 32}$,
G.~Cortiana$^\textrm{\scriptsize 103}$,
G.~Costa$^\textrm{\scriptsize 94a}$,
M.J.~Costa$^\textrm{\scriptsize 170}$,
D.~Costanzo$^\textrm{\scriptsize 141}$,
G.~Cottin$^\textrm{\scriptsize 30}$,
G.~Cowan$^\textrm{\scriptsize 80}$,
B.E.~Cox$^\textrm{\scriptsize 87}$,
K.~Cranmer$^\textrm{\scriptsize 112}$,
S.J.~Crawley$^\textrm{\scriptsize 56}$,
G.~Cree$^\textrm{\scriptsize 31}$,
S.~Cr\'ep\'e-Renaudin$^\textrm{\scriptsize 58}$,
F.~Crescioli$^\textrm{\scriptsize 83}$,
W.A.~Cribbs$^\textrm{\scriptsize 148a,148b}$,
M.~Crispin~Ortuzar$^\textrm{\scriptsize 122}$,
M.~Cristinziani$^\textrm{\scriptsize 23}$,
V.~Croft$^\textrm{\scriptsize 108}$,
G.~Crosetti$^\textrm{\scriptsize 40a,40b}$,
A.~Cueto$^\textrm{\scriptsize 85}$,
T.~Cuhadar~Donszelmann$^\textrm{\scriptsize 141}$,
J.~Cummings$^\textrm{\scriptsize 179}$,
M.~Curatolo$^\textrm{\scriptsize 50}$,
J.~C\'uth$^\textrm{\scriptsize 86}$,
H.~Czirr$^\textrm{\scriptsize 143}$,
P.~Czodrowski$^\textrm{\scriptsize 3}$,
G.~D'amen$^\textrm{\scriptsize 22a,22b}$,
S.~D'Auria$^\textrm{\scriptsize 56}$,
M.~D'Onofrio$^\textrm{\scriptsize 77}$,
M.J.~Da~Cunha~Sargedas~De~Sousa$^\textrm{\scriptsize 128a,128b}$,
C.~Da~Via$^\textrm{\scriptsize 87}$,
W.~Dabrowski$^\textrm{\scriptsize 41a}$,
T.~Dado$^\textrm{\scriptsize 146a}$,
T.~Dai$^\textrm{\scriptsize 92}$,
O.~Dale$^\textrm{\scriptsize 15}$,
F.~Dallaire$^\textrm{\scriptsize 97}$,
C.~Dallapiccola$^\textrm{\scriptsize 89}$,
M.~Dam$^\textrm{\scriptsize 39}$,
J.R.~Dandoy$^\textrm{\scriptsize 33}$,
N.P.~Dang$^\textrm{\scriptsize 51}$,
A.C.~Daniells$^\textrm{\scriptsize 19}$,
N.S.~Dann$^\textrm{\scriptsize 87}$,
M.~Danninger$^\textrm{\scriptsize 171}$,
M.~Dano~Hoffmann$^\textrm{\scriptsize 138}$,
V.~Dao$^\textrm{\scriptsize 51}$,
G.~Darbo$^\textrm{\scriptsize 53a}$,
S.~Darmora$^\textrm{\scriptsize 8}$,
J.~Dassoulas$^\textrm{\scriptsize 3}$,
A.~Dattagupta$^\textrm{\scriptsize 118}$,
W.~Davey$^\textrm{\scriptsize 23}$,
C.~David$^\textrm{\scriptsize 172}$,
T.~Davidek$^\textrm{\scriptsize 131}$,
M.~Davies$^\textrm{\scriptsize 155}$,
P.~Davison$^\textrm{\scriptsize 81}$,
E.~Dawe$^\textrm{\scriptsize 91}$,
I.~Dawson$^\textrm{\scriptsize 141}$,
K.~De$^\textrm{\scriptsize 8}$,
R.~de~Asmundis$^\textrm{\scriptsize 106a}$,
A.~De~Benedetti$^\textrm{\scriptsize 115}$,
S.~De~Castro$^\textrm{\scriptsize 22a,22b}$,
S.~De~Cecco$^\textrm{\scriptsize 83}$,
N.~De~Groot$^\textrm{\scriptsize 108}$,
P.~de~Jong$^\textrm{\scriptsize 109}$,
H.~De~la~Torre$^\textrm{\scriptsize 93}$,
F.~De~Lorenzi$^\textrm{\scriptsize 67}$,
A.~De~Maria$^\textrm{\scriptsize 57}$,
D.~De~Pedis$^\textrm{\scriptsize 134a}$,
A.~De~Salvo$^\textrm{\scriptsize 134a}$,
U.~De~Sanctis$^\textrm{\scriptsize 151}$,
A.~De~Santo$^\textrm{\scriptsize 151}$,
J.B.~De~Vivie~De~Regie$^\textrm{\scriptsize 119}$,
W.J.~Dearnaley$^\textrm{\scriptsize 75}$,
R.~Debbe$^\textrm{\scriptsize 27}$,
C.~Debenedetti$^\textrm{\scriptsize 139}$,
D.V.~Dedovich$^\textrm{\scriptsize 68}$,
N.~Dehghanian$^\textrm{\scriptsize 3}$,
I.~Deigaard$^\textrm{\scriptsize 109}$,
M.~Del~Gaudio$^\textrm{\scriptsize 40a,40b}$,
J.~Del~Peso$^\textrm{\scriptsize 85}$,
T.~Del~Prete$^\textrm{\scriptsize 126a,126b}$,
D.~Delgove$^\textrm{\scriptsize 119}$,
F.~Deliot$^\textrm{\scriptsize 138}$,
C.M.~Delitzsch$^\textrm{\scriptsize 52}$,
A.~Dell'Acqua$^\textrm{\scriptsize 32}$,
L.~Dell'Asta$^\textrm{\scriptsize 24}$,
M.~Dell'Orso$^\textrm{\scriptsize 126a,126b}$,
M.~Della~Pietra$^\textrm{\scriptsize 106a}$$^{,m}$,
D.~della~Volpe$^\textrm{\scriptsize 52}$,
M.~Delmastro$^\textrm{\scriptsize 5}$,
P.A.~Delsart$^\textrm{\scriptsize 58}$,
D.A.~DeMarco$^\textrm{\scriptsize 161}$,
S.~Demers$^\textrm{\scriptsize 179}$,
M.~Demichev$^\textrm{\scriptsize 68}$,
A.~Demilly$^\textrm{\scriptsize 83}$,
S.P.~Denisov$^\textrm{\scriptsize 132}$,
D.~Denysiuk$^\textrm{\scriptsize 138}$,
D.~Derendarz$^\textrm{\scriptsize 42}$,
J.E.~Derkaoui$^\textrm{\scriptsize 137d}$,
F.~Derue$^\textrm{\scriptsize 83}$,
P.~Dervan$^\textrm{\scriptsize 77}$,
K.~Desch$^\textrm{\scriptsize 23}$,
C.~Deterre$^\textrm{\scriptsize 45}$,
K.~Dette$^\textrm{\scriptsize 46}$,
P.O.~Deviveiros$^\textrm{\scriptsize 32}$,
A.~Dewhurst$^\textrm{\scriptsize 133}$,
S.~Dhaliwal$^\textrm{\scriptsize 25}$,
A.~Di~Ciaccio$^\textrm{\scriptsize 135a,135b}$,
L.~Di~Ciaccio$^\textrm{\scriptsize 5}$,
W.K.~Di~Clemente$^\textrm{\scriptsize 124}$,
C.~Di~Donato$^\textrm{\scriptsize 106a,106b}$,
A.~Di~Girolamo$^\textrm{\scriptsize 32}$,
B.~Di~Girolamo$^\textrm{\scriptsize 32}$,
B.~Di~Micco$^\textrm{\scriptsize 136a,136b}$,
R.~Di~Nardo$^\textrm{\scriptsize 32}$,
K.F.~Di~Petrillo$^\textrm{\scriptsize 59}$,
A.~Di~Simone$^\textrm{\scriptsize 51}$,
R.~Di~Sipio$^\textrm{\scriptsize 161}$,
D.~Di~Valentino$^\textrm{\scriptsize 31}$,
C.~Diaconu$^\textrm{\scriptsize 88}$,
M.~Diamond$^\textrm{\scriptsize 161}$,
F.A.~Dias$^\textrm{\scriptsize 49}$,
M.A.~Diaz$^\textrm{\scriptsize 34a}$,
E.B.~Diehl$^\textrm{\scriptsize 92}$,
J.~Dietrich$^\textrm{\scriptsize 17}$,
S.~D\'iez~Cornell$^\textrm{\scriptsize 45}$,
A.~Dimitrievska$^\textrm{\scriptsize 14}$,
J.~Dingfelder$^\textrm{\scriptsize 23}$,
P.~Dita$^\textrm{\scriptsize 28b}$,
S.~Dita$^\textrm{\scriptsize 28b}$,
F.~Dittus$^\textrm{\scriptsize 32}$,
F.~Djama$^\textrm{\scriptsize 88}$,
T.~Djobava$^\textrm{\scriptsize 54b}$,
J.I.~Djuvsland$^\textrm{\scriptsize 60a}$,
M.A.B.~do~Vale$^\textrm{\scriptsize 26c}$,
D.~Dobos$^\textrm{\scriptsize 32}$,
M.~Dobre$^\textrm{\scriptsize 28b}$,
C.~Doglioni$^\textrm{\scriptsize 84}$,
J.~Dolejsi$^\textrm{\scriptsize 131}$,
Z.~Dolezal$^\textrm{\scriptsize 131}$,
M.~Donadelli$^\textrm{\scriptsize 26d}$,
S.~Donati$^\textrm{\scriptsize 126a,126b}$,
P.~Dondero$^\textrm{\scriptsize 123a,123b}$,
J.~Donini$^\textrm{\scriptsize 37}$,
J.~Dopke$^\textrm{\scriptsize 133}$,
A.~Doria$^\textrm{\scriptsize 106a}$,
M.T.~Dova$^\textrm{\scriptsize 74}$,
A.T.~Doyle$^\textrm{\scriptsize 56}$,
E.~Drechsler$^\textrm{\scriptsize 57}$,
M.~Dris$^\textrm{\scriptsize 10}$,
Y.~Du$^\textrm{\scriptsize 36b}$,
J.~Duarte-Campderros$^\textrm{\scriptsize 155}$,
E.~Duchovni$^\textrm{\scriptsize 175}$,
G.~Duckeck$^\textrm{\scriptsize 102}$,
O.A.~Ducu$^\textrm{\scriptsize 97}$$^{,o}$,
D.~Duda$^\textrm{\scriptsize 109}$,
A.~Dudarev$^\textrm{\scriptsize 32}$,
A.Chr.~Dudder$^\textrm{\scriptsize 86}$,
E.M.~Duffield$^\textrm{\scriptsize 16}$,
L.~Duflot$^\textrm{\scriptsize 119}$,
M.~D\"uhrssen$^\textrm{\scriptsize 32}$,
M.~Dumancic$^\textrm{\scriptsize 175}$,
A.K.~Duncan$^\textrm{\scriptsize 56}$,
M.~Dunford$^\textrm{\scriptsize 60a}$,
H.~Duran~Yildiz$^\textrm{\scriptsize 4a}$,
M.~D\"uren$^\textrm{\scriptsize 55}$,
A.~Durglishvili$^\textrm{\scriptsize 54b}$,
D.~Duschinger$^\textrm{\scriptsize 47}$,
B.~Dutta$^\textrm{\scriptsize 45}$,
M.~Dyndal$^\textrm{\scriptsize 45}$,
C.~Eckardt$^\textrm{\scriptsize 45}$,
K.M.~Ecker$^\textrm{\scriptsize 103}$,
R.C.~Edgar$^\textrm{\scriptsize 92}$,
N.C.~Edwards$^\textrm{\scriptsize 49}$,
T.~Eifert$^\textrm{\scriptsize 32}$,
G.~Eigen$^\textrm{\scriptsize 15}$,
K.~Einsweiler$^\textrm{\scriptsize 16}$,
T.~Ekelof$^\textrm{\scriptsize 168}$,
M.~El~Kacimi$^\textrm{\scriptsize 137c}$,
V.~Ellajosyula$^\textrm{\scriptsize 88}$,
M.~Ellert$^\textrm{\scriptsize 168}$,
S.~Elles$^\textrm{\scriptsize 5}$,
F.~Ellinghaus$^\textrm{\scriptsize 178}$,
A.A.~Elliot$^\textrm{\scriptsize 172}$,
N.~Ellis$^\textrm{\scriptsize 32}$,
J.~Elmsheuser$^\textrm{\scriptsize 27}$,
M.~Elsing$^\textrm{\scriptsize 32}$,
D.~Emeliyanov$^\textrm{\scriptsize 133}$,
Y.~Enari$^\textrm{\scriptsize 157}$,
O.C.~Endner$^\textrm{\scriptsize 86}$,
J.S.~Ennis$^\textrm{\scriptsize 173}$,
J.~Erdmann$^\textrm{\scriptsize 46}$,
A.~Ereditato$^\textrm{\scriptsize 18}$,
G.~Ernis$^\textrm{\scriptsize 178}$,
J.~Ernst$^\textrm{\scriptsize 2}$,
M.~Ernst$^\textrm{\scriptsize 27}$,
S.~Errede$^\textrm{\scriptsize 169}$,
E.~Ertel$^\textrm{\scriptsize 86}$,
M.~Escalier$^\textrm{\scriptsize 119}$,
H.~Esch$^\textrm{\scriptsize 46}$,
C.~Escobar$^\textrm{\scriptsize 127}$,
B.~Esposito$^\textrm{\scriptsize 50}$,
A.I.~Etienvre$^\textrm{\scriptsize 138}$,
E.~Etzion$^\textrm{\scriptsize 155}$,
H.~Evans$^\textrm{\scriptsize 64}$,
A.~Ezhilov$^\textrm{\scriptsize 125}$,
F.~Fabbri$^\textrm{\scriptsize 22a,22b}$,
L.~Fabbri$^\textrm{\scriptsize 22a,22b}$,
G.~Facini$^\textrm{\scriptsize 33}$,
R.M.~Fakhrutdinov$^\textrm{\scriptsize 132}$,
S.~Falciano$^\textrm{\scriptsize 134a}$,
R.J.~Falla$^\textrm{\scriptsize 81}$,
J.~Faltova$^\textrm{\scriptsize 32}$,
Y.~Fang$^\textrm{\scriptsize 35a}$,
M.~Fanti$^\textrm{\scriptsize 94a,94b}$,
A.~Farbin$^\textrm{\scriptsize 8}$,
A.~Farilla$^\textrm{\scriptsize 136a}$,
C.~Farina$^\textrm{\scriptsize 127}$,
E.M.~Farina$^\textrm{\scriptsize 123a,123b}$,
T.~Farooque$^\textrm{\scriptsize 13}$,
S.~Farrell$^\textrm{\scriptsize 16}$,
S.M.~Farrington$^\textrm{\scriptsize 173}$,
P.~Farthouat$^\textrm{\scriptsize 32}$,
F.~Fassi$^\textrm{\scriptsize 137e}$,
P.~Fassnacht$^\textrm{\scriptsize 32}$,
D.~Fassouliotis$^\textrm{\scriptsize 9}$,
M.~Faucci~Giannelli$^\textrm{\scriptsize 80}$,
A.~Favareto$^\textrm{\scriptsize 53a,53b}$,
W.J.~Fawcett$^\textrm{\scriptsize 122}$,
L.~Fayard$^\textrm{\scriptsize 119}$,
O.L.~Fedin$^\textrm{\scriptsize 125}$$^{,p}$,
W.~Fedorko$^\textrm{\scriptsize 171}$,
S.~Feigl$^\textrm{\scriptsize 121}$,
L.~Feligioni$^\textrm{\scriptsize 88}$,
C.~Feng$^\textrm{\scriptsize 36b}$,
E.J.~Feng$^\textrm{\scriptsize 32}$,
H.~Feng$^\textrm{\scriptsize 92}$,
A.B.~Fenyuk$^\textrm{\scriptsize 132}$,
L.~Feremenga$^\textrm{\scriptsize 8}$,
P.~Fernandez~Martinez$^\textrm{\scriptsize 170}$,
S.~Fernandez~Perez$^\textrm{\scriptsize 13}$,
J.~Ferrando$^\textrm{\scriptsize 45}$,
A.~Ferrari$^\textrm{\scriptsize 168}$,
P.~Ferrari$^\textrm{\scriptsize 109}$,
R.~Ferrari$^\textrm{\scriptsize 123a}$,
D.E.~Ferreira~de~Lima$^\textrm{\scriptsize 60b}$,
A.~Ferrer$^\textrm{\scriptsize 170}$,
D.~Ferrere$^\textrm{\scriptsize 52}$,
C.~Ferretti$^\textrm{\scriptsize 92}$,
F.~Fiedler$^\textrm{\scriptsize 86}$,
A.~Filip\v{c}i\v{c}$^\textrm{\scriptsize 78}$,
M.~Filipuzzi$^\textrm{\scriptsize 45}$,
F.~Filthaut$^\textrm{\scriptsize 108}$,
M.~Fincke-Keeler$^\textrm{\scriptsize 172}$,
K.D.~Finelli$^\textrm{\scriptsize 152}$,
M.C.N.~Fiolhais$^\textrm{\scriptsize 128a,128c}$,
L.~Fiorini$^\textrm{\scriptsize 170}$,
A.~Fischer$^\textrm{\scriptsize 2}$,
C.~Fischer$^\textrm{\scriptsize 13}$,
J.~Fischer$^\textrm{\scriptsize 178}$,
W.C.~Fisher$^\textrm{\scriptsize 93}$,
N.~Flaschel$^\textrm{\scriptsize 45}$,
I.~Fleck$^\textrm{\scriptsize 143}$,
P.~Fleischmann$^\textrm{\scriptsize 92}$,
G.T.~Fletcher$^\textrm{\scriptsize 141}$,
R.R.M.~Fletcher$^\textrm{\scriptsize 124}$,
T.~Flick$^\textrm{\scriptsize 178}$,
B.M.~Flierl$^\textrm{\scriptsize 102}$,
L.R.~Flores~Castillo$^\textrm{\scriptsize 62a}$,
M.J.~Flowerdew$^\textrm{\scriptsize 103}$,
G.T.~Forcolin$^\textrm{\scriptsize 87}$,
A.~Formica$^\textrm{\scriptsize 138}$,
A.~Forti$^\textrm{\scriptsize 87}$,
A.G.~Foster$^\textrm{\scriptsize 19}$,
D.~Fournier$^\textrm{\scriptsize 119}$,
H.~Fox$^\textrm{\scriptsize 75}$,
S.~Fracchia$^\textrm{\scriptsize 13}$,
P.~Francavilla$^\textrm{\scriptsize 83}$,
M.~Franchini$^\textrm{\scriptsize 22a,22b}$,
D.~Francis$^\textrm{\scriptsize 32}$,
L.~Franconi$^\textrm{\scriptsize 121}$,
M.~Franklin$^\textrm{\scriptsize 59}$,
M.~Frate$^\textrm{\scriptsize 166}$,
M.~Fraternali$^\textrm{\scriptsize 123a,123b}$,
D.~Freeborn$^\textrm{\scriptsize 81}$,
S.M.~Fressard-Batraneanu$^\textrm{\scriptsize 32}$,
F.~Friedrich$^\textrm{\scriptsize 47}$,
D.~Froidevaux$^\textrm{\scriptsize 32}$,
J.A.~Frost$^\textrm{\scriptsize 122}$,
C.~Fukunaga$^\textrm{\scriptsize 158}$,
E.~Fullana~Torregrosa$^\textrm{\scriptsize 86}$,
T.~Fusayasu$^\textrm{\scriptsize 104}$,
J.~Fuster$^\textrm{\scriptsize 170}$,
C.~Gabaldon$^\textrm{\scriptsize 58}$,
O.~Gabizon$^\textrm{\scriptsize 154}$,
A.~Gabrielli$^\textrm{\scriptsize 22a,22b}$,
A.~Gabrielli$^\textrm{\scriptsize 16}$,
G.P.~Gach$^\textrm{\scriptsize 41a}$,
S.~Gadatsch$^\textrm{\scriptsize 32}$,
G.~Gagliardi$^\textrm{\scriptsize 53a,53b}$,
L.G.~Gagnon$^\textrm{\scriptsize 97}$,
P.~Gagnon$^\textrm{\scriptsize 64}$,
C.~Galea$^\textrm{\scriptsize 108}$,
B.~Galhardo$^\textrm{\scriptsize 128a,128c}$,
E.J.~Gallas$^\textrm{\scriptsize 122}$,
B.J.~Gallop$^\textrm{\scriptsize 133}$,
P.~Gallus$^\textrm{\scriptsize 130}$,
G.~Galster$^\textrm{\scriptsize 39}$,
K.K.~Gan$^\textrm{\scriptsize 113}$,
S.~Ganguly$^\textrm{\scriptsize 37}$,
J.~Gao$^\textrm{\scriptsize 36a}$,
Y.~Gao$^\textrm{\scriptsize 49}$,
Y.S.~Gao$^\textrm{\scriptsize 145}$$^{,g}$,
F.M.~Garay~Walls$^\textrm{\scriptsize 49}$,
C.~Garc\'ia$^\textrm{\scriptsize 170}$,
J.E.~Garc\'ia~Navarro$^\textrm{\scriptsize 170}$,
M.~Garcia-Sciveres$^\textrm{\scriptsize 16}$,
R.W.~Gardner$^\textrm{\scriptsize 33}$,
N.~Garelli$^\textrm{\scriptsize 145}$,
V.~Garonne$^\textrm{\scriptsize 121}$,
A.~Gascon~Bravo$^\textrm{\scriptsize 45}$,
K.~Gasnikova$^\textrm{\scriptsize 45}$,
C.~Gatti$^\textrm{\scriptsize 50}$,
A.~Gaudiello$^\textrm{\scriptsize 53a,53b}$,
G.~Gaudio$^\textrm{\scriptsize 123a}$,
L.~Gauthier$^\textrm{\scriptsize 97}$,
I.L.~Gavrilenko$^\textrm{\scriptsize 98}$,
C.~Gay$^\textrm{\scriptsize 171}$,
G.~Gaycken$^\textrm{\scriptsize 23}$,
E.N.~Gazis$^\textrm{\scriptsize 10}$,
Z.~Gecse$^\textrm{\scriptsize 171}$,
C.N.P.~Gee$^\textrm{\scriptsize 133}$,
Ch.~Geich-Gimbel$^\textrm{\scriptsize 23}$,
M.~Geisen$^\textrm{\scriptsize 86}$,
M.P.~Geisler$^\textrm{\scriptsize 60a}$,
K.~Gellerstedt$^\textrm{\scriptsize 148a,148b}$,
C.~Gemme$^\textrm{\scriptsize 53a}$,
M.H.~Genest$^\textrm{\scriptsize 58}$,
C.~Geng$^\textrm{\scriptsize 36a}$$^{,q}$,
S.~Gentile$^\textrm{\scriptsize 134a,134b}$,
C.~Gentsos$^\textrm{\scriptsize 156}$,
S.~George$^\textrm{\scriptsize 80}$,
D.~Gerbaudo$^\textrm{\scriptsize 13}$,
A.~Gershon$^\textrm{\scriptsize 155}$,
S.~Ghasemi$^\textrm{\scriptsize 143}$,
M.~Ghneimat$^\textrm{\scriptsize 23}$,
B.~Giacobbe$^\textrm{\scriptsize 22a}$,
S.~Giagu$^\textrm{\scriptsize 134a,134b}$,
P.~Giannetti$^\textrm{\scriptsize 126a,126b}$,
S.M.~Gibson$^\textrm{\scriptsize 80}$,
M.~Gignac$^\textrm{\scriptsize 171}$,
M.~Gilchriese$^\textrm{\scriptsize 16}$,
T.P.S.~Gillam$^\textrm{\scriptsize 30}$,
D.~Gillberg$^\textrm{\scriptsize 31}$,
G.~Gilles$^\textrm{\scriptsize 178}$,
D.M.~Gingrich$^\textrm{\scriptsize 3}$$^{,d}$,
N.~Giokaris$^\textrm{\scriptsize 9}$$^{,*}$,
M.P.~Giordani$^\textrm{\scriptsize 167a,167c}$,
F.M.~Giorgi$^\textrm{\scriptsize 22a}$,
P.F.~Giraud$^\textrm{\scriptsize 138}$,
P.~Giromini$^\textrm{\scriptsize 59}$,
D.~Giugni$^\textrm{\scriptsize 94a}$,
F.~Giuli$^\textrm{\scriptsize 122}$,
C.~Giuliani$^\textrm{\scriptsize 103}$,
M.~Giulini$^\textrm{\scriptsize 60b}$,
B.K.~Gjelsten$^\textrm{\scriptsize 121}$,
S.~Gkaitatzis$^\textrm{\scriptsize 156}$,
I.~Gkialas$^\textrm{\scriptsize 9}$,
E.L.~Gkougkousis$^\textrm{\scriptsize 119}$,
L.K.~Gladilin$^\textrm{\scriptsize 101}$,
C.~Glasman$^\textrm{\scriptsize 85}$,
J.~Glatzer$^\textrm{\scriptsize 13}$,
P.C.F.~Glaysher$^\textrm{\scriptsize 49}$,
A.~Glazov$^\textrm{\scriptsize 45}$,
M.~Goblirsch-Kolb$^\textrm{\scriptsize 25}$,
J.~Godlewski$^\textrm{\scriptsize 42}$,
S.~Goldfarb$^\textrm{\scriptsize 91}$,
T.~Golling$^\textrm{\scriptsize 52}$,
D.~Golubkov$^\textrm{\scriptsize 132}$,
A.~Gomes$^\textrm{\scriptsize 128a,128b,128d}$,
R.~Gon\c{c}alo$^\textrm{\scriptsize 128a}$,
J.~Goncalves~Pinto~Firmino~Da~Costa$^\textrm{\scriptsize 138}$,
G.~Gonella$^\textrm{\scriptsize 51}$,
L.~Gonella$^\textrm{\scriptsize 19}$,
A.~Gongadze$^\textrm{\scriptsize 68}$,
S.~Gonz\'alez~de~la~Hoz$^\textrm{\scriptsize 170}$,
S.~Gonzalez-Sevilla$^\textrm{\scriptsize 52}$,
L.~Goossens$^\textrm{\scriptsize 32}$,
P.A.~Gorbounov$^\textrm{\scriptsize 99}$,
H.A.~Gordon$^\textrm{\scriptsize 27}$,
I.~Gorelov$^\textrm{\scriptsize 107}$,
B.~Gorini$^\textrm{\scriptsize 32}$,
E.~Gorini$^\textrm{\scriptsize 76a,76b}$,
A.~Gori\v{s}ek$^\textrm{\scriptsize 78}$,
E.~Gornicki$^\textrm{\scriptsize 42}$,
A.T.~Goshaw$^\textrm{\scriptsize 48}$,
C.~G\"ossling$^\textrm{\scriptsize 46}$,
M.I.~Gostkin$^\textrm{\scriptsize 68}$,
C.R.~Goudet$^\textrm{\scriptsize 119}$,
D.~Goujdami$^\textrm{\scriptsize 137c}$,
A.G.~Goussiou$^\textrm{\scriptsize 140}$,
N.~Govender$^\textrm{\scriptsize 147b}$$^{,r}$,
E.~Gozani$^\textrm{\scriptsize 154}$,
L.~Graber$^\textrm{\scriptsize 57}$,
I.~Grabowska-Bold$^\textrm{\scriptsize 41a}$,
P.O.J.~Gradin$^\textrm{\scriptsize 58}$,
P.~Grafstr\"om$^\textrm{\scriptsize 22a,22b}$,
J.~Gramling$^\textrm{\scriptsize 52}$,
E.~Gramstad$^\textrm{\scriptsize 121}$,
S.~Grancagnolo$^\textrm{\scriptsize 17}$,
V.~Gratchev$^\textrm{\scriptsize 125}$,
P.M.~Gravila$^\textrm{\scriptsize 28e}$,
H.M.~Gray$^\textrm{\scriptsize 32}$,
E.~Graziani$^\textrm{\scriptsize 136a}$,
Z.D.~Greenwood$^\textrm{\scriptsize 82}$$^{,s}$,
C.~Grefe$^\textrm{\scriptsize 23}$,
K.~Gregersen$^\textrm{\scriptsize 81}$,
I.M.~Gregor$^\textrm{\scriptsize 45}$,
P.~Grenier$^\textrm{\scriptsize 145}$,
K.~Grevtsov$^\textrm{\scriptsize 5}$,
J.~Griffiths$^\textrm{\scriptsize 8}$,
A.A.~Grillo$^\textrm{\scriptsize 139}$,
K.~Grimm$^\textrm{\scriptsize 75}$,
S.~Grinstein$^\textrm{\scriptsize 13}$$^{,t}$,
Ph.~Gris$^\textrm{\scriptsize 37}$,
J.-F.~Grivaz$^\textrm{\scriptsize 119}$,
S.~Groh$^\textrm{\scriptsize 86}$,
E.~Gross$^\textrm{\scriptsize 175}$,
J.~Grosse-Knetter$^\textrm{\scriptsize 57}$,
G.C.~Grossi$^\textrm{\scriptsize 82}$,
Z.J.~Grout$^\textrm{\scriptsize 81}$,
L.~Guan$^\textrm{\scriptsize 92}$,
W.~Guan$^\textrm{\scriptsize 176}$,
J.~Guenther$^\textrm{\scriptsize 65}$,
F.~Guescini$^\textrm{\scriptsize 52}$,
D.~Guest$^\textrm{\scriptsize 166}$,
O.~Gueta$^\textrm{\scriptsize 155}$,
B.~Gui$^\textrm{\scriptsize 113}$,
E.~Guido$^\textrm{\scriptsize 53a,53b}$,
T.~Guillemin$^\textrm{\scriptsize 5}$,
S.~Guindon$^\textrm{\scriptsize 2}$,
U.~Gul$^\textrm{\scriptsize 56}$,
C.~Gumpert$^\textrm{\scriptsize 32}$,
J.~Guo$^\textrm{\scriptsize 36c}$,
Y.~Guo$^\textrm{\scriptsize 36a}$$^{,q}$,
R.~Gupta$^\textrm{\scriptsize 43}$,
S.~Gupta$^\textrm{\scriptsize 122}$,
G.~Gustavino$^\textrm{\scriptsize 134a,134b}$,
P.~Gutierrez$^\textrm{\scriptsize 115}$,
N.G.~Gutierrez~Ortiz$^\textrm{\scriptsize 81}$,
C.~Gutschow$^\textrm{\scriptsize 81}$,
C.~Guyot$^\textrm{\scriptsize 138}$,
C.~Gwenlan$^\textrm{\scriptsize 122}$,
C.B.~Gwilliam$^\textrm{\scriptsize 77}$,
A.~Haas$^\textrm{\scriptsize 112}$,
C.~Haber$^\textrm{\scriptsize 16}$,
H.K.~Hadavand$^\textrm{\scriptsize 8}$,
A.~Hadef$^\textrm{\scriptsize 88}$,
S.~Hageb\"ock$^\textrm{\scriptsize 23}$,
M.~Hagihara$^\textrm{\scriptsize 164}$,
Z.~Hajduk$^\textrm{\scriptsize 42}$,
H.~Hakobyan$^\textrm{\scriptsize 180}$$^{,*}$,
M.~Haleem$^\textrm{\scriptsize 45}$,
J.~Haley$^\textrm{\scriptsize 116}$,
G.~Halladjian$^\textrm{\scriptsize 93}$,
G.D.~Hallewell$^\textrm{\scriptsize 88}$,
K.~Hamacher$^\textrm{\scriptsize 178}$,
P.~Hamal$^\textrm{\scriptsize 117}$,
K.~Hamano$^\textrm{\scriptsize 172}$,
A.~Hamilton$^\textrm{\scriptsize 147a}$,
G.N.~Hamity$^\textrm{\scriptsize 141}$,
P.G.~Hamnett$^\textrm{\scriptsize 45}$,
L.~Han$^\textrm{\scriptsize 36a}$,
K.~Hanagaki$^\textrm{\scriptsize 69}$$^{,u}$,
K.~Hanawa$^\textrm{\scriptsize 157}$,
M.~Hance$^\textrm{\scriptsize 139}$,
B.~Haney$^\textrm{\scriptsize 124}$,
P.~Hanke$^\textrm{\scriptsize 60a}$,
R.~Hanna$^\textrm{\scriptsize 138}$,
J.B.~Hansen$^\textrm{\scriptsize 39}$,
J.D.~Hansen$^\textrm{\scriptsize 39}$,
M.C.~Hansen$^\textrm{\scriptsize 23}$,
P.H.~Hansen$^\textrm{\scriptsize 39}$,
K.~Hara$^\textrm{\scriptsize 164}$,
A.S.~Hard$^\textrm{\scriptsize 176}$,
T.~Harenberg$^\textrm{\scriptsize 178}$,
F.~Hariri$^\textrm{\scriptsize 119}$,
S.~Harkusha$^\textrm{\scriptsize 95}$,
R.D.~Harrington$^\textrm{\scriptsize 49}$,
P.F.~Harrison$^\textrm{\scriptsize 173}$,
F.~Hartjes$^\textrm{\scriptsize 109}$,
N.M.~Hartmann$^\textrm{\scriptsize 102}$,
M.~Hasegawa$^\textrm{\scriptsize 70}$,
Y.~Hasegawa$^\textrm{\scriptsize 142}$,
A.~Hasib$^\textrm{\scriptsize 115}$,
S.~Hassani$^\textrm{\scriptsize 138}$,
S.~Haug$^\textrm{\scriptsize 18}$,
R.~Hauser$^\textrm{\scriptsize 93}$,
L.~Hauswald$^\textrm{\scriptsize 47}$,
M.~Havranek$^\textrm{\scriptsize 129}$,
C.M.~Hawkes$^\textrm{\scriptsize 19}$,
R.J.~Hawkings$^\textrm{\scriptsize 32}$,
D.~Hayakawa$^\textrm{\scriptsize 159}$,
D.~Hayden$^\textrm{\scriptsize 93}$,
C.P.~Hays$^\textrm{\scriptsize 122}$,
J.M.~Hays$^\textrm{\scriptsize 79}$,
H.S.~Hayward$^\textrm{\scriptsize 77}$,
S.J.~Haywood$^\textrm{\scriptsize 133}$,
S.J.~Head$^\textrm{\scriptsize 19}$,
T.~Heck$^\textrm{\scriptsize 86}$,
V.~Hedberg$^\textrm{\scriptsize 84}$,
L.~Heelan$^\textrm{\scriptsize 8}$,
S.~Heim$^\textrm{\scriptsize 124}$,
T.~Heim$^\textrm{\scriptsize 16}$,
B.~Heinemann$^\textrm{\scriptsize 16}$,
J.J.~Heinrich$^\textrm{\scriptsize 102}$,
L.~Heinrich$^\textrm{\scriptsize 112}$,
C.~Heinz$^\textrm{\scriptsize 55}$,
J.~Hejbal$^\textrm{\scriptsize 129}$,
L.~Helary$^\textrm{\scriptsize 32}$,
S.~Hellman$^\textrm{\scriptsize 148a,148b}$,
C.~Helsens$^\textrm{\scriptsize 32}$,
J.~Henderson$^\textrm{\scriptsize 122}$,
R.C.W.~Henderson$^\textrm{\scriptsize 75}$,
Y.~Heng$^\textrm{\scriptsize 176}$,
S.~Henkelmann$^\textrm{\scriptsize 171}$,
A.M.~Henriques~Correia$^\textrm{\scriptsize 32}$,
S.~Henrot-Versille$^\textrm{\scriptsize 119}$,
G.H.~Herbert$^\textrm{\scriptsize 17}$,
H.~Herde$^\textrm{\scriptsize 25}$,
V.~Herget$^\textrm{\scriptsize 177}$,
Y.~Hern\'andez~Jim\'enez$^\textrm{\scriptsize 147c}$,
G.~Herten$^\textrm{\scriptsize 51}$,
R.~Hertenberger$^\textrm{\scriptsize 102}$,
L.~Hervas$^\textrm{\scriptsize 32}$,
G.G.~Hesketh$^\textrm{\scriptsize 81}$,
N.P.~Hessey$^\textrm{\scriptsize 109}$,
J.W.~Hetherly$^\textrm{\scriptsize 43}$,
E.~Hig\'on-Rodriguez$^\textrm{\scriptsize 170}$,
E.~Hill$^\textrm{\scriptsize 172}$,
J.C.~Hill$^\textrm{\scriptsize 30}$,
K.H.~Hiller$^\textrm{\scriptsize 45}$,
S.J.~Hillier$^\textrm{\scriptsize 19}$,
I.~Hinchliffe$^\textrm{\scriptsize 16}$,
E.~Hines$^\textrm{\scriptsize 124}$,
R.R.~Hinman$^\textrm{\scriptsize 16}$,
M.~Hirose$^\textrm{\scriptsize 51}$,
D.~Hirschbuehl$^\textrm{\scriptsize 178}$,
X.~Hoad$^\textrm{\scriptsize 49}$,
J.~Hobbs$^\textrm{\scriptsize 150}$,
N.~Hod$^\textrm{\scriptsize 163a}$,
M.C.~Hodgkinson$^\textrm{\scriptsize 141}$,
P.~Hodgson$^\textrm{\scriptsize 141}$,
A.~Hoecker$^\textrm{\scriptsize 32}$,
M.R.~Hoeferkamp$^\textrm{\scriptsize 107}$,
F.~Hoenig$^\textrm{\scriptsize 102}$,
D.~Hohn$^\textrm{\scriptsize 23}$,
T.R.~Holmes$^\textrm{\scriptsize 16}$,
M.~Homann$^\textrm{\scriptsize 46}$,
T.~Honda$^\textrm{\scriptsize 69}$,
T.M.~Hong$^\textrm{\scriptsize 127}$,
B.H.~Hooberman$^\textrm{\scriptsize 169}$,
W.H.~Hopkins$^\textrm{\scriptsize 118}$,
Y.~Horii$^\textrm{\scriptsize 105}$,
A.J.~Horton$^\textrm{\scriptsize 144}$,
J-Y.~Hostachy$^\textrm{\scriptsize 58}$,
S.~Hou$^\textrm{\scriptsize 153}$,
A.~Hoummada$^\textrm{\scriptsize 137a}$,
J.~Howarth$^\textrm{\scriptsize 45}$,
J.~Hoya$^\textrm{\scriptsize 74}$,
M.~Hrabovsky$^\textrm{\scriptsize 117}$,
I.~Hristova$^\textrm{\scriptsize 17}$,
J.~Hrivnac$^\textrm{\scriptsize 119}$,
T.~Hryn'ova$^\textrm{\scriptsize 5}$,
A.~Hrynevich$^\textrm{\scriptsize 96}$,
P.J.~Hsu$^\textrm{\scriptsize 63}$,
S.-C.~Hsu$^\textrm{\scriptsize 140}$,
Q.~Hu$^\textrm{\scriptsize 36a}$,
S.~Hu$^\textrm{\scriptsize 36c}$,
Y.~Huang$^\textrm{\scriptsize 45}$,
Z.~Hubacek$^\textrm{\scriptsize 130}$,
F.~Hubaut$^\textrm{\scriptsize 88}$,
F.~Huegging$^\textrm{\scriptsize 23}$,
T.B.~Huffman$^\textrm{\scriptsize 122}$,
E.W.~Hughes$^\textrm{\scriptsize 38}$,
G.~Hughes$^\textrm{\scriptsize 75}$,
M.~Huhtinen$^\textrm{\scriptsize 32}$,
P.~Huo$^\textrm{\scriptsize 150}$,
N.~Huseynov$^\textrm{\scriptsize 68}$$^{,b}$,
J.~Huston$^\textrm{\scriptsize 93}$,
J.~Huth$^\textrm{\scriptsize 59}$,
G.~Iacobucci$^\textrm{\scriptsize 52}$,
G.~Iakovidis$^\textrm{\scriptsize 27}$,
I.~Ibragimov$^\textrm{\scriptsize 143}$,
L.~Iconomidou-Fayard$^\textrm{\scriptsize 119}$,
E.~Ideal$^\textrm{\scriptsize 179}$,
P.~Iengo$^\textrm{\scriptsize 32}$,
O.~Igonkina$^\textrm{\scriptsize 109}$$^{,v}$,
T.~Iizawa$^\textrm{\scriptsize 174}$,
Y.~Ikegami$^\textrm{\scriptsize 69}$,
M.~Ikeno$^\textrm{\scriptsize 69}$,
Y.~Ilchenko$^\textrm{\scriptsize 11}$$^{,w}$,
D.~Iliadis$^\textrm{\scriptsize 156}$,
N.~Ilic$^\textrm{\scriptsize 145}$,
G.~Introzzi$^\textrm{\scriptsize 123a,123b}$,
P.~Ioannou$^\textrm{\scriptsize 9}$$^{,*}$,
M.~Iodice$^\textrm{\scriptsize 136a}$,
K.~Iordanidou$^\textrm{\scriptsize 38}$,
V.~Ippolito$^\textrm{\scriptsize 59}$,
N.~Ishijima$^\textrm{\scriptsize 120}$,
M.~Ishino$^\textrm{\scriptsize 157}$,
M.~Ishitsuka$^\textrm{\scriptsize 159}$,
R.~Ishmukhametov$^\textrm{\scriptsize 113}$,
C.~Issever$^\textrm{\scriptsize 122}$,
S.~Istin$^\textrm{\scriptsize 20a}$,
F.~Ito$^\textrm{\scriptsize 164}$,
J.M.~Iturbe~Ponce$^\textrm{\scriptsize 87}$,
R.~Iuppa$^\textrm{\scriptsize 162a,162b}$,
W.~Iwanski$^\textrm{\scriptsize 65}$,
H.~Iwasaki$^\textrm{\scriptsize 69}$,
J.M.~Izen$^\textrm{\scriptsize 44}$,
V.~Izzo$^\textrm{\scriptsize 106a}$,
S.~Jabbar$^\textrm{\scriptsize 3}$,
B.~Jackson$^\textrm{\scriptsize 124}$,
P.~Jackson$^\textrm{\scriptsize 1}$,
V.~Jain$^\textrm{\scriptsize 2}$,
K.B.~Jakobi$^\textrm{\scriptsize 86}$,
K.~Jakobs$^\textrm{\scriptsize 51}$,
S.~Jakobsen$^\textrm{\scriptsize 32}$,
T.~Jakoubek$^\textrm{\scriptsize 129}$,
D.O.~Jamin$^\textrm{\scriptsize 116}$,
D.K.~Jana$^\textrm{\scriptsize 82}$,
R.~Jansky$^\textrm{\scriptsize 65}$,
J.~Janssen$^\textrm{\scriptsize 23}$,
M.~Janus$^\textrm{\scriptsize 57}$,
P.A.~Janus$^\textrm{\scriptsize 41a}$,
G.~Jarlskog$^\textrm{\scriptsize 84}$,
N.~Javadov$^\textrm{\scriptsize 68}$$^{,b}$,
T.~Jav\r{u}rek$^\textrm{\scriptsize 51}$,
M.~Javurkova$^\textrm{\scriptsize 51}$,
F.~Jeanneau$^\textrm{\scriptsize 138}$,
L.~Jeanty$^\textrm{\scriptsize 16}$,
J.~Jejelava$^\textrm{\scriptsize 54a}$$^{,x}$,
G.-Y.~Jeng$^\textrm{\scriptsize 152}$,
D.~Jennens$^\textrm{\scriptsize 91}$,
P.~Jenni$^\textrm{\scriptsize 51}$$^{,y}$,
C.~Jeske$^\textrm{\scriptsize 173}$,
S.~J\'ez\'equel$^\textrm{\scriptsize 5}$,
H.~Ji$^\textrm{\scriptsize 176}$,
J.~Jia$^\textrm{\scriptsize 150}$,
H.~Jiang$^\textrm{\scriptsize 67}$,
Y.~Jiang$^\textrm{\scriptsize 36a}$,
Z.~Jiang$^\textrm{\scriptsize 145}$,
S.~Jiggins$^\textrm{\scriptsize 81}$,
J.~Jimenez~Pena$^\textrm{\scriptsize 170}$,
S.~Jin$^\textrm{\scriptsize 35a}$,
A.~Jinaru$^\textrm{\scriptsize 28b}$,
O.~Jinnouchi$^\textrm{\scriptsize 159}$,
H.~Jivan$^\textrm{\scriptsize 147c}$,
P.~Johansson$^\textrm{\scriptsize 141}$,
K.A.~Johns$^\textrm{\scriptsize 7}$,
W.J.~Johnson$^\textrm{\scriptsize 140}$,
K.~Jon-And$^\textrm{\scriptsize 148a,148b}$,
G.~Jones$^\textrm{\scriptsize 173}$,
R.W.L.~Jones$^\textrm{\scriptsize 75}$,
S.~Jones$^\textrm{\scriptsize 7}$,
T.J.~Jones$^\textrm{\scriptsize 77}$,
J.~Jongmanns$^\textrm{\scriptsize 60a}$,
P.M.~Jorge$^\textrm{\scriptsize 128a,128b}$,
J.~Jovicevic$^\textrm{\scriptsize 163a}$,
X.~Ju$^\textrm{\scriptsize 176}$,
A.~Juste~Rozas$^\textrm{\scriptsize 13}$$^{,t}$,
M.K.~K\"{o}hler$^\textrm{\scriptsize 175}$,
A.~Kaczmarska$^\textrm{\scriptsize 42}$,
M.~Kado$^\textrm{\scriptsize 119}$,
H.~Kagan$^\textrm{\scriptsize 113}$,
M.~Kagan$^\textrm{\scriptsize 145}$,
S.J.~Kahn$^\textrm{\scriptsize 88}$,
T.~Kaji$^\textrm{\scriptsize 174}$,
E.~Kajomovitz$^\textrm{\scriptsize 48}$,
C.W.~Kalderon$^\textrm{\scriptsize 122}$,
A.~Kaluza$^\textrm{\scriptsize 86}$,
S.~Kama$^\textrm{\scriptsize 43}$,
A.~Kamenshchikov$^\textrm{\scriptsize 132}$,
N.~Kanaya$^\textrm{\scriptsize 157}$,
S.~Kaneti$^\textrm{\scriptsize 30}$,
L.~Kanjir$^\textrm{\scriptsize 78}$,
V.A.~Kantserov$^\textrm{\scriptsize 100}$,
J.~Kanzaki$^\textrm{\scriptsize 69}$,
B.~Kaplan$^\textrm{\scriptsize 112}$,
L.S.~Kaplan$^\textrm{\scriptsize 176}$,
A.~Kapliy$^\textrm{\scriptsize 33}$,
D.~Kar$^\textrm{\scriptsize 147c}$,
K.~Karakostas$^\textrm{\scriptsize 10}$,
A.~Karamaoun$^\textrm{\scriptsize 3}$,
N.~Karastathis$^\textrm{\scriptsize 10}$,
M.J.~Kareem$^\textrm{\scriptsize 57}$,
E.~Karentzos$^\textrm{\scriptsize 10}$,
M.~Karnevskiy$^\textrm{\scriptsize 86}$,
S.N.~Karpov$^\textrm{\scriptsize 68}$,
Z.M.~Karpova$^\textrm{\scriptsize 68}$,
K.~Karthik$^\textrm{\scriptsize 112}$,
V.~Kartvelishvili$^\textrm{\scriptsize 75}$,
A.N.~Karyukhin$^\textrm{\scriptsize 132}$,
K.~Kasahara$^\textrm{\scriptsize 164}$,
L.~Kashif$^\textrm{\scriptsize 176}$,
R.D.~Kass$^\textrm{\scriptsize 113}$,
A.~Kastanas$^\textrm{\scriptsize 149}$,
Y.~Kataoka$^\textrm{\scriptsize 157}$,
C.~Kato$^\textrm{\scriptsize 157}$,
A.~Katre$^\textrm{\scriptsize 52}$,
J.~Katzy$^\textrm{\scriptsize 45}$,
K.~Kawade$^\textrm{\scriptsize 105}$,
K.~Kawagoe$^\textrm{\scriptsize 73}$,
T.~Kawamoto$^\textrm{\scriptsize 157}$,
G.~Kawamura$^\textrm{\scriptsize 57}$,
V.F.~Kazanin$^\textrm{\scriptsize 111}$$^{,c}$,
R.~Keeler$^\textrm{\scriptsize 172}$,
R.~Kehoe$^\textrm{\scriptsize 43}$,
J.S.~Keller$^\textrm{\scriptsize 45}$,
J.J.~Kempster$^\textrm{\scriptsize 80}$,
H.~Keoshkerian$^\textrm{\scriptsize 161}$,
O.~Kepka$^\textrm{\scriptsize 129}$,
B.P.~Ker\v{s}evan$^\textrm{\scriptsize 78}$,
S.~Kersten$^\textrm{\scriptsize 178}$,
R.A.~Keyes$^\textrm{\scriptsize 90}$,
M.~Khader$^\textrm{\scriptsize 169}$,
F.~Khalil-zada$^\textrm{\scriptsize 12}$,
A.~Khanov$^\textrm{\scriptsize 116}$,
A.G.~Kharlamov$^\textrm{\scriptsize 111}$$^{,c}$,
T.~Kharlamova$^\textrm{\scriptsize 111}$$^{,c}$,
T.J.~Khoo$^\textrm{\scriptsize 52}$,
V.~Khovanskiy$^\textrm{\scriptsize 99}$,
E.~Khramov$^\textrm{\scriptsize 68}$,
J.~Khubua$^\textrm{\scriptsize 54b}$$^{,z}$,
S.~Kido$^\textrm{\scriptsize 70}$,
C.R.~Kilby$^\textrm{\scriptsize 80}$,
H.Y.~Kim$^\textrm{\scriptsize 8}$,
S.H.~Kim$^\textrm{\scriptsize 164}$,
Y.K.~Kim$^\textrm{\scriptsize 33}$,
N.~Kimura$^\textrm{\scriptsize 156}$,
O.M.~Kind$^\textrm{\scriptsize 17}$,
B.T.~King$^\textrm{\scriptsize 77}$,
M.~King$^\textrm{\scriptsize 170}$,
J.~Kirk$^\textrm{\scriptsize 133}$,
A.E.~Kiryunin$^\textrm{\scriptsize 103}$,
T.~Kishimoto$^\textrm{\scriptsize 157}$,
D.~Kisielewska$^\textrm{\scriptsize 41a}$,
F.~Kiss$^\textrm{\scriptsize 51}$,
K.~Kiuchi$^\textrm{\scriptsize 164}$,
O.~Kivernyk$^\textrm{\scriptsize 138}$,
E.~Kladiva$^\textrm{\scriptsize 146b}$,
M.H.~Klein$^\textrm{\scriptsize 38}$,
M.~Klein$^\textrm{\scriptsize 77}$,
U.~Klein$^\textrm{\scriptsize 77}$,
K.~Kleinknecht$^\textrm{\scriptsize 86}$,
P.~Klimek$^\textrm{\scriptsize 110}$,
A.~Klimentov$^\textrm{\scriptsize 27}$,
R.~Klingenberg$^\textrm{\scriptsize 46}$,
T.~Klioutchnikova$^\textrm{\scriptsize 32}$,
E.-E.~Kluge$^\textrm{\scriptsize 60a}$,
P.~Kluit$^\textrm{\scriptsize 109}$,
S.~Kluth$^\textrm{\scriptsize 103}$,
J.~Knapik$^\textrm{\scriptsize 42}$,
E.~Kneringer$^\textrm{\scriptsize 65}$,
E.B.F.G.~Knoops$^\textrm{\scriptsize 88}$,
A.~Knue$^\textrm{\scriptsize 103}$,
A.~Kobayashi$^\textrm{\scriptsize 157}$,
D.~Kobayashi$^\textrm{\scriptsize 159}$,
T.~Kobayashi$^\textrm{\scriptsize 157}$,
M.~Kobel$^\textrm{\scriptsize 47}$,
M.~Kocian$^\textrm{\scriptsize 145}$,
P.~Kodys$^\textrm{\scriptsize 131}$,
T.~Koffas$^\textrm{\scriptsize 31}$,
E.~Koffeman$^\textrm{\scriptsize 109}$,
N.M.~K\"ohler$^\textrm{\scriptsize 103}$,
T.~Koi$^\textrm{\scriptsize 145}$,
H.~Kolanoski$^\textrm{\scriptsize 17}$,
M.~Kolb$^\textrm{\scriptsize 60b}$,
I.~Koletsou$^\textrm{\scriptsize 5}$,
A.A.~Komar$^\textrm{\scriptsize 98}$$^{,*}$,
Y.~Komori$^\textrm{\scriptsize 157}$,
T.~Kondo$^\textrm{\scriptsize 69}$,
N.~Kondrashova$^\textrm{\scriptsize 36c}$,
K.~K\"oneke$^\textrm{\scriptsize 51}$,
A.C.~K\"onig$^\textrm{\scriptsize 108}$,
T.~Kono$^\textrm{\scriptsize 69}$$^{,aa}$,
R.~Konoplich$^\textrm{\scriptsize 112}$$^{,ab}$,
N.~Konstantinidis$^\textrm{\scriptsize 81}$,
R.~Kopeliansky$^\textrm{\scriptsize 64}$,
S.~Koperny$^\textrm{\scriptsize 41a}$,
L.~K\"opke$^\textrm{\scriptsize 86}$,
A.K.~Kopp$^\textrm{\scriptsize 51}$,
K.~Korcyl$^\textrm{\scriptsize 42}$,
K.~Kordas$^\textrm{\scriptsize 156}$,
A.~Korn$^\textrm{\scriptsize 81}$,
A.A.~Korol$^\textrm{\scriptsize 111}$$^{,c}$,
I.~Korolkov$^\textrm{\scriptsize 13}$,
E.V.~Korolkova$^\textrm{\scriptsize 141}$,
O.~Kortner$^\textrm{\scriptsize 103}$,
S.~Kortner$^\textrm{\scriptsize 103}$,
T.~Kosek$^\textrm{\scriptsize 131}$,
V.V.~Kostyukhin$^\textrm{\scriptsize 23}$,
A.~Kotwal$^\textrm{\scriptsize 48}$,
A.~Koulouris$^\textrm{\scriptsize 10}$,
A.~Kourkoumeli-Charalampidi$^\textrm{\scriptsize 123a,123b}$,
C.~Kourkoumelis$^\textrm{\scriptsize 9}$,
V.~Kouskoura$^\textrm{\scriptsize 27}$,
A.B.~Kowalewska$^\textrm{\scriptsize 42}$,
R.~Kowalewski$^\textrm{\scriptsize 172}$,
T.Z.~Kowalski$^\textrm{\scriptsize 41a}$,
C.~Kozakai$^\textrm{\scriptsize 157}$,
W.~Kozanecki$^\textrm{\scriptsize 138}$,
A.S.~Kozhin$^\textrm{\scriptsize 132}$,
V.A.~Kramarenko$^\textrm{\scriptsize 101}$,
G.~Kramberger$^\textrm{\scriptsize 78}$,
D.~Krasnopevtsev$^\textrm{\scriptsize 100}$,
M.W.~Krasny$^\textrm{\scriptsize 83}$,
A.~Krasznahorkay$^\textrm{\scriptsize 32}$,
A.~Kravchenko$^\textrm{\scriptsize 27}$,
M.~Kretz$^\textrm{\scriptsize 60c}$,
J.~Kretzschmar$^\textrm{\scriptsize 77}$,
K.~Kreutzfeldt$^\textrm{\scriptsize 55}$,
P.~Krieger$^\textrm{\scriptsize 161}$,
K.~Krizka$^\textrm{\scriptsize 33}$,
K.~Kroeninger$^\textrm{\scriptsize 46}$,
H.~Kroha$^\textrm{\scriptsize 103}$,
J.~Kroll$^\textrm{\scriptsize 124}$,
J.~Kroseberg$^\textrm{\scriptsize 23}$,
J.~Krstic$^\textrm{\scriptsize 14}$,
U.~Kruchonak$^\textrm{\scriptsize 68}$,
H.~Kr\"uger$^\textrm{\scriptsize 23}$,
N.~Krumnack$^\textrm{\scriptsize 67}$,
M.C.~Kruse$^\textrm{\scriptsize 48}$,
M.~Kruskal$^\textrm{\scriptsize 24}$,
T.~Kubota$^\textrm{\scriptsize 91}$,
H.~Kucuk$^\textrm{\scriptsize 81}$,
S.~Kuday$^\textrm{\scriptsize 4b}$,
J.T.~Kuechler$^\textrm{\scriptsize 178}$,
S.~Kuehn$^\textrm{\scriptsize 51}$,
A.~Kugel$^\textrm{\scriptsize 60c}$,
F.~Kuger$^\textrm{\scriptsize 177}$,
T.~Kuhl$^\textrm{\scriptsize 45}$,
V.~Kukhtin$^\textrm{\scriptsize 68}$,
R.~Kukla$^\textrm{\scriptsize 138}$,
Y.~Kulchitsky$^\textrm{\scriptsize 95}$,
S.~Kuleshov$^\textrm{\scriptsize 34b}$,
M.~Kuna$^\textrm{\scriptsize 134a,134b}$,
T.~Kunigo$^\textrm{\scriptsize 71}$,
A.~Kupco$^\textrm{\scriptsize 129}$,
H.~Kurashige$^\textrm{\scriptsize 70}$,
L.L.~Kurchaninov$^\textrm{\scriptsize 163a}$,
Y.A.~Kurochkin$^\textrm{\scriptsize 95}$,
M.G.~Kurth$^\textrm{\scriptsize 44}$,
V.~Kus$^\textrm{\scriptsize 129}$,
E.S.~Kuwertz$^\textrm{\scriptsize 172}$,
M.~Kuze$^\textrm{\scriptsize 159}$,
J.~Kvita$^\textrm{\scriptsize 117}$,
T.~Kwan$^\textrm{\scriptsize 172}$,
D.~Kyriazopoulos$^\textrm{\scriptsize 141}$,
A.~La~Rosa$^\textrm{\scriptsize 103}$,
J.L.~La~Rosa~Navarro$^\textrm{\scriptsize 26d}$,
L.~La~Rotonda$^\textrm{\scriptsize 40a,40b}$,
C.~Lacasta$^\textrm{\scriptsize 170}$,
F.~Lacava$^\textrm{\scriptsize 134a,134b}$,
J.~Lacey$^\textrm{\scriptsize 31}$,
H.~Lacker$^\textrm{\scriptsize 17}$,
D.~Lacour$^\textrm{\scriptsize 83}$,
V.R.~Lacuesta$^\textrm{\scriptsize 170}$,
E.~Ladygin$^\textrm{\scriptsize 68}$,
R.~Lafaye$^\textrm{\scriptsize 5}$,
B.~Laforge$^\textrm{\scriptsize 83}$,
T.~Lagouri$^\textrm{\scriptsize 179}$,
S.~Lai$^\textrm{\scriptsize 57}$,
S.~Lammers$^\textrm{\scriptsize 64}$,
W.~Lampl$^\textrm{\scriptsize 7}$,
E.~Lan\c{c}on$^\textrm{\scriptsize 138}$,
U.~Landgraf$^\textrm{\scriptsize 51}$,
M.P.J.~Landon$^\textrm{\scriptsize 79}$,
M.C.~Lanfermann$^\textrm{\scriptsize 52}$,
V.S.~Lang$^\textrm{\scriptsize 60a}$,
J.C.~Lange$^\textrm{\scriptsize 13}$,
A.J.~Lankford$^\textrm{\scriptsize 166}$,
F.~Lanni$^\textrm{\scriptsize 27}$,
K.~Lantzsch$^\textrm{\scriptsize 23}$,
A.~Lanza$^\textrm{\scriptsize 123a}$,
S.~Laplace$^\textrm{\scriptsize 83}$,
C.~Lapoire$^\textrm{\scriptsize 32}$,
J.F.~Laporte$^\textrm{\scriptsize 138}$,
T.~Lari$^\textrm{\scriptsize 94a}$,
F.~Lasagni~Manghi$^\textrm{\scriptsize 22a,22b}$,
M.~Lassnig$^\textrm{\scriptsize 32}$,
P.~Laurelli$^\textrm{\scriptsize 50}$,
W.~Lavrijsen$^\textrm{\scriptsize 16}$,
A.T.~Law$^\textrm{\scriptsize 139}$,
P.~Laycock$^\textrm{\scriptsize 77}$,
T.~Lazovich$^\textrm{\scriptsize 59}$,
M.~Lazzaroni$^\textrm{\scriptsize 94a,94b}$,
B.~Le$^\textrm{\scriptsize 91}$,
O.~Le~Dortz$^\textrm{\scriptsize 83}$,
E.~Le~Guirriec$^\textrm{\scriptsize 88}$,
E.P.~Le~Quilleuc$^\textrm{\scriptsize 138}$,
M.~LeBlanc$^\textrm{\scriptsize 172}$,
T.~LeCompte$^\textrm{\scriptsize 6}$,
F.~Ledroit-Guillon$^\textrm{\scriptsize 58}$,
C.A.~Lee$^\textrm{\scriptsize 27}$,
S.C.~Lee$^\textrm{\scriptsize 153}$,
L.~Lee$^\textrm{\scriptsize 1}$,
B.~Lefebvre$^\textrm{\scriptsize 90}$,
G.~Lefebvre$^\textrm{\scriptsize 83}$,
M.~Lefebvre$^\textrm{\scriptsize 172}$,
F.~Legger$^\textrm{\scriptsize 102}$,
C.~Leggett$^\textrm{\scriptsize 16}$,
A.~Lehan$^\textrm{\scriptsize 77}$,
G.~Lehmann~Miotto$^\textrm{\scriptsize 32}$,
X.~Lei$^\textrm{\scriptsize 7}$,
W.A.~Leight$^\textrm{\scriptsize 31}$,
A.G.~Leister$^\textrm{\scriptsize 179}$,
M.A.L.~Leite$^\textrm{\scriptsize 26d}$,
R.~Leitner$^\textrm{\scriptsize 131}$,
D.~Lellouch$^\textrm{\scriptsize 175}$,
B.~Lemmer$^\textrm{\scriptsize 57}$,
K.J.C.~Leney$^\textrm{\scriptsize 81}$,
T.~Lenz$^\textrm{\scriptsize 23}$,
B.~Lenzi$^\textrm{\scriptsize 32}$,
R.~Leone$^\textrm{\scriptsize 7}$,
S.~Leone$^\textrm{\scriptsize 126a,126b}$,
C.~Leonidopoulos$^\textrm{\scriptsize 49}$,
S.~Leontsinis$^\textrm{\scriptsize 10}$,
G.~Lerner$^\textrm{\scriptsize 151}$,
C.~Leroy$^\textrm{\scriptsize 97}$,
A.A.J.~Lesage$^\textrm{\scriptsize 138}$,
C.G.~Lester$^\textrm{\scriptsize 30}$,
M.~Levchenko$^\textrm{\scriptsize 125}$,
J.~Lev\^eque$^\textrm{\scriptsize 5}$,
D.~Levin$^\textrm{\scriptsize 92}$,
L.J.~Levinson$^\textrm{\scriptsize 175}$,
M.~Levy$^\textrm{\scriptsize 19}$,
D.~Lewis$^\textrm{\scriptsize 79}$,
M.~Leyton$^\textrm{\scriptsize 44}$,
B.~Li$^\textrm{\scriptsize 36a}$$^{,q}$,
C.~Li$^\textrm{\scriptsize 36a}$,
H.~Li$^\textrm{\scriptsize 150}$,
L.~Li$^\textrm{\scriptsize 48}$,
L.~Li$^\textrm{\scriptsize 36c}$,
Q.~Li$^\textrm{\scriptsize 35a}$,
S.~Li$^\textrm{\scriptsize 48}$,
X.~Li$^\textrm{\scriptsize 87}$,
Y.~Li$^\textrm{\scriptsize 143}$,
Z.~Liang$^\textrm{\scriptsize 35a}$,
B.~Liberti$^\textrm{\scriptsize 135a}$,
A.~Liblong$^\textrm{\scriptsize 161}$,
P.~Lichard$^\textrm{\scriptsize 32}$,
K.~Lie$^\textrm{\scriptsize 169}$,
J.~Liebal$^\textrm{\scriptsize 23}$,
W.~Liebig$^\textrm{\scriptsize 15}$,
A.~Limosani$^\textrm{\scriptsize 152}$,
S.C.~Lin$^\textrm{\scriptsize 153}$$^{,ac}$,
T.H.~Lin$^\textrm{\scriptsize 86}$,
B.E.~Lindquist$^\textrm{\scriptsize 150}$,
A.E.~Lionti$^\textrm{\scriptsize 52}$,
E.~Lipeles$^\textrm{\scriptsize 124}$,
A.~Lipniacka$^\textrm{\scriptsize 15}$,
M.~Lisovyi$^\textrm{\scriptsize 60b}$,
T.M.~Liss$^\textrm{\scriptsize 169}$,
A.~Lister$^\textrm{\scriptsize 171}$,
A.M.~Litke$^\textrm{\scriptsize 139}$,
B.~Liu$^\textrm{\scriptsize 153}$$^{,ad}$,
D.~Liu$^\textrm{\scriptsize 153}$,
H.~Liu$^\textrm{\scriptsize 92}$,
H.~Liu$^\textrm{\scriptsize 27}$,
J.~Liu$^\textrm{\scriptsize 36b}$,
J.B.~Liu$^\textrm{\scriptsize 36a}$,
K.~Liu$^\textrm{\scriptsize 88}$,
L.~Liu$^\textrm{\scriptsize 169}$,
M.~Liu$^\textrm{\scriptsize 36a}$,
Y.L.~Liu$^\textrm{\scriptsize 36a}$,
Y.~Liu$^\textrm{\scriptsize 36a}$,
M.~Livan$^\textrm{\scriptsize 123a,123b}$,
A.~Lleres$^\textrm{\scriptsize 58}$,
J.~Llorente~Merino$^\textrm{\scriptsize 35a}$,
S.L.~Lloyd$^\textrm{\scriptsize 79}$,
F.~Lo~Sterzo$^\textrm{\scriptsize 153}$,
E.M.~Lobodzinska$^\textrm{\scriptsize 45}$,
P.~Loch$^\textrm{\scriptsize 7}$,
F.K.~Loebinger$^\textrm{\scriptsize 87}$,
K.M.~Loew$^\textrm{\scriptsize 25}$,
A.~Loginov$^\textrm{\scriptsize 179}$$^{,*}$,
T.~Lohse$^\textrm{\scriptsize 17}$,
K.~Lohwasser$^\textrm{\scriptsize 45}$,
M.~Lokajicek$^\textrm{\scriptsize 129}$,
B.A.~Long$^\textrm{\scriptsize 24}$,
J.D.~Long$^\textrm{\scriptsize 169}$,
R.E.~Long$^\textrm{\scriptsize 75}$,
L.~Longo$^\textrm{\scriptsize 76a,76b}$,
K.A.~Looper$^\textrm{\scriptsize 113}$,
J.A.~Lopez$^\textrm{\scriptsize 34b}$,
D.~Lopez~Mateos$^\textrm{\scriptsize 59}$,
B.~Lopez~Paredes$^\textrm{\scriptsize 141}$,
I.~Lopez~Paz$^\textrm{\scriptsize 13}$,
A.~Lopez~Solis$^\textrm{\scriptsize 83}$,
J.~Lorenz$^\textrm{\scriptsize 102}$,
N.~Lorenzo~Martinez$^\textrm{\scriptsize 64}$,
M.~Losada$^\textrm{\scriptsize 21}$,
P.J.~L{\"o}sel$^\textrm{\scriptsize 102}$,
X.~Lou$^\textrm{\scriptsize 35a}$,
A.~Lounis$^\textrm{\scriptsize 119}$,
J.~Love$^\textrm{\scriptsize 6}$,
P.A.~Love$^\textrm{\scriptsize 75}$,
H.~Lu$^\textrm{\scriptsize 62a}$,
N.~Lu$^\textrm{\scriptsize 92}$,
H.J.~Lubatti$^\textrm{\scriptsize 140}$,
C.~Luci$^\textrm{\scriptsize 134a,134b}$,
A.~Lucotte$^\textrm{\scriptsize 58}$,
C.~Luedtke$^\textrm{\scriptsize 51}$,
F.~Luehring$^\textrm{\scriptsize 64}$,
W.~Lukas$^\textrm{\scriptsize 65}$,
L.~Luminari$^\textrm{\scriptsize 134a}$,
O.~Lundberg$^\textrm{\scriptsize 148a,148b}$,
B.~Lund-Jensen$^\textrm{\scriptsize 149}$,
P.M.~Luzi$^\textrm{\scriptsize 83}$,
D.~Lynn$^\textrm{\scriptsize 27}$,
R.~Lysak$^\textrm{\scriptsize 129}$,
E.~Lytken$^\textrm{\scriptsize 84}$,
V.~Lyubushkin$^\textrm{\scriptsize 68}$,
H.~Ma$^\textrm{\scriptsize 27}$,
L.L.~Ma$^\textrm{\scriptsize 36b}$,
Y.~Ma$^\textrm{\scriptsize 36b}$,
G.~Maccarrone$^\textrm{\scriptsize 50}$,
A.~Macchiolo$^\textrm{\scriptsize 103}$,
C.M.~Macdonald$^\textrm{\scriptsize 141}$,
B.~Ma\v{c}ek$^\textrm{\scriptsize 78}$,
J.~Machado~Miguens$^\textrm{\scriptsize 124,128b}$,
D.~Madaffari$^\textrm{\scriptsize 88}$,
R.~Madar$^\textrm{\scriptsize 37}$,
H.J.~Maddocks$^\textrm{\scriptsize 168}$,
W.F.~Mader$^\textrm{\scriptsize 47}$,
A.~Madsen$^\textrm{\scriptsize 45}$,
J.~Maeda$^\textrm{\scriptsize 70}$,
S.~Maeland$^\textrm{\scriptsize 15}$,
T.~Maeno$^\textrm{\scriptsize 27}$,
A.~Maevskiy$^\textrm{\scriptsize 101}$,
E.~Magradze$^\textrm{\scriptsize 57}$,
J.~Mahlstedt$^\textrm{\scriptsize 109}$,
C.~Maiani$^\textrm{\scriptsize 119}$,
C.~Maidantchik$^\textrm{\scriptsize 26a}$,
A.A.~Maier$^\textrm{\scriptsize 103}$,
T.~Maier$^\textrm{\scriptsize 102}$,
A.~Maio$^\textrm{\scriptsize 128a,128b,128d}$,
S.~Majewski$^\textrm{\scriptsize 118}$,
Y.~Makida$^\textrm{\scriptsize 69}$,
N.~Makovec$^\textrm{\scriptsize 119}$,
B.~Malaescu$^\textrm{\scriptsize 83}$,
Pa.~Malecki$^\textrm{\scriptsize 42}$,
V.P.~Maleev$^\textrm{\scriptsize 125}$,
F.~Malek$^\textrm{\scriptsize 58}$,
U.~Mallik$^\textrm{\scriptsize 66}$,
D.~Malon$^\textrm{\scriptsize 6}$,
C.~Malone$^\textrm{\scriptsize 145}$,
C.~Malone$^\textrm{\scriptsize 30}$,
S.~Maltezos$^\textrm{\scriptsize 10}$,
S.~Malyukov$^\textrm{\scriptsize 32}$,
J.~Mamuzic$^\textrm{\scriptsize 170}$,
G.~Mancini$^\textrm{\scriptsize 50}$,
L.~Mandelli$^\textrm{\scriptsize 94a}$,
I.~Mandi\'{c}$^\textrm{\scriptsize 78}$,
J.~Maneira$^\textrm{\scriptsize 128a,128b}$,
L.~Manhaes~de~Andrade~Filho$^\textrm{\scriptsize 26b}$,
J.~Manjarres~Ramos$^\textrm{\scriptsize 163b}$,
A.~Mann$^\textrm{\scriptsize 102}$,
A.~Manousos$^\textrm{\scriptsize 32}$,
B.~Mansoulie$^\textrm{\scriptsize 138}$,
J.D.~Mansour$^\textrm{\scriptsize 35a}$,
R.~Mantifel$^\textrm{\scriptsize 90}$,
M.~Mantoani$^\textrm{\scriptsize 57}$,
S.~Manzoni$^\textrm{\scriptsize 94a,94b}$,
L.~Mapelli$^\textrm{\scriptsize 32}$,
G.~Marceca$^\textrm{\scriptsize 29}$,
L.~March$^\textrm{\scriptsize 52}$,
G.~Marchiori$^\textrm{\scriptsize 83}$,
M.~Marcisovsky$^\textrm{\scriptsize 129}$,
M.~Marjanovic$^\textrm{\scriptsize 14}$,
D.E.~Marley$^\textrm{\scriptsize 92}$,
F.~Marroquim$^\textrm{\scriptsize 26a}$,
S.P.~Marsden$^\textrm{\scriptsize 87}$,
Z.~Marshall$^\textrm{\scriptsize 16}$,
S.~Marti-Garcia$^\textrm{\scriptsize 170}$,
B.~Martin$^\textrm{\scriptsize 93}$,
T.A.~Martin$^\textrm{\scriptsize 173}$,
V.J.~Martin$^\textrm{\scriptsize 49}$,
B.~Martin~dit~Latour$^\textrm{\scriptsize 15}$,
M.~Martinez$^\textrm{\scriptsize 13}$$^{,t}$,
V.I.~Martinez~Outschoorn$^\textrm{\scriptsize 169}$,
S.~Martin-Haugh$^\textrm{\scriptsize 133}$,
V.S.~Martoiu$^\textrm{\scriptsize 28b}$,
A.C.~Martyniuk$^\textrm{\scriptsize 81}$,
A.~Marzin$^\textrm{\scriptsize 32}$,
L.~Masetti$^\textrm{\scriptsize 86}$,
T.~Mashimo$^\textrm{\scriptsize 157}$,
R.~Mashinistov$^\textrm{\scriptsize 98}$,
J.~Masik$^\textrm{\scriptsize 87}$,
A.L.~Maslennikov$^\textrm{\scriptsize 111}$$^{,c}$,
I.~Massa$^\textrm{\scriptsize 22a,22b}$,
L.~Massa$^\textrm{\scriptsize 22a,22b}$,
P.~Mastrandrea$^\textrm{\scriptsize 5}$,
A.~Mastroberardino$^\textrm{\scriptsize 40a,40b}$,
T.~Masubuchi$^\textrm{\scriptsize 157}$,
P.~M\"attig$^\textrm{\scriptsize 178}$,
J.~Mattmann$^\textrm{\scriptsize 86}$,
J.~Maurer$^\textrm{\scriptsize 28b}$,
S.J.~Maxfield$^\textrm{\scriptsize 77}$,
D.A.~Maximov$^\textrm{\scriptsize 111}$$^{,c}$,
R.~Mazini$^\textrm{\scriptsize 153}$,
I.~Maznas$^\textrm{\scriptsize 156}$,
S.M.~Mazza$^\textrm{\scriptsize 94a,94b}$,
N.C.~Mc~Fadden$^\textrm{\scriptsize 107}$,
G.~Mc~Goldrick$^\textrm{\scriptsize 161}$,
S.P.~Mc~Kee$^\textrm{\scriptsize 92}$,
A.~McCarn$^\textrm{\scriptsize 92}$,
R.L.~McCarthy$^\textrm{\scriptsize 150}$,
T.G.~McCarthy$^\textrm{\scriptsize 103}$,
L.I.~McClymont$^\textrm{\scriptsize 81}$,
E.F.~McDonald$^\textrm{\scriptsize 91}$,
J.A.~Mcfayden$^\textrm{\scriptsize 81}$,
G.~Mchedlidze$^\textrm{\scriptsize 57}$,
S.J.~McMahon$^\textrm{\scriptsize 133}$,
R.A.~McPherson$^\textrm{\scriptsize 172}$$^{,n}$,
M.~Medinnis$^\textrm{\scriptsize 45}$,
S.~Meehan$^\textrm{\scriptsize 140}$,
S.~Mehlhase$^\textrm{\scriptsize 102}$,
A.~Mehta$^\textrm{\scriptsize 77}$,
K.~Meier$^\textrm{\scriptsize 60a}$,
C.~Meineck$^\textrm{\scriptsize 102}$,
B.~Meirose$^\textrm{\scriptsize 44}$,
D.~Melini$^\textrm{\scriptsize 170}$$^{,ae}$,
B.R.~Mellado~Garcia$^\textrm{\scriptsize 147c}$,
M.~Melo$^\textrm{\scriptsize 146a}$,
F.~Meloni$^\textrm{\scriptsize 18}$,
S.B.~Menary$^\textrm{\scriptsize 87}$,
L.~Meng$^\textrm{\scriptsize 77}$,
X.T.~Meng$^\textrm{\scriptsize 92}$,
A.~Mengarelli$^\textrm{\scriptsize 22a,22b}$,
S.~Menke$^\textrm{\scriptsize 103}$,
E.~Meoni$^\textrm{\scriptsize 165}$,
S.~Mergelmeyer$^\textrm{\scriptsize 17}$,
P.~Mermod$^\textrm{\scriptsize 52}$,
L.~Merola$^\textrm{\scriptsize 106a,106b}$,
C.~Meroni$^\textrm{\scriptsize 94a}$,
F.S.~Merritt$^\textrm{\scriptsize 33}$,
A.~Messina$^\textrm{\scriptsize 134a,134b}$,
J.~Metcalfe$^\textrm{\scriptsize 6}$,
A.S.~Mete$^\textrm{\scriptsize 166}$,
C.~Meyer$^\textrm{\scriptsize 86}$,
C.~Meyer$^\textrm{\scriptsize 124}$,
J-P.~Meyer$^\textrm{\scriptsize 138}$,
J.~Meyer$^\textrm{\scriptsize 109}$,
H.~Meyer~Zu~Theenhausen$^\textrm{\scriptsize 60a}$,
F.~Miano$^\textrm{\scriptsize 151}$,
R.P.~Middleton$^\textrm{\scriptsize 133}$,
S.~Miglioranzi$^\textrm{\scriptsize 53a,53b}$,
L.~Mijovi\'{c}$^\textrm{\scriptsize 49}$,
G.~Mikenberg$^\textrm{\scriptsize 175}$,
M.~Mikestikova$^\textrm{\scriptsize 129}$,
M.~Miku\v{z}$^\textrm{\scriptsize 78}$,
M.~Milesi$^\textrm{\scriptsize 91}$,
A.~Milic$^\textrm{\scriptsize 27}$,
D.W.~Miller$^\textrm{\scriptsize 33}$,
C.~Mills$^\textrm{\scriptsize 49}$,
A.~Milov$^\textrm{\scriptsize 175}$,
D.A.~Milstead$^\textrm{\scriptsize 148a,148b}$,
A.A.~Minaenko$^\textrm{\scriptsize 132}$,
Y.~Minami$^\textrm{\scriptsize 157}$,
I.A.~Minashvili$^\textrm{\scriptsize 68}$,
A.I.~Mincer$^\textrm{\scriptsize 112}$,
B.~Mindur$^\textrm{\scriptsize 41a}$,
M.~Mineev$^\textrm{\scriptsize 68}$,
Y.~Minegishi$^\textrm{\scriptsize 157}$,
Y.~Ming$^\textrm{\scriptsize 176}$,
L.M.~Mir$^\textrm{\scriptsize 13}$,
K.P.~Mistry$^\textrm{\scriptsize 124}$,
T.~Mitani$^\textrm{\scriptsize 174}$,
J.~Mitrevski$^\textrm{\scriptsize 102}$,
V.A.~Mitsou$^\textrm{\scriptsize 170}$,
A.~Miucci$^\textrm{\scriptsize 18}$,
P.S.~Miyagawa$^\textrm{\scriptsize 141}$,
A.~Mizukami$^\textrm{\scriptsize 69}$,
J.U.~Mj\"ornmark$^\textrm{\scriptsize 84}$,
M.~Mlynarikova$^\textrm{\scriptsize 131}$,
T.~Moa$^\textrm{\scriptsize 148a,148b}$,
K.~Mochizuki$^\textrm{\scriptsize 97}$,
P.~Mogg$^\textrm{\scriptsize 51}$,
S.~Mohapatra$^\textrm{\scriptsize 38}$,
S.~Molander$^\textrm{\scriptsize 148a,148b}$,
R.~Moles-Valls$^\textrm{\scriptsize 23}$,
R.~Monden$^\textrm{\scriptsize 71}$,
M.C.~Mondragon$^\textrm{\scriptsize 93}$,
K.~M\"onig$^\textrm{\scriptsize 45}$,
J.~Monk$^\textrm{\scriptsize 39}$,
E.~Monnier$^\textrm{\scriptsize 88}$,
A.~Montalbano$^\textrm{\scriptsize 150}$,
J.~Montejo~Berlingen$^\textrm{\scriptsize 32}$,
F.~Monticelli$^\textrm{\scriptsize 74}$,
S.~Monzani$^\textrm{\scriptsize 94a,94b}$,
R.W.~Moore$^\textrm{\scriptsize 3}$,
N.~Morange$^\textrm{\scriptsize 119}$,
D.~Moreno$^\textrm{\scriptsize 21}$,
M.~Moreno~Ll\'acer$^\textrm{\scriptsize 57}$,
P.~Morettini$^\textrm{\scriptsize 53a}$,
S.~Morgenstern$^\textrm{\scriptsize 32}$,
D.~Mori$^\textrm{\scriptsize 144}$,
T.~Mori$^\textrm{\scriptsize 157}$,
M.~Morii$^\textrm{\scriptsize 59}$,
M.~Morinaga$^\textrm{\scriptsize 157}$,
V.~Morisbak$^\textrm{\scriptsize 121}$,
S.~Moritz$^\textrm{\scriptsize 86}$,
A.K.~Morley$^\textrm{\scriptsize 152}$,
G.~Mornacchi$^\textrm{\scriptsize 32}$,
J.D.~Morris$^\textrm{\scriptsize 79}$,
L.~Morvaj$^\textrm{\scriptsize 150}$,
P.~Moschovakos$^\textrm{\scriptsize 10}$,
M.~Mosidze$^\textrm{\scriptsize 54b}$,
H.J.~Moss$^\textrm{\scriptsize 141}$,
J.~Moss$^\textrm{\scriptsize 145}$$^{,af}$,
K.~Motohashi$^\textrm{\scriptsize 159}$,
R.~Mount$^\textrm{\scriptsize 145}$,
E.~Mountricha$^\textrm{\scriptsize 27}$,
E.J.W.~Moyse$^\textrm{\scriptsize 89}$,
S.~Muanza$^\textrm{\scriptsize 88}$,
R.D.~Mudd$^\textrm{\scriptsize 19}$,
F.~Mueller$^\textrm{\scriptsize 103}$,
J.~Mueller$^\textrm{\scriptsize 127}$,
R.S.P.~Mueller$^\textrm{\scriptsize 102}$,
T.~Mueller$^\textrm{\scriptsize 30}$,
D.~Muenstermann$^\textrm{\scriptsize 75}$,
P.~Mullen$^\textrm{\scriptsize 56}$,
G.A.~Mullier$^\textrm{\scriptsize 18}$,
F.J.~Munoz~Sanchez$^\textrm{\scriptsize 87}$,
J.A.~Murillo~Quijada$^\textrm{\scriptsize 19}$,
W.J.~Murray$^\textrm{\scriptsize 173,133}$,
H.~Musheghyan$^\textrm{\scriptsize 57}$,
M.~Mu\v{s}kinja$^\textrm{\scriptsize 78}$,
A.G.~Myagkov$^\textrm{\scriptsize 132}$$^{,ag}$,
M.~Myska$^\textrm{\scriptsize 130}$,
B.P.~Nachman$^\textrm{\scriptsize 145}$,
O.~Nackenhorst$^\textrm{\scriptsize 52}$,
K.~Nagai$^\textrm{\scriptsize 122}$,
R.~Nagai$^\textrm{\scriptsize 69}$$^{,aa}$,
K.~Nagano$^\textrm{\scriptsize 69}$,
Y.~Nagasaka$^\textrm{\scriptsize 61}$,
K.~Nagata$^\textrm{\scriptsize 164}$,
M.~Nagel$^\textrm{\scriptsize 51}$,
E.~Nagy$^\textrm{\scriptsize 88}$,
A.M.~Nairz$^\textrm{\scriptsize 32}$,
Y.~Nakahama$^\textrm{\scriptsize 105}$,
K.~Nakamura$^\textrm{\scriptsize 69}$,
T.~Nakamura$^\textrm{\scriptsize 157}$,
I.~Nakano$^\textrm{\scriptsize 114}$,
R.F.~Naranjo~Garcia$^\textrm{\scriptsize 45}$,
R.~Narayan$^\textrm{\scriptsize 11}$,
D.I.~Narrias~Villar$^\textrm{\scriptsize 60a}$,
I.~Naryshkin$^\textrm{\scriptsize 125}$,
T.~Naumann$^\textrm{\scriptsize 45}$,
G.~Navarro$^\textrm{\scriptsize 21}$,
R.~Nayyar$^\textrm{\scriptsize 7}$,
H.A.~Neal$^\textrm{\scriptsize 92}$,
P.Yu.~Nechaeva$^\textrm{\scriptsize 98}$,
T.J.~Neep$^\textrm{\scriptsize 87}$,
A.~Negri$^\textrm{\scriptsize 123a,123b}$,
M.~Negrini$^\textrm{\scriptsize 22a}$,
S.~Nektarijevic$^\textrm{\scriptsize 108}$,
C.~Nellist$^\textrm{\scriptsize 119}$,
A.~Nelson$^\textrm{\scriptsize 166}$,
S.~Nemecek$^\textrm{\scriptsize 129}$,
P.~Nemethy$^\textrm{\scriptsize 112}$,
A.A.~Nepomuceno$^\textrm{\scriptsize 26a}$,
M.~Nessi$^\textrm{\scriptsize 32}$$^{,ah}$,
M.S.~Neubauer$^\textrm{\scriptsize 169}$,
M.~Neumann$^\textrm{\scriptsize 178}$,
R.M.~Neves$^\textrm{\scriptsize 112}$,
P.~Nevski$^\textrm{\scriptsize 27}$,
P.R.~Newman$^\textrm{\scriptsize 19}$,
D.H.~Nguyen$^\textrm{\scriptsize 6}$,
T.~Nguyen~Manh$^\textrm{\scriptsize 97}$,
R.B.~Nickerson$^\textrm{\scriptsize 122}$,
R.~Nicolaidou$^\textrm{\scriptsize 138}$,
J.~Nielsen$^\textrm{\scriptsize 139}$,
A.~Nikiforov$^\textrm{\scriptsize 17}$,
V.~Nikolaenko$^\textrm{\scriptsize 132}$$^{,ag}$,
I.~Nikolic-Audit$^\textrm{\scriptsize 83}$,
K.~Nikolopoulos$^\textrm{\scriptsize 19}$,
J.K.~Nilsen$^\textrm{\scriptsize 121}$,
P.~Nilsson$^\textrm{\scriptsize 27}$,
Y.~Ninomiya$^\textrm{\scriptsize 157}$,
A.~Nisati$^\textrm{\scriptsize 134a}$,
R.~Nisius$^\textrm{\scriptsize 103}$,
T.~Nobe$^\textrm{\scriptsize 157}$,
M.~Nomachi$^\textrm{\scriptsize 120}$,
I.~Nomidis$^\textrm{\scriptsize 31}$,
T.~Nooney$^\textrm{\scriptsize 79}$,
S.~Norberg$^\textrm{\scriptsize 115}$,
M.~Nordberg$^\textrm{\scriptsize 32}$,
N.~Norjoharuddeen$^\textrm{\scriptsize 122}$,
O.~Novgorodova$^\textrm{\scriptsize 47}$,
S.~Nowak$^\textrm{\scriptsize 103}$,
M.~Nozaki$^\textrm{\scriptsize 69}$,
L.~Nozka$^\textrm{\scriptsize 117}$,
K.~Ntekas$^\textrm{\scriptsize 166}$,
E.~Nurse$^\textrm{\scriptsize 81}$,
F.~Nuti$^\textrm{\scriptsize 91}$,
F.~O'grady$^\textrm{\scriptsize 7}$,
D.C.~O'Neil$^\textrm{\scriptsize 144}$,
A.A.~O'Rourke$^\textrm{\scriptsize 45}$,
V.~O'Shea$^\textrm{\scriptsize 56}$,
F.G.~Oakham$^\textrm{\scriptsize 31}$$^{,d}$,
H.~Oberlack$^\textrm{\scriptsize 103}$,
T.~Obermann$^\textrm{\scriptsize 23}$,
J.~Ocariz$^\textrm{\scriptsize 83}$,
A.~Ochi$^\textrm{\scriptsize 70}$,
I.~Ochoa$^\textrm{\scriptsize 38}$,
J.P.~Ochoa-Ricoux$^\textrm{\scriptsize 34a}$,
S.~Oda$^\textrm{\scriptsize 73}$,
S.~Odaka$^\textrm{\scriptsize 69}$,
H.~Ogren$^\textrm{\scriptsize 64}$,
A.~Oh$^\textrm{\scriptsize 87}$,
S.H.~Oh$^\textrm{\scriptsize 48}$,
C.C.~Ohm$^\textrm{\scriptsize 16}$,
H.~Ohman$^\textrm{\scriptsize 168}$,
H.~Oide$^\textrm{\scriptsize 53a,53b}$,
H.~Okawa$^\textrm{\scriptsize 164}$,
Y.~Okumura$^\textrm{\scriptsize 157}$,
T.~Okuyama$^\textrm{\scriptsize 69}$,
A.~Olariu$^\textrm{\scriptsize 28b}$,
L.F.~Oleiro~Seabra$^\textrm{\scriptsize 128a}$,
S.A.~Olivares~Pino$^\textrm{\scriptsize 49}$,
D.~Oliveira~Damazio$^\textrm{\scriptsize 27}$,
A.~Olszewski$^\textrm{\scriptsize 42}$,
J.~Olszowska$^\textrm{\scriptsize 42}$,
A.~Onofre$^\textrm{\scriptsize 128a,128e}$,
K.~Onogi$^\textrm{\scriptsize 105}$,
P.U.E.~Onyisi$^\textrm{\scriptsize 11}$$^{,w}$,
M.J.~Oreglia$^\textrm{\scriptsize 33}$,
Y.~Oren$^\textrm{\scriptsize 155}$,
D.~Orestano$^\textrm{\scriptsize 136a,136b}$,
N.~Orlando$^\textrm{\scriptsize 62b}$,
R.S.~Orr$^\textrm{\scriptsize 161}$,
B.~Osculati$^\textrm{\scriptsize 53a,53b}$$^{,*}$,
R.~Ospanov$^\textrm{\scriptsize 87}$,
G.~Otero~y~Garzon$^\textrm{\scriptsize 29}$,
H.~Otono$^\textrm{\scriptsize 73}$,
M.~Ouchrif$^\textrm{\scriptsize 137d}$,
F.~Ould-Saada$^\textrm{\scriptsize 121}$,
A.~Ouraou$^\textrm{\scriptsize 138}$,
K.P.~Oussoren$^\textrm{\scriptsize 109}$,
Q.~Ouyang$^\textrm{\scriptsize 35a}$,
M.~Owen$^\textrm{\scriptsize 56}$,
R.E.~Owen$^\textrm{\scriptsize 19}$,
V.E.~Ozcan$^\textrm{\scriptsize 20a}$,
N.~Ozturk$^\textrm{\scriptsize 8}$,
K.~Pachal$^\textrm{\scriptsize 144}$,
A.~Pacheco~Pages$^\textrm{\scriptsize 13}$,
L.~Pacheco~Rodriguez$^\textrm{\scriptsize 138}$,
C.~Padilla~Aranda$^\textrm{\scriptsize 13}$,
S.~Pagan~Griso$^\textrm{\scriptsize 16}$,
M.~Paganini$^\textrm{\scriptsize 179}$,
F.~Paige$^\textrm{\scriptsize 27}$,
P.~Pais$^\textrm{\scriptsize 89}$,
K.~Pajchel$^\textrm{\scriptsize 121}$,
G.~Palacino$^\textrm{\scriptsize 64}$,
S.~Palazzo$^\textrm{\scriptsize 40a,40b}$,
S.~Palestini$^\textrm{\scriptsize 32}$,
M.~Palka$^\textrm{\scriptsize 41b}$,
D.~Pallin$^\textrm{\scriptsize 37}$,
E.St.~Panagiotopoulou$^\textrm{\scriptsize 10}$,
I.~Panagoulias$^\textrm{\scriptsize 10}$,
C.E.~Pandini$^\textrm{\scriptsize 83}$,
J.G.~Panduro~Vazquez$^\textrm{\scriptsize 80}$,
P.~Pani$^\textrm{\scriptsize 148a,148b}$,
S.~Panitkin$^\textrm{\scriptsize 27}$,
D.~Pantea$^\textrm{\scriptsize 28b}$,
L.~Paolozzi$^\textrm{\scriptsize 52}$,
Th.D.~Papadopoulou$^\textrm{\scriptsize 10}$,
K.~Papageorgiou$^\textrm{\scriptsize 9}$,
A.~Paramonov$^\textrm{\scriptsize 6}$,
D.~Paredes~Hernandez$^\textrm{\scriptsize 179}$,
A.J.~Parker$^\textrm{\scriptsize 75}$,
M.A.~Parker$^\textrm{\scriptsize 30}$,
K.A.~Parker$^\textrm{\scriptsize 141}$,
F.~Parodi$^\textrm{\scriptsize 53a,53b}$,
J.A.~Parsons$^\textrm{\scriptsize 38}$,
U.~Parzefall$^\textrm{\scriptsize 51}$,
V.R.~Pascuzzi$^\textrm{\scriptsize 161}$,
E.~Pasqualucci$^\textrm{\scriptsize 134a}$,
S.~Passaggio$^\textrm{\scriptsize 53a}$,
Fr.~Pastore$^\textrm{\scriptsize 80}$,
G.~P\'asztor$^\textrm{\scriptsize 31}$$^{,ai}$,
S.~Pataraia$^\textrm{\scriptsize 178}$,
J.R.~Pater$^\textrm{\scriptsize 87}$,
T.~Pauly$^\textrm{\scriptsize 32}$,
J.~Pearce$^\textrm{\scriptsize 172}$,
B.~Pearson$^\textrm{\scriptsize 115}$,
L.E.~Pedersen$^\textrm{\scriptsize 39}$,
S.~Pedraza~Lopez$^\textrm{\scriptsize 170}$,
R.~Pedro$^\textrm{\scriptsize 128a,128b}$,
S.V.~Peleganchuk$^\textrm{\scriptsize 111}$$^{,c}$,
O.~Penc$^\textrm{\scriptsize 129}$,
C.~Peng$^\textrm{\scriptsize 35a}$,
H.~Peng$^\textrm{\scriptsize 36a}$,
J.~Penwell$^\textrm{\scriptsize 64}$,
B.S.~Peralva$^\textrm{\scriptsize 26b}$,
M.M.~Perego$^\textrm{\scriptsize 138}$,
D.V.~Perepelitsa$^\textrm{\scriptsize 27}$,
E.~Perez~Codina$^\textrm{\scriptsize 163a}$,
L.~Perini$^\textrm{\scriptsize 94a,94b}$,
H.~Pernegger$^\textrm{\scriptsize 32}$,
S.~Perrella$^\textrm{\scriptsize 106a,106b}$,
R.~Peschke$^\textrm{\scriptsize 45}$,
V.D.~Peshekhonov$^\textrm{\scriptsize 68}$,
K.~Peters$^\textrm{\scriptsize 45}$,
R.F.Y.~Peters$^\textrm{\scriptsize 87}$,
B.A.~Petersen$^\textrm{\scriptsize 32}$,
T.C.~Petersen$^\textrm{\scriptsize 39}$,
E.~Petit$^\textrm{\scriptsize 58}$,
A.~Petridis$^\textrm{\scriptsize 1}$,
C.~Petridou$^\textrm{\scriptsize 156}$,
P.~Petroff$^\textrm{\scriptsize 119}$,
E.~Petrolo$^\textrm{\scriptsize 134a}$,
M.~Petrov$^\textrm{\scriptsize 122}$,
F.~Petrucci$^\textrm{\scriptsize 136a,136b}$,
N.E.~Pettersson$^\textrm{\scriptsize 89}$,
A.~Peyaud$^\textrm{\scriptsize 138}$,
R.~Pezoa$^\textrm{\scriptsize 34b}$,
P.W.~Phillips$^\textrm{\scriptsize 133}$,
G.~Piacquadio$^\textrm{\scriptsize 145}$$^{,aj}$,
E.~Pianori$^\textrm{\scriptsize 173}$,
A.~Picazio$^\textrm{\scriptsize 89}$,
E.~Piccaro$^\textrm{\scriptsize 79}$,
M.~Piccinini$^\textrm{\scriptsize 22a,22b}$,
M.A.~Pickering$^\textrm{\scriptsize 122}$,
R.~Piegaia$^\textrm{\scriptsize 29}$,
J.E.~Pilcher$^\textrm{\scriptsize 33}$,
A.D.~Pilkington$^\textrm{\scriptsize 87}$,
A.W.J.~Pin$^\textrm{\scriptsize 87}$,
M.~Pinamonti$^\textrm{\scriptsize 167a,167c}$$^{,ak}$,
J.L.~Pinfold$^\textrm{\scriptsize 3}$,
A.~Pingel$^\textrm{\scriptsize 39}$,
S.~Pires$^\textrm{\scriptsize 83}$,
H.~Pirumov$^\textrm{\scriptsize 45}$,
M.~Pitt$^\textrm{\scriptsize 175}$,
L.~Plazak$^\textrm{\scriptsize 146a}$,
M.-A.~Pleier$^\textrm{\scriptsize 27}$,
V.~Pleskot$^\textrm{\scriptsize 86}$,
E.~Plotnikova$^\textrm{\scriptsize 68}$,
D.~Pluth$^\textrm{\scriptsize 67}$,
R.~Poettgen$^\textrm{\scriptsize 148a,148b}$,
L.~Poggioli$^\textrm{\scriptsize 119}$,
D.~Pohl$^\textrm{\scriptsize 23}$,
G.~Polesello$^\textrm{\scriptsize 123a}$,
A.~Poley$^\textrm{\scriptsize 45}$,
A.~Policicchio$^\textrm{\scriptsize 40a,40b}$,
R.~Polifka$^\textrm{\scriptsize 161}$,
A.~Polini$^\textrm{\scriptsize 22a}$,
C.S.~Pollard$^\textrm{\scriptsize 56}$,
V.~Polychronakos$^\textrm{\scriptsize 27}$,
K.~Pomm\`es$^\textrm{\scriptsize 32}$,
L.~Pontecorvo$^\textrm{\scriptsize 134a}$,
B.G.~Pope$^\textrm{\scriptsize 93}$,
G.A.~Popeneciu$^\textrm{\scriptsize 28c}$,
A.~Poppleton$^\textrm{\scriptsize 32}$,
S.~Pospisil$^\textrm{\scriptsize 130}$,
K.~Potamianos$^\textrm{\scriptsize 16}$,
I.N.~Potrap$^\textrm{\scriptsize 68}$,
C.J.~Potter$^\textrm{\scriptsize 30}$,
C.T.~Potter$^\textrm{\scriptsize 118}$,
G.~Poulard$^\textrm{\scriptsize 32}$,
J.~Poveda$^\textrm{\scriptsize 32}$,
V.~Pozdnyakov$^\textrm{\scriptsize 68}$,
M.E.~Pozo~Astigarraga$^\textrm{\scriptsize 32}$,
P.~Pralavorio$^\textrm{\scriptsize 88}$,
A.~Pranko$^\textrm{\scriptsize 16}$,
S.~Prell$^\textrm{\scriptsize 67}$,
D.~Price$^\textrm{\scriptsize 87}$,
L.E.~Price$^\textrm{\scriptsize 6}$,
M.~Primavera$^\textrm{\scriptsize 76a}$,
S.~Prince$^\textrm{\scriptsize 90}$,
K.~Prokofiev$^\textrm{\scriptsize 62c}$,
F.~Prokoshin$^\textrm{\scriptsize 34b}$,
S.~Protopopescu$^\textrm{\scriptsize 27}$,
J.~Proudfoot$^\textrm{\scriptsize 6}$,
M.~Przybycien$^\textrm{\scriptsize 41a}$,
D.~Puddu$^\textrm{\scriptsize 136a,136b}$,
M.~Purohit$^\textrm{\scriptsize 27}$$^{,al}$,
P.~Puzo$^\textrm{\scriptsize 119}$,
J.~Qian$^\textrm{\scriptsize 92}$,
G.~Qin$^\textrm{\scriptsize 56}$,
Y.~Qin$^\textrm{\scriptsize 87}$,
A.~Quadt$^\textrm{\scriptsize 57}$,
W.B.~Quayle$^\textrm{\scriptsize 167a,167b}$,
M.~Queitsch-Maitland$^\textrm{\scriptsize 45}$,
D.~Quilty$^\textrm{\scriptsize 56}$,
S.~Raddum$^\textrm{\scriptsize 121}$,
V.~Radeka$^\textrm{\scriptsize 27}$,
V.~Radescu$^\textrm{\scriptsize 122}$,
S.K.~Radhakrishnan$^\textrm{\scriptsize 150}$,
P.~Radloff$^\textrm{\scriptsize 118}$,
P.~Rados$^\textrm{\scriptsize 91}$,
F.~Ragusa$^\textrm{\scriptsize 94a,94b}$,
G.~Rahal$^\textrm{\scriptsize 181}$,
J.A.~Raine$^\textrm{\scriptsize 87}$,
S.~Rajagopalan$^\textrm{\scriptsize 27}$,
M.~Rammensee$^\textrm{\scriptsize 32}$,
C.~Rangel-Smith$^\textrm{\scriptsize 168}$,
M.G.~Ratti$^\textrm{\scriptsize 94a,94b}$,
D.M.~Rauch$^\textrm{\scriptsize 45}$,
F.~Rauscher$^\textrm{\scriptsize 102}$,
S.~Rave$^\textrm{\scriptsize 86}$,
T.~Ravenscroft$^\textrm{\scriptsize 56}$,
I.~Ravinovich$^\textrm{\scriptsize 175}$,
M.~Raymond$^\textrm{\scriptsize 32}$,
A.L.~Read$^\textrm{\scriptsize 121}$,
N.P.~Readioff$^\textrm{\scriptsize 77}$,
M.~Reale$^\textrm{\scriptsize 76a,76b}$,
D.M.~Rebuzzi$^\textrm{\scriptsize 123a,123b}$,
A.~Redelbach$^\textrm{\scriptsize 177}$,
G.~Redlinger$^\textrm{\scriptsize 27}$,
R.~Reece$^\textrm{\scriptsize 139}$,
R.G.~Reed$^\textrm{\scriptsize 147c}$,
K.~Reeves$^\textrm{\scriptsize 44}$,
L.~Rehnisch$^\textrm{\scriptsize 17}$,
J.~Reichert$^\textrm{\scriptsize 124}$,
A.~Reiss$^\textrm{\scriptsize 86}$,
C.~Rembser$^\textrm{\scriptsize 32}$,
H.~Ren$^\textrm{\scriptsize 35a}$,
M.~Rescigno$^\textrm{\scriptsize 134a}$,
S.~Resconi$^\textrm{\scriptsize 94a}$,
O.L.~Rezanova$^\textrm{\scriptsize 111}$$^{,c}$,
P.~Reznicek$^\textrm{\scriptsize 131}$,
R.~Rezvani$^\textrm{\scriptsize 97}$,
R.~Richter$^\textrm{\scriptsize 103}$,
S.~Richter$^\textrm{\scriptsize 81}$,
E.~Richter-Was$^\textrm{\scriptsize 41b}$,
O.~Ricken$^\textrm{\scriptsize 23}$,
M.~Ridel$^\textrm{\scriptsize 83}$,
P.~Rieck$^\textrm{\scriptsize 17}$,
C.J.~Riegel$^\textrm{\scriptsize 178}$,
J.~Rieger$^\textrm{\scriptsize 57}$,
O.~Rifki$^\textrm{\scriptsize 115}$,
M.~Rijssenbeek$^\textrm{\scriptsize 150}$,
A.~Rimoldi$^\textrm{\scriptsize 123a,123b}$,
M.~Rimoldi$^\textrm{\scriptsize 18}$,
L.~Rinaldi$^\textrm{\scriptsize 22a}$,
B.~Risti\'{c}$^\textrm{\scriptsize 52}$,
E.~Ritsch$^\textrm{\scriptsize 32}$,
I.~Riu$^\textrm{\scriptsize 13}$,
F.~Rizatdinova$^\textrm{\scriptsize 116}$,
E.~Rizvi$^\textrm{\scriptsize 79}$,
C.~Rizzi$^\textrm{\scriptsize 13}$,
S.H.~Robertson$^\textrm{\scriptsize 90}$$^{,n}$,
A.~Robichaud-Veronneau$^\textrm{\scriptsize 90}$,
D.~Robinson$^\textrm{\scriptsize 30}$,
J.E.M.~Robinson$^\textrm{\scriptsize 45}$,
A.~Robson$^\textrm{\scriptsize 56}$,
C.~Roda$^\textrm{\scriptsize 126a,126b}$,
Y.~Rodina$^\textrm{\scriptsize 88}$$^{,am}$,
A.~Rodriguez~Perez$^\textrm{\scriptsize 13}$,
D.~Rodriguez~Rodriguez$^\textrm{\scriptsize 170}$,
S.~Roe$^\textrm{\scriptsize 32}$,
C.S.~Rogan$^\textrm{\scriptsize 59}$,
O.~R{\o}hne$^\textrm{\scriptsize 121}$,
J.~Roloff$^\textrm{\scriptsize 59}$,
A.~Romaniouk$^\textrm{\scriptsize 100}$,
M.~Romano$^\textrm{\scriptsize 22a,22b}$,
S.M.~Romano~Saez$^\textrm{\scriptsize 37}$,
E.~Romero~Adam$^\textrm{\scriptsize 170}$,
N.~Rompotis$^\textrm{\scriptsize 140}$,
M.~Ronzani$^\textrm{\scriptsize 51}$,
L.~Roos$^\textrm{\scriptsize 83}$,
E.~Ros$^\textrm{\scriptsize 170}$,
S.~Rosati$^\textrm{\scriptsize 134a}$,
K.~Rosbach$^\textrm{\scriptsize 51}$,
P.~Rose$^\textrm{\scriptsize 139}$,
N.-A.~Rosien$^\textrm{\scriptsize 57}$,
V.~Rossetti$^\textrm{\scriptsize 148a,148b}$,
E.~Rossi$^\textrm{\scriptsize 106a,106b}$,
L.P.~Rossi$^\textrm{\scriptsize 53a}$,
J.H.N.~Rosten$^\textrm{\scriptsize 30}$,
R.~Rosten$^\textrm{\scriptsize 140}$,
M.~Rotaru$^\textrm{\scriptsize 28b}$,
I.~Roth$^\textrm{\scriptsize 175}$,
J.~Rothberg$^\textrm{\scriptsize 140}$,
D.~Rousseau$^\textrm{\scriptsize 119}$,
A.~Rozanov$^\textrm{\scriptsize 88}$,
Y.~Rozen$^\textrm{\scriptsize 154}$,
X.~Ruan$^\textrm{\scriptsize 147c}$,
F.~Rubbo$^\textrm{\scriptsize 145}$,
M.S.~Rudolph$^\textrm{\scriptsize 161}$,
F.~R\"uhr$^\textrm{\scriptsize 51}$,
A.~Ruiz-Martinez$^\textrm{\scriptsize 31}$,
Z.~Rurikova$^\textrm{\scriptsize 51}$,
N.A.~Rusakovich$^\textrm{\scriptsize 68}$,
A.~Ruschke$^\textrm{\scriptsize 102}$,
H.L.~Russell$^\textrm{\scriptsize 140}$,
J.P.~Rutherfoord$^\textrm{\scriptsize 7}$,
N.~Ruthmann$^\textrm{\scriptsize 32}$,
Y.F.~Ryabov$^\textrm{\scriptsize 125}$,
M.~Rybar$^\textrm{\scriptsize 169}$,
G.~Rybkin$^\textrm{\scriptsize 119}$,
S.~Ryu$^\textrm{\scriptsize 6}$,
A.~Ryzhov$^\textrm{\scriptsize 132}$,
G.F.~Rzehorz$^\textrm{\scriptsize 57}$,
A.F.~Saavedra$^\textrm{\scriptsize 152}$,
G.~Sabato$^\textrm{\scriptsize 109}$,
S.~Sacerdoti$^\textrm{\scriptsize 29}$,
H.F-W.~Sadrozinski$^\textrm{\scriptsize 139}$,
R.~Sadykov$^\textrm{\scriptsize 68}$,
F.~Safai~Tehrani$^\textrm{\scriptsize 134a}$,
P.~Saha$^\textrm{\scriptsize 110}$,
M.~Sahinsoy$^\textrm{\scriptsize 60a}$,
M.~Saimpert$^\textrm{\scriptsize 138}$,
T.~Saito$^\textrm{\scriptsize 157}$,
H.~Sakamoto$^\textrm{\scriptsize 157}$,
Y.~Sakurai$^\textrm{\scriptsize 174}$,
G.~Salamanna$^\textrm{\scriptsize 136a,136b}$,
A.~Salamon$^\textrm{\scriptsize 135a,135b}$,
J.E.~Salazar~Loyola$^\textrm{\scriptsize 34b}$,
D.~Salek$^\textrm{\scriptsize 109}$,
P.H.~Sales~De~Bruin$^\textrm{\scriptsize 140}$,
D.~Salihagic$^\textrm{\scriptsize 103}$,
A.~Salnikov$^\textrm{\scriptsize 145}$,
J.~Salt$^\textrm{\scriptsize 170}$,
D.~Salvatore$^\textrm{\scriptsize 40a,40b}$,
F.~Salvatore$^\textrm{\scriptsize 151}$,
A.~Salvucci$^\textrm{\scriptsize 62a,62b,62c}$,
A.~Salzburger$^\textrm{\scriptsize 32}$,
D.~Sammel$^\textrm{\scriptsize 51}$,
D.~Sampsonidis$^\textrm{\scriptsize 156}$,
J.~S\'anchez$^\textrm{\scriptsize 170}$,
V.~Sanchez~Martinez$^\textrm{\scriptsize 170}$,
A.~Sanchez~Pineda$^\textrm{\scriptsize 106a,106b}$,
H.~Sandaker$^\textrm{\scriptsize 121}$,
R.L.~Sandbach$^\textrm{\scriptsize 79}$,
M.~Sandhoff$^\textrm{\scriptsize 178}$,
C.~Sandoval$^\textrm{\scriptsize 21}$,
D.P.C.~Sankey$^\textrm{\scriptsize 133}$,
M.~Sannino$^\textrm{\scriptsize 53a,53b}$,
A.~Sansoni$^\textrm{\scriptsize 50}$,
C.~Santoni$^\textrm{\scriptsize 37}$,
R.~Santonico$^\textrm{\scriptsize 135a,135b}$,
H.~Santos$^\textrm{\scriptsize 128a}$,
I.~Santoyo~Castillo$^\textrm{\scriptsize 151}$,
K.~Sapp$^\textrm{\scriptsize 127}$,
A.~Sapronov$^\textrm{\scriptsize 68}$,
J.G.~Saraiva$^\textrm{\scriptsize 128a,128d}$,
B.~Sarrazin$^\textrm{\scriptsize 23}$,
O.~Sasaki$^\textrm{\scriptsize 69}$,
K.~Sato$^\textrm{\scriptsize 164}$,
E.~Sauvan$^\textrm{\scriptsize 5}$,
G.~Savage$^\textrm{\scriptsize 80}$,
P.~Savard$^\textrm{\scriptsize 161}$$^{,d}$,
N.~Savic$^\textrm{\scriptsize 103}$,
C.~Sawyer$^\textrm{\scriptsize 133}$,
L.~Sawyer$^\textrm{\scriptsize 82}$$^{,s}$,
J.~Saxon$^\textrm{\scriptsize 33}$,
C.~Sbarra$^\textrm{\scriptsize 22a}$,
A.~Sbrizzi$^\textrm{\scriptsize 22a,22b}$,
T.~Scanlon$^\textrm{\scriptsize 81}$,
D.A.~Scannicchio$^\textrm{\scriptsize 166}$,
M.~Scarcella$^\textrm{\scriptsize 152}$,
V.~Scarfone$^\textrm{\scriptsize 40a,40b}$,
J.~Schaarschmidt$^\textrm{\scriptsize 175}$,
P.~Schacht$^\textrm{\scriptsize 103}$,
B.M.~Schachtner$^\textrm{\scriptsize 102}$,
D.~Schaefer$^\textrm{\scriptsize 32}$,
L.~Schaefer$^\textrm{\scriptsize 124}$,
R.~Schaefer$^\textrm{\scriptsize 45}$,
J.~Schaeffer$^\textrm{\scriptsize 86}$,
S.~Schaepe$^\textrm{\scriptsize 23}$,
S.~Schaetzel$^\textrm{\scriptsize 60b}$,
U.~Sch\"afer$^\textrm{\scriptsize 86}$,
A.C.~Schaffer$^\textrm{\scriptsize 119}$,
D.~Schaile$^\textrm{\scriptsize 102}$,
R.D.~Schamberger$^\textrm{\scriptsize 150}$,
V.~Scharf$^\textrm{\scriptsize 60a}$,
V.A.~Schegelsky$^\textrm{\scriptsize 125}$,
D.~Scheirich$^\textrm{\scriptsize 131}$,
M.~Schernau$^\textrm{\scriptsize 166}$,
C.~Schiavi$^\textrm{\scriptsize 53a,53b}$,
S.~Schier$^\textrm{\scriptsize 139}$,
C.~Schillo$^\textrm{\scriptsize 51}$,
M.~Schioppa$^\textrm{\scriptsize 40a,40b}$,
S.~Schlenker$^\textrm{\scriptsize 32}$,
K.R.~Schmidt-Sommerfeld$^\textrm{\scriptsize 103}$,
K.~Schmieden$^\textrm{\scriptsize 32}$,
C.~Schmitt$^\textrm{\scriptsize 86}$,
S.~Schmitt$^\textrm{\scriptsize 45}$,
S.~Schmitz$^\textrm{\scriptsize 86}$,
B.~Schneider$^\textrm{\scriptsize 163a}$,
U.~Schnoor$^\textrm{\scriptsize 51}$,
L.~Schoeffel$^\textrm{\scriptsize 138}$,
A.~Schoening$^\textrm{\scriptsize 60b}$,
B.D.~Schoenrock$^\textrm{\scriptsize 93}$,
E.~Schopf$^\textrm{\scriptsize 23}$,
M.~Schott$^\textrm{\scriptsize 86}$,
J.F.P.~Schouwenberg$^\textrm{\scriptsize 108}$,
J.~Schovancova$^\textrm{\scriptsize 8}$,
S.~Schramm$^\textrm{\scriptsize 52}$,
M.~Schreyer$^\textrm{\scriptsize 177}$,
N.~Schuh$^\textrm{\scriptsize 86}$,
A.~Schulte$^\textrm{\scriptsize 86}$,
M.J.~Schultens$^\textrm{\scriptsize 23}$,
H.-C.~Schultz-Coulon$^\textrm{\scriptsize 60a}$,
H.~Schulz$^\textrm{\scriptsize 17}$,
M.~Schumacher$^\textrm{\scriptsize 51}$,
B.A.~Schumm$^\textrm{\scriptsize 139}$,
Ph.~Schune$^\textrm{\scriptsize 138}$,
A.~Schwartzman$^\textrm{\scriptsize 145}$,
T.A.~Schwarz$^\textrm{\scriptsize 92}$,
H.~Schweiger$^\textrm{\scriptsize 87}$,
Ph.~Schwemling$^\textrm{\scriptsize 138}$,
R.~Schwienhorst$^\textrm{\scriptsize 93}$,
J.~Schwindling$^\textrm{\scriptsize 138}$,
T.~Schwindt$^\textrm{\scriptsize 23}$,
G.~Sciolla$^\textrm{\scriptsize 25}$,
F.~Scuri$^\textrm{\scriptsize 126a,126b}$,
F.~Scutti$^\textrm{\scriptsize 91}$,
J.~Searcy$^\textrm{\scriptsize 92}$,
P.~Seema$^\textrm{\scriptsize 23}$,
S.C.~Seidel$^\textrm{\scriptsize 107}$,
A.~Seiden$^\textrm{\scriptsize 139}$,
F.~Seifert$^\textrm{\scriptsize 130}$,
J.M.~Seixas$^\textrm{\scriptsize 26a}$,
G.~Sekhniaidze$^\textrm{\scriptsize 106a}$,
K.~Sekhon$^\textrm{\scriptsize 92}$,
S.J.~Sekula$^\textrm{\scriptsize 43}$,
D.M.~Seliverstov$^\textrm{\scriptsize 125}$$^{,*}$,
N.~Semprini-Cesari$^\textrm{\scriptsize 22a,22b}$,
C.~Serfon$^\textrm{\scriptsize 121}$,
L.~Serin$^\textrm{\scriptsize 119}$,
L.~Serkin$^\textrm{\scriptsize 167a,167b}$,
M.~Sessa$^\textrm{\scriptsize 136a,136b}$,
R.~Seuster$^\textrm{\scriptsize 172}$,
H.~Severini$^\textrm{\scriptsize 115}$,
T.~Sfiligoj$^\textrm{\scriptsize 78}$,
F.~Sforza$^\textrm{\scriptsize 32}$,
A.~Sfyrla$^\textrm{\scriptsize 52}$,
E.~Shabalina$^\textrm{\scriptsize 57}$,
N.W.~Shaikh$^\textrm{\scriptsize 148a,148b}$,
L.Y.~Shan$^\textrm{\scriptsize 35a}$,
R.~Shang$^\textrm{\scriptsize 169}$,
J.T.~Shank$^\textrm{\scriptsize 24}$,
M.~Shapiro$^\textrm{\scriptsize 16}$,
P.B.~Shatalov$^\textrm{\scriptsize 99}$,
K.~Shaw$^\textrm{\scriptsize 167a,167b}$,
S.M.~Shaw$^\textrm{\scriptsize 87}$,
A.~Shcherbakova$^\textrm{\scriptsize 148a,148b}$,
C.Y.~Shehu$^\textrm{\scriptsize 151}$,
P.~Sherwood$^\textrm{\scriptsize 81}$,
L.~Shi$^\textrm{\scriptsize 153}$$^{,an}$,
S.~Shimizu$^\textrm{\scriptsize 70}$,
C.O.~Shimmin$^\textrm{\scriptsize 166}$,
M.~Shimojima$^\textrm{\scriptsize 104}$,
S.~Shirabe$^\textrm{\scriptsize 73}$,
M.~Shiyakova$^\textrm{\scriptsize 68}$$^{,ao}$,
A.~Shmeleva$^\textrm{\scriptsize 98}$,
D.~Shoaleh~Saadi$^\textrm{\scriptsize 97}$,
M.J.~Shochet$^\textrm{\scriptsize 33}$,
S.~Shojaii$^\textrm{\scriptsize 94a}$,
D.R.~Shope$^\textrm{\scriptsize 115}$,
S.~Shrestha$^\textrm{\scriptsize 113}$,
E.~Shulga$^\textrm{\scriptsize 100}$,
M.A.~Shupe$^\textrm{\scriptsize 7}$,
P.~Sicho$^\textrm{\scriptsize 129}$,
A.M.~Sickles$^\textrm{\scriptsize 169}$,
P.E.~Sidebo$^\textrm{\scriptsize 149}$,
E.~Sideras~Haddad$^\textrm{\scriptsize 147c}$,
O.~Sidiropoulou$^\textrm{\scriptsize 177}$,
D.~Sidorov$^\textrm{\scriptsize 116}$,
A.~Sidoti$^\textrm{\scriptsize 22a,22b}$,
F.~Siegert$^\textrm{\scriptsize 47}$,
Dj.~Sijacki$^\textrm{\scriptsize 14}$,
J.~Silva$^\textrm{\scriptsize 128a,128d}$,
S.B.~Silverstein$^\textrm{\scriptsize 148a}$,
V.~Simak$^\textrm{\scriptsize 130}$,
Lj.~Simic$^\textrm{\scriptsize 14}$,
S.~Simion$^\textrm{\scriptsize 119}$,
E.~Simioni$^\textrm{\scriptsize 86}$,
B.~Simmons$^\textrm{\scriptsize 81}$,
D.~Simon$^\textrm{\scriptsize 37}$,
M.~Simon$^\textrm{\scriptsize 86}$,
P.~Sinervo$^\textrm{\scriptsize 161}$,
N.B.~Sinev$^\textrm{\scriptsize 118}$,
M.~Sioli$^\textrm{\scriptsize 22a,22b}$,
G.~Siragusa$^\textrm{\scriptsize 177}$,
S.Yu.~Sivoklokov$^\textrm{\scriptsize 101}$,
J.~Sj\"{o}lin$^\textrm{\scriptsize 148a,148b}$,
M.B.~Skinner$^\textrm{\scriptsize 75}$,
H.P.~Skottowe$^\textrm{\scriptsize 59}$,
P.~Skubic$^\textrm{\scriptsize 115}$,
M.~Slater$^\textrm{\scriptsize 19}$,
T.~Slavicek$^\textrm{\scriptsize 130}$,
M.~Slawinska$^\textrm{\scriptsize 109}$,
K.~Sliwa$^\textrm{\scriptsize 165}$,
R.~Slovak$^\textrm{\scriptsize 131}$,
V.~Smakhtin$^\textrm{\scriptsize 175}$,
B.H.~Smart$^\textrm{\scriptsize 5}$,
L.~Smestad$^\textrm{\scriptsize 15}$,
J.~Smiesko$^\textrm{\scriptsize 146a}$,
S.Yu.~Smirnov$^\textrm{\scriptsize 100}$,
Y.~Smirnov$^\textrm{\scriptsize 100}$,
L.N.~Smirnova$^\textrm{\scriptsize 101}$$^{,ap}$,
O.~Smirnova$^\textrm{\scriptsize 84}$,
J.W.~Smith$^\textrm{\scriptsize 57}$,
M.N.K.~Smith$^\textrm{\scriptsize 38}$,
R.W.~Smith$^\textrm{\scriptsize 38}$,
M.~Smizanska$^\textrm{\scriptsize 75}$,
K.~Smolek$^\textrm{\scriptsize 130}$,
A.A.~Snesarev$^\textrm{\scriptsize 98}$,
I.M.~Snyder$^\textrm{\scriptsize 118}$,
S.~Snyder$^\textrm{\scriptsize 27}$,
R.~Sobie$^\textrm{\scriptsize 172}$$^{,n}$,
F.~Socher$^\textrm{\scriptsize 47}$,
A.~Soffer$^\textrm{\scriptsize 155}$,
D.A.~Soh$^\textrm{\scriptsize 153}$,
G.~Sokhrannyi$^\textrm{\scriptsize 78}$,
C.A.~Solans~Sanchez$^\textrm{\scriptsize 32}$,
M.~Solar$^\textrm{\scriptsize 130}$,
E.Yu.~Soldatov$^\textrm{\scriptsize 100}$,
U.~Soldevila$^\textrm{\scriptsize 170}$,
A.A.~Solodkov$^\textrm{\scriptsize 132}$,
A.~Soloshenko$^\textrm{\scriptsize 68}$,
O.V.~Solovyanov$^\textrm{\scriptsize 132}$,
V.~Solovyev$^\textrm{\scriptsize 125}$,
P.~Sommer$^\textrm{\scriptsize 51}$,
H.~Son$^\textrm{\scriptsize 165}$,
H.Y.~Song$^\textrm{\scriptsize 36a}$$^{,aq}$,
A.~Sood$^\textrm{\scriptsize 16}$,
A.~Sopczak$^\textrm{\scriptsize 130}$,
V.~Sopko$^\textrm{\scriptsize 130}$,
V.~Sorin$^\textrm{\scriptsize 13}$,
D.~Sosa$^\textrm{\scriptsize 60b}$,
C.L.~Sotiropoulou$^\textrm{\scriptsize 126a,126b}$,
R.~Soualah$^\textrm{\scriptsize 167a,167c}$,
A.M.~Soukharev$^\textrm{\scriptsize 111}$$^{,c}$,
D.~South$^\textrm{\scriptsize 45}$,
B.C.~Sowden$^\textrm{\scriptsize 80}$,
S.~Spagnolo$^\textrm{\scriptsize 76a,76b}$,
M.~Spalla$^\textrm{\scriptsize 126a,126b}$,
M.~Spangenberg$^\textrm{\scriptsize 173}$,
F.~Span\`o$^\textrm{\scriptsize 80}$,
D.~Sperlich$^\textrm{\scriptsize 17}$,
F.~Spettel$^\textrm{\scriptsize 103}$,
R.~Spighi$^\textrm{\scriptsize 22a}$,
G.~Spigo$^\textrm{\scriptsize 32}$,
L.A.~Spiller$^\textrm{\scriptsize 91}$,
M.~Spousta$^\textrm{\scriptsize 131}$,
R.D.~St.~Denis$^\textrm{\scriptsize 56}$$^{,*}$,
A.~Stabile$^\textrm{\scriptsize 94a}$,
R.~Stamen$^\textrm{\scriptsize 60a}$,
S.~Stamm$^\textrm{\scriptsize 17}$,
E.~Stanecka$^\textrm{\scriptsize 42}$,
R.W.~Stanek$^\textrm{\scriptsize 6}$,
C.~Stanescu$^\textrm{\scriptsize 136a}$,
M.~Stanescu-Bellu$^\textrm{\scriptsize 45}$,
M.M.~Stanitzki$^\textrm{\scriptsize 45}$,
S.~Stapnes$^\textrm{\scriptsize 121}$,
E.A.~Starchenko$^\textrm{\scriptsize 132}$,
G.H.~Stark$^\textrm{\scriptsize 33}$,
J.~Stark$^\textrm{\scriptsize 58}$,
S.H~Stark$^\textrm{\scriptsize 39}$,
P.~Staroba$^\textrm{\scriptsize 129}$,
P.~Starovoitov$^\textrm{\scriptsize 60a}$,
S.~St\"arz$^\textrm{\scriptsize 32}$,
R.~Staszewski$^\textrm{\scriptsize 42}$,
P.~Steinberg$^\textrm{\scriptsize 27}$,
B.~Stelzer$^\textrm{\scriptsize 144}$,
H.J.~Stelzer$^\textrm{\scriptsize 32}$,
O.~Stelzer-Chilton$^\textrm{\scriptsize 163a}$,
H.~Stenzel$^\textrm{\scriptsize 55}$,
G.A.~Stewart$^\textrm{\scriptsize 56}$,
J.A.~Stillings$^\textrm{\scriptsize 23}$,
M.C.~Stockton$^\textrm{\scriptsize 90}$,
M.~Stoebe$^\textrm{\scriptsize 90}$,
G.~Stoicea$^\textrm{\scriptsize 28b}$,
P.~Stolte$^\textrm{\scriptsize 57}$,
S.~Stonjek$^\textrm{\scriptsize 103}$,
A.R.~Stradling$^\textrm{\scriptsize 8}$,
A.~Straessner$^\textrm{\scriptsize 47}$,
M.E.~Stramaglia$^\textrm{\scriptsize 18}$,
J.~Strandberg$^\textrm{\scriptsize 149}$,
S.~Strandberg$^\textrm{\scriptsize 148a,148b}$,
A.~Strandlie$^\textrm{\scriptsize 121}$,
M.~Strauss$^\textrm{\scriptsize 115}$,
P.~Strizenec$^\textrm{\scriptsize 146b}$,
R.~Str\"ohmer$^\textrm{\scriptsize 177}$,
D.M.~Strom$^\textrm{\scriptsize 118}$,
R.~Stroynowski$^\textrm{\scriptsize 43}$,
A.~Strubig$^\textrm{\scriptsize 108}$,
S.A.~Stucci$^\textrm{\scriptsize 27}$,
B.~Stugu$^\textrm{\scriptsize 15}$,
N.A.~Styles$^\textrm{\scriptsize 45}$,
D.~Su$^\textrm{\scriptsize 145}$,
J.~Su$^\textrm{\scriptsize 127}$,
S.~Suchek$^\textrm{\scriptsize 60a}$,
Y.~Sugaya$^\textrm{\scriptsize 120}$,
M.~Suk$^\textrm{\scriptsize 130}$,
V.V.~Sulin$^\textrm{\scriptsize 98}$,
S.~Sultansoy$^\textrm{\scriptsize 4c}$,
T.~Sumida$^\textrm{\scriptsize 71}$,
S.~Sun$^\textrm{\scriptsize 59}$,
X.~Sun$^\textrm{\scriptsize 35a}$,
J.E.~Sundermann$^\textrm{\scriptsize 51}$,
K.~Suruliz$^\textrm{\scriptsize 151}$,
C.J.E.~Suster$^\textrm{\scriptsize 152}$,
M.R.~Sutton$^\textrm{\scriptsize 151}$,
S.~Suzuki$^\textrm{\scriptsize 69}$,
M.~Svatos$^\textrm{\scriptsize 129}$,
M.~Swiatlowski$^\textrm{\scriptsize 33}$,
S.P.~Swift$^\textrm{\scriptsize 2}$,
I.~Sykora$^\textrm{\scriptsize 146a}$,
T.~Sykora$^\textrm{\scriptsize 131}$,
D.~Ta$^\textrm{\scriptsize 51}$,
C.~Taccini$^\textrm{\scriptsize 136a,136b}$,
K.~Tackmann$^\textrm{\scriptsize 45}$,
J.~Taenzer$^\textrm{\scriptsize 161}$,
A.~Taffard$^\textrm{\scriptsize 166}$,
R.~Tafirout$^\textrm{\scriptsize 163a}$,
N.~Taiblum$^\textrm{\scriptsize 155}$,
H.~Takai$^\textrm{\scriptsize 27}$,
R.~Takashima$^\textrm{\scriptsize 72}$,
T.~Takeshita$^\textrm{\scriptsize 142}$,
Y.~Takubo$^\textrm{\scriptsize 69}$,
M.~Talby$^\textrm{\scriptsize 88}$,
A.A.~Talyshev$^\textrm{\scriptsize 111}$$^{,c}$,
K.G.~Tan$^\textrm{\scriptsize 91}$,
J.~Tanaka$^\textrm{\scriptsize 157}$,
M.~Tanaka$^\textrm{\scriptsize 159}$,
R.~Tanaka$^\textrm{\scriptsize 119}$,
S.~Tanaka$^\textrm{\scriptsize 69}$,
R.~Tanioka$^\textrm{\scriptsize 70}$,
B.B.~Tannenwald$^\textrm{\scriptsize 113}$,
S.~Tapia~Araya$^\textrm{\scriptsize 34b}$,
S.~Tapprogge$^\textrm{\scriptsize 86}$,
S.~Tarem$^\textrm{\scriptsize 154}$,
G.F.~Tartarelli$^\textrm{\scriptsize 94a}$,
P.~Tas$^\textrm{\scriptsize 131}$,
M.~Tasevsky$^\textrm{\scriptsize 129}$,
T.~Tashiro$^\textrm{\scriptsize 71}$,
E.~Tassi$^\textrm{\scriptsize 40a,40b}$,
A.~Tavares~Delgado$^\textrm{\scriptsize 128a,128b}$,
Y.~Tayalati$^\textrm{\scriptsize 137e}$,
A.C.~Taylor$^\textrm{\scriptsize 107}$,
G.N.~Taylor$^\textrm{\scriptsize 91}$,
P.T.E.~Taylor$^\textrm{\scriptsize 91}$,
W.~Taylor$^\textrm{\scriptsize 163b}$,
F.A.~Teischinger$^\textrm{\scriptsize 32}$,
P.~Teixeira-Dias$^\textrm{\scriptsize 80}$,
K.K.~Temming$^\textrm{\scriptsize 51}$,
D.~Temple$^\textrm{\scriptsize 144}$,
H.~Ten~Kate$^\textrm{\scriptsize 32}$,
P.K.~Teng$^\textrm{\scriptsize 153}$,
J.J.~Teoh$^\textrm{\scriptsize 120}$,
F.~Tepel$^\textrm{\scriptsize 178}$,
S.~Terada$^\textrm{\scriptsize 69}$,
K.~Terashi$^\textrm{\scriptsize 157}$,
J.~Terron$^\textrm{\scriptsize 85}$,
S.~Terzo$^\textrm{\scriptsize 13}$,
M.~Testa$^\textrm{\scriptsize 50}$,
R.J.~Teuscher$^\textrm{\scriptsize 161}$$^{,n}$,
T.~Theveneaux-Pelzer$^\textrm{\scriptsize 88}$,
J.P.~Thomas$^\textrm{\scriptsize 19}$,
J.~Thomas-Wilsker$^\textrm{\scriptsize 80}$,
P.D.~Thompson$^\textrm{\scriptsize 19}$,
A.S.~Thompson$^\textrm{\scriptsize 56}$,
L.A.~Thomsen$^\textrm{\scriptsize 179}$,
E.~Thomson$^\textrm{\scriptsize 124}$,
M.J.~Tibbetts$^\textrm{\scriptsize 16}$,
R.E.~Ticse~Torres$^\textrm{\scriptsize 88}$,
V.O.~Tikhomirov$^\textrm{\scriptsize 98}$$^{,ar}$,
Yu.A.~Tikhonov$^\textrm{\scriptsize 111}$$^{,c}$,
S.~Timoshenko$^\textrm{\scriptsize 100}$,
P.~Tipton$^\textrm{\scriptsize 179}$,
S.~Tisserant$^\textrm{\scriptsize 88}$,
K.~Todome$^\textrm{\scriptsize 159}$,
T.~Todorov$^\textrm{\scriptsize 5}$$^{,*}$,
S.~Todorova-Nova$^\textrm{\scriptsize 131}$,
J.~Tojo$^\textrm{\scriptsize 73}$,
S.~Tok\'ar$^\textrm{\scriptsize 146a}$,
K.~Tokushuku$^\textrm{\scriptsize 69}$,
E.~Tolley$^\textrm{\scriptsize 59}$,
L.~Tomlinson$^\textrm{\scriptsize 87}$,
M.~Tomoto$^\textrm{\scriptsize 105}$,
L.~Tompkins$^\textrm{\scriptsize 145}$$^{,as}$,
K.~Toms$^\textrm{\scriptsize 107}$,
B.~Tong$^\textrm{\scriptsize 59}$,
P.~Tornambe$^\textrm{\scriptsize 51}$,
E.~Torrence$^\textrm{\scriptsize 118}$,
H.~Torres$^\textrm{\scriptsize 144}$,
E.~Torr\'o~Pastor$^\textrm{\scriptsize 140}$,
J.~Toth$^\textrm{\scriptsize 88}$$^{,at}$,
F.~Touchard$^\textrm{\scriptsize 88}$,
D.R.~Tovey$^\textrm{\scriptsize 141}$,
T.~Trefzger$^\textrm{\scriptsize 177}$,
A.~Tricoli$^\textrm{\scriptsize 27}$,
I.M.~Trigger$^\textrm{\scriptsize 163a}$,
S.~Trincaz-Duvoid$^\textrm{\scriptsize 83}$,
M.F.~Tripiana$^\textrm{\scriptsize 13}$,
W.~Trischuk$^\textrm{\scriptsize 161}$,
B.~Trocm\'e$^\textrm{\scriptsize 58}$,
A.~Trofymov$^\textrm{\scriptsize 45}$,
C.~Troncon$^\textrm{\scriptsize 94a}$,
M.~Trottier-McDonald$^\textrm{\scriptsize 16}$,
M.~Trovatelli$^\textrm{\scriptsize 172}$,
L.~Truong$^\textrm{\scriptsize 167a,167c}$,
M.~Trzebinski$^\textrm{\scriptsize 42}$,
A.~Trzupek$^\textrm{\scriptsize 42}$,
J.C-L.~Tseng$^\textrm{\scriptsize 122}$,
P.V.~Tsiareshka$^\textrm{\scriptsize 95}$,
G.~Tsipolitis$^\textrm{\scriptsize 10}$,
N.~Tsirintanis$^\textrm{\scriptsize 9}$,
S.~Tsiskaridze$^\textrm{\scriptsize 13}$,
V.~Tsiskaridze$^\textrm{\scriptsize 51}$,
E.G.~Tskhadadze$^\textrm{\scriptsize 54a}$,
K.M.~Tsui$^\textrm{\scriptsize 62a}$,
I.I.~Tsukerman$^\textrm{\scriptsize 99}$,
V.~Tsulaia$^\textrm{\scriptsize 16}$,
S.~Tsuno$^\textrm{\scriptsize 69}$,
D.~Tsybychev$^\textrm{\scriptsize 150}$,
Y.~Tu$^\textrm{\scriptsize 62b}$,
A.~Tudorache$^\textrm{\scriptsize 28b}$,
V.~Tudorache$^\textrm{\scriptsize 28b}$,
T.T.~Tulbure$^\textrm{\scriptsize 28a}$,
A.N.~Tuna$^\textrm{\scriptsize 59}$,
S.A.~Tupputi$^\textrm{\scriptsize 22a,22b}$,
S.~Turchikhin$^\textrm{\scriptsize 68}$,
D.~Turgeman$^\textrm{\scriptsize 175}$,
I.~Turk~Cakir$^\textrm{\scriptsize 4b}$$^{,au}$,
R.~Turra$^\textrm{\scriptsize 94a,94b}$,
P.M.~Tuts$^\textrm{\scriptsize 38}$,
G.~Ucchielli$^\textrm{\scriptsize 22a,22b}$,
I.~Ueda$^\textrm{\scriptsize 157}$,
M.~Ughetto$^\textrm{\scriptsize 148a,148b}$,
F.~Ukegawa$^\textrm{\scriptsize 164}$,
G.~Unal$^\textrm{\scriptsize 32}$,
A.~Undrus$^\textrm{\scriptsize 27}$,
G.~Unel$^\textrm{\scriptsize 166}$,
F.C.~Ungaro$^\textrm{\scriptsize 91}$,
Y.~Unno$^\textrm{\scriptsize 69}$,
C.~Unverdorben$^\textrm{\scriptsize 102}$,
J.~Urban$^\textrm{\scriptsize 146b}$,
P.~Urquijo$^\textrm{\scriptsize 91}$,
P.~Urrejola$^\textrm{\scriptsize 86}$,
G.~Usai$^\textrm{\scriptsize 8}$,
J.~Usui$^\textrm{\scriptsize 69}$,
L.~Vacavant$^\textrm{\scriptsize 88}$,
V.~Vacek$^\textrm{\scriptsize 130}$,
B.~Vachon$^\textrm{\scriptsize 90}$,
C.~Valderanis$^\textrm{\scriptsize 102}$,
E.~Valdes~Santurio$^\textrm{\scriptsize 148a,148b}$,
N.~Valencic$^\textrm{\scriptsize 109}$,
S.~Valentinetti$^\textrm{\scriptsize 22a,22b}$,
A.~Valero$^\textrm{\scriptsize 170}$,
L.~Valery$^\textrm{\scriptsize 13}$,
S.~Valkar$^\textrm{\scriptsize 131}$,
J.A.~Valls~Ferrer$^\textrm{\scriptsize 170}$,
W.~Van~Den~Wollenberg$^\textrm{\scriptsize 109}$,
P.C.~Van~Der~Deijl$^\textrm{\scriptsize 109}$,
H.~van~der~Graaf$^\textrm{\scriptsize 109}$,
N.~van~Eldik$^\textrm{\scriptsize 154}$,
P.~van~Gemmeren$^\textrm{\scriptsize 6}$,
J.~Van~Nieuwkoop$^\textrm{\scriptsize 144}$,
I.~van~Vulpen$^\textrm{\scriptsize 109}$,
M.C.~van~Woerden$^\textrm{\scriptsize 109}$,
M.~Vanadia$^\textrm{\scriptsize 134a,134b}$,
W.~Vandelli$^\textrm{\scriptsize 32}$,
R.~Vanguri$^\textrm{\scriptsize 124}$,
A.~Vaniachine$^\textrm{\scriptsize 160}$,
P.~Vankov$^\textrm{\scriptsize 109}$,
G.~Vardanyan$^\textrm{\scriptsize 180}$,
R.~Vari$^\textrm{\scriptsize 134a}$,
E.W.~Varnes$^\textrm{\scriptsize 7}$,
T.~Varol$^\textrm{\scriptsize 43}$,
D.~Varouchas$^\textrm{\scriptsize 83}$,
A.~Vartapetian$^\textrm{\scriptsize 8}$,
K.E.~Varvell$^\textrm{\scriptsize 152}$,
J.G.~Vasquez$^\textrm{\scriptsize 179}$,
G.A.~Vasquez$^\textrm{\scriptsize 34b}$,
F.~Vazeille$^\textrm{\scriptsize 37}$,
T.~Vazquez~Schroeder$^\textrm{\scriptsize 90}$,
J.~Veatch$^\textrm{\scriptsize 57}$,
V.~Veeraraghavan$^\textrm{\scriptsize 7}$,
L.M.~Veloce$^\textrm{\scriptsize 161}$,
F.~Veloso$^\textrm{\scriptsize 128a,128c}$,
S.~Veneziano$^\textrm{\scriptsize 134a}$,
A.~Ventura$^\textrm{\scriptsize 76a,76b}$,
M.~Venturi$^\textrm{\scriptsize 172}$,
N.~Venturi$^\textrm{\scriptsize 161}$,
A.~Venturini$^\textrm{\scriptsize 25}$,
V.~Vercesi$^\textrm{\scriptsize 123a}$,
M.~Verducci$^\textrm{\scriptsize 134a,134b}$,
W.~Verkerke$^\textrm{\scriptsize 109}$,
J.C.~Vermeulen$^\textrm{\scriptsize 109}$,
A.~Vest$^\textrm{\scriptsize 47}$$^{,av}$,
M.C.~Vetterli$^\textrm{\scriptsize 144}$$^{,d}$,
O.~Viazlo$^\textrm{\scriptsize 84}$,
I.~Vichou$^\textrm{\scriptsize 169}$$^{,*}$,
T.~Vickey$^\textrm{\scriptsize 141}$,
O.E.~Vickey~Boeriu$^\textrm{\scriptsize 141}$,
G.H.A.~Viehhauser$^\textrm{\scriptsize 122}$,
S.~Viel$^\textrm{\scriptsize 16}$,
L.~Vigani$^\textrm{\scriptsize 122}$,
M.~Villa$^\textrm{\scriptsize 22a,22b}$,
M.~Villaplana~Perez$^\textrm{\scriptsize 94a,94b}$,
E.~Vilucchi$^\textrm{\scriptsize 50}$,
M.G.~Vincter$^\textrm{\scriptsize 31}$,
V.B.~Vinogradov$^\textrm{\scriptsize 68}$,
C.~Vittori$^\textrm{\scriptsize 22a,22b}$,
I.~Vivarelli$^\textrm{\scriptsize 151}$,
S.~Vlachos$^\textrm{\scriptsize 10}$,
M.~Vlasak$^\textrm{\scriptsize 130}$,
M.~Vogel$^\textrm{\scriptsize 178}$,
P.~Vokac$^\textrm{\scriptsize 130}$,
G.~Volpi$^\textrm{\scriptsize 126a,126b}$,
M.~Volpi$^\textrm{\scriptsize 91}$,
H.~von~der~Schmitt$^\textrm{\scriptsize 103}$,
E.~von~Toerne$^\textrm{\scriptsize 23}$,
V.~Vorobel$^\textrm{\scriptsize 131}$,
K.~Vorobev$^\textrm{\scriptsize 100}$,
M.~Vos$^\textrm{\scriptsize 170}$,
R.~Voss$^\textrm{\scriptsize 32}$,
J.H.~Vossebeld$^\textrm{\scriptsize 77}$,
N.~Vranjes$^\textrm{\scriptsize 14}$,
M.~Vranjes~Milosavljevic$^\textrm{\scriptsize 14}$,
V.~Vrba$^\textrm{\scriptsize 129}$,
M.~Vreeswijk$^\textrm{\scriptsize 109}$,
R.~Vuillermet$^\textrm{\scriptsize 32}$,
I.~Vukotic$^\textrm{\scriptsize 33}$,
P.~Wagner$^\textrm{\scriptsize 23}$,
W.~Wagner$^\textrm{\scriptsize 178}$,
H.~Wahlberg$^\textrm{\scriptsize 74}$,
S.~Wahrmund$^\textrm{\scriptsize 47}$,
J.~Wakabayashi$^\textrm{\scriptsize 105}$,
J.~Walder$^\textrm{\scriptsize 75}$,
R.~Walker$^\textrm{\scriptsize 102}$,
W.~Walkowiak$^\textrm{\scriptsize 143}$,
V.~Wallangen$^\textrm{\scriptsize 148a,148b}$,
C.~Wang$^\textrm{\scriptsize 35b}$,
C.~Wang$^\textrm{\scriptsize 36b}$$^{,aw}$,
F.~Wang$^\textrm{\scriptsize 176}$,
H.~Wang$^\textrm{\scriptsize 16}$,
H.~Wang$^\textrm{\scriptsize 43}$,
J.~Wang$^\textrm{\scriptsize 45}$,
J.~Wang$^\textrm{\scriptsize 152}$,
K.~Wang$^\textrm{\scriptsize 90}$,
R.~Wang$^\textrm{\scriptsize 6}$,
S.M.~Wang$^\textrm{\scriptsize 153}$,
T.~Wang$^\textrm{\scriptsize 38}$,
W.~Wang$^\textrm{\scriptsize 36a}$,
C.~Wanotayaroj$^\textrm{\scriptsize 118}$,
A.~Warburton$^\textrm{\scriptsize 90}$,
C.P.~Ward$^\textrm{\scriptsize 30}$,
D.R.~Wardrope$^\textrm{\scriptsize 81}$,
A.~Washbrook$^\textrm{\scriptsize 49}$,
P.M.~Watkins$^\textrm{\scriptsize 19}$,
A.T.~Watson$^\textrm{\scriptsize 19}$,
M.F.~Watson$^\textrm{\scriptsize 19}$,
G.~Watts$^\textrm{\scriptsize 140}$,
S.~Watts$^\textrm{\scriptsize 87}$,
B.M.~Waugh$^\textrm{\scriptsize 81}$,
S.~Webb$^\textrm{\scriptsize 86}$,
M.S.~Weber$^\textrm{\scriptsize 18}$,
S.W.~Weber$^\textrm{\scriptsize 177}$,
S.A.~Weber$^\textrm{\scriptsize 31}$,
J.S.~Webster$^\textrm{\scriptsize 6}$,
A.R.~Weidberg$^\textrm{\scriptsize 122}$,
B.~Weinert$^\textrm{\scriptsize 64}$,
J.~Weingarten$^\textrm{\scriptsize 57}$,
C.~Weiser$^\textrm{\scriptsize 51}$,
H.~Weits$^\textrm{\scriptsize 109}$,
P.S.~Wells$^\textrm{\scriptsize 32}$,
T.~Wenaus$^\textrm{\scriptsize 27}$,
T.~Wengler$^\textrm{\scriptsize 32}$,
S.~Wenig$^\textrm{\scriptsize 32}$,
N.~Wermes$^\textrm{\scriptsize 23}$,
M.D.~Werner$^\textrm{\scriptsize 67}$,
P.~Werner$^\textrm{\scriptsize 32}$,
M.~Wessels$^\textrm{\scriptsize 60a}$,
J.~Wetter$^\textrm{\scriptsize 165}$,
K.~Whalen$^\textrm{\scriptsize 118}$,
N.L.~Whallon$^\textrm{\scriptsize 140}$,
A.M.~Wharton$^\textrm{\scriptsize 75}$,
A.~White$^\textrm{\scriptsize 8}$,
M.J.~White$^\textrm{\scriptsize 1}$,
R.~White$^\textrm{\scriptsize 34b}$,
D.~Whiteson$^\textrm{\scriptsize 166}$,
F.J.~Wickens$^\textrm{\scriptsize 133}$,
W.~Wiedenmann$^\textrm{\scriptsize 176}$,
M.~Wielers$^\textrm{\scriptsize 133}$,
C.~Wiglesworth$^\textrm{\scriptsize 39}$,
L.A.M.~Wiik-Fuchs$^\textrm{\scriptsize 23}$,
A.~Wildauer$^\textrm{\scriptsize 103}$,
F.~Wilk$^\textrm{\scriptsize 87}$,
H.G.~Wilkens$^\textrm{\scriptsize 32}$,
H.H.~Williams$^\textrm{\scriptsize 124}$,
S.~Williams$^\textrm{\scriptsize 109}$,
C.~Willis$^\textrm{\scriptsize 93}$,
S.~Willocq$^\textrm{\scriptsize 89}$,
J.A.~Wilson$^\textrm{\scriptsize 19}$,
I.~Wingerter-Seez$^\textrm{\scriptsize 5}$,
F.~Winklmeier$^\textrm{\scriptsize 118}$,
O.J.~Winston$^\textrm{\scriptsize 151}$,
B.T.~Winter$^\textrm{\scriptsize 23}$,
M.~Wittgen$^\textrm{\scriptsize 145}$,
T.M.H.~Wolf$^\textrm{\scriptsize 109}$,
R.~Wolff$^\textrm{\scriptsize 88}$,
M.W.~Wolter$^\textrm{\scriptsize 42}$,
H.~Wolters$^\textrm{\scriptsize 128a,128c}$,
S.D.~Worm$^\textrm{\scriptsize 133}$,
B.K.~Wosiek$^\textrm{\scriptsize 42}$,
J.~Wotschack$^\textrm{\scriptsize 32}$,
M.J.~Woudstra$^\textrm{\scriptsize 87}$,
K.W.~Wozniak$^\textrm{\scriptsize 42}$,
M.~Wu$^\textrm{\scriptsize 58}$,
M.~Wu$^\textrm{\scriptsize 33}$,
S.L.~Wu$^\textrm{\scriptsize 176}$,
X.~Wu$^\textrm{\scriptsize 52}$,
Y.~Wu$^\textrm{\scriptsize 92}$,
T.R.~Wyatt$^\textrm{\scriptsize 87}$,
B.M.~Wynne$^\textrm{\scriptsize 49}$,
S.~Xella$^\textrm{\scriptsize 39}$,
Z.~Xi$^\textrm{\scriptsize 92}$,
D.~Xu$^\textrm{\scriptsize 35a}$,
L.~Xu$^\textrm{\scriptsize 27}$,
B.~Yabsley$^\textrm{\scriptsize 152}$,
S.~Yacoob$^\textrm{\scriptsize 147a}$,
D.~Yamaguchi$^\textrm{\scriptsize 159}$,
Y.~Yamaguchi$^\textrm{\scriptsize 120}$,
A.~Yamamoto$^\textrm{\scriptsize 69}$,
S.~Yamamoto$^\textrm{\scriptsize 157}$,
T.~Yamanaka$^\textrm{\scriptsize 157}$,
K.~Yamauchi$^\textrm{\scriptsize 105}$,
Y.~Yamazaki$^\textrm{\scriptsize 70}$,
Z.~Yan$^\textrm{\scriptsize 24}$,
H.~Yang$^\textrm{\scriptsize 36c}$,
H.~Yang$^\textrm{\scriptsize 176}$,
Y.~Yang$^\textrm{\scriptsize 153}$,
Z.~Yang$^\textrm{\scriptsize 15}$,
W-M.~Yao$^\textrm{\scriptsize 16}$,
Y.C.~Yap$^\textrm{\scriptsize 83}$,
Y.~Yasu$^\textrm{\scriptsize 69}$,
E.~Yatsenko$^\textrm{\scriptsize 5}$,
K.H.~Yau~Wong$^\textrm{\scriptsize 23}$,
J.~Ye$^\textrm{\scriptsize 43}$,
S.~Ye$^\textrm{\scriptsize 27}$,
I.~Yeletskikh$^\textrm{\scriptsize 68}$,
E.~Yildirim$^\textrm{\scriptsize 86}$,
K.~Yorita$^\textrm{\scriptsize 174}$,
R.~Yoshida$^\textrm{\scriptsize 6}$,
K.~Yoshihara$^\textrm{\scriptsize 124}$,
C.~Young$^\textrm{\scriptsize 145}$,
C.J.S.~Young$^\textrm{\scriptsize 32}$,
S.~Youssef$^\textrm{\scriptsize 24}$,
D.R.~Yu$^\textrm{\scriptsize 16}$,
J.~Yu$^\textrm{\scriptsize 8}$,
J.M.~Yu$^\textrm{\scriptsize 92}$,
J.~Yu$^\textrm{\scriptsize 67}$,
L.~Yuan$^\textrm{\scriptsize 70}$,
S.P.Y.~Yuen$^\textrm{\scriptsize 23}$,
I.~Yusuff$^\textrm{\scriptsize 30}$$^{,ax}$,
B.~Zabinski$^\textrm{\scriptsize 42}$,
G.~Zacharis$^\textrm{\scriptsize 10}$,
R.~Zaidan$^\textrm{\scriptsize 66}$,
A.M.~Zaitsev$^\textrm{\scriptsize 132}$$^{,ag}$,
N.~Zakharchuk$^\textrm{\scriptsize 45}$,
J.~Zalieckas$^\textrm{\scriptsize 15}$,
A.~Zaman$^\textrm{\scriptsize 150}$,
S.~Zambito$^\textrm{\scriptsize 59}$,
L.~Zanello$^\textrm{\scriptsize 134a,134b}$,
D.~Zanzi$^\textrm{\scriptsize 91}$,
C.~Zeitnitz$^\textrm{\scriptsize 178}$,
M.~Zeman$^\textrm{\scriptsize 130}$,
A.~Zemla$^\textrm{\scriptsize 41a}$,
J.C.~Zeng$^\textrm{\scriptsize 169}$,
Q.~Zeng$^\textrm{\scriptsize 145}$,
O.~Zenin$^\textrm{\scriptsize 132}$,
T.~\v{Z}eni\v{s}$^\textrm{\scriptsize 146a}$,
D.~Zerwas$^\textrm{\scriptsize 119}$,
D.~Zhang$^\textrm{\scriptsize 92}$,
F.~Zhang$^\textrm{\scriptsize 176}$,
G.~Zhang$^\textrm{\scriptsize 36a}$$^{,aq}$,
H.~Zhang$^\textrm{\scriptsize 35b}$,
J.~Zhang$^\textrm{\scriptsize 6}$,
L.~Zhang$^\textrm{\scriptsize 51}$,
L.~Zhang$^\textrm{\scriptsize 36a}$,
M.~Zhang$^\textrm{\scriptsize 169}$,
R.~Zhang$^\textrm{\scriptsize 23}$,
R.~Zhang$^\textrm{\scriptsize 36a}$$^{,aw}$,
X.~Zhang$^\textrm{\scriptsize 36b}$,
Z.~Zhang$^\textrm{\scriptsize 119}$,
X.~Zhao$^\textrm{\scriptsize 43}$,
Y.~Zhao$^\textrm{\scriptsize 36b}$$^{,ay}$,
Z.~Zhao$^\textrm{\scriptsize 36a}$,
A.~Zhemchugov$^\textrm{\scriptsize 68}$,
J.~Zhong$^\textrm{\scriptsize 122}$,
B.~Zhou$^\textrm{\scriptsize 92}$,
C.~Zhou$^\textrm{\scriptsize 176}$,
L.~Zhou$^\textrm{\scriptsize 38}$,
L.~Zhou$^\textrm{\scriptsize 43}$,
M.~Zhou$^\textrm{\scriptsize 150}$,
N.~Zhou$^\textrm{\scriptsize 35c}$,
C.G.~Zhu$^\textrm{\scriptsize 36b}$,
H.~Zhu$^\textrm{\scriptsize 35a}$,
J.~Zhu$^\textrm{\scriptsize 92}$,
Y.~Zhu$^\textrm{\scriptsize 36a}$,
X.~Zhuang$^\textrm{\scriptsize 35a}$,
K.~Zhukov$^\textrm{\scriptsize 98}$,
A.~Zibell$^\textrm{\scriptsize 177}$,
D.~Zieminska$^\textrm{\scriptsize 64}$,
N.I.~Zimine$^\textrm{\scriptsize 68}$,
C.~Zimmermann$^\textrm{\scriptsize 86}$,
S.~Zimmermann$^\textrm{\scriptsize 51}$,
Z.~Zinonos$^\textrm{\scriptsize 57}$,
M.~Zinser$^\textrm{\scriptsize 86}$,
M.~Ziolkowski$^\textrm{\scriptsize 143}$,
L.~\v{Z}ivkovi\'{c}$^\textrm{\scriptsize 14}$,
G.~Zobernig$^\textrm{\scriptsize 176}$,
A.~Zoccoli$^\textrm{\scriptsize 22a,22b}$,
M.~zur~Nedden$^\textrm{\scriptsize 17}$,
L.~Zwalinski$^\textrm{\scriptsize 32}$.
\bigskip
\\
$^{1}$ Department of Physics, University of Adelaide, Adelaide, Australia\\
$^{2}$ Physics Department, SUNY Albany, Albany NY, United States of America\\
$^{3}$ Department of Physics, University of Alberta, Edmonton AB, Canada\\
$^{4}$ $^{(a)}$ Department of Physics, Ankara University, Ankara; $^{(b)}$ Istanbul Aydin University, Istanbul; $^{(c)}$ Division of Physics, TOBB University of Economics and Technology, Ankara, Turkey\\
$^{5}$ LAPP, CNRS/IN2P3 and Universit{\'e} Savoie Mont Blanc, Annecy-le-Vieux, France\\
$^{6}$ High Energy Physics Division, Argonne National Laboratory, Argonne IL, United States of America\\
$^{7}$ Department of Physics, University of Arizona, Tucson AZ, United States of America\\
$^{8}$ Department of Physics, The University of Texas at Arlington, Arlington TX, United States of America\\
$^{9}$ Physics Department, National and Kapodistrian University of Athens, Athens, Greece\\
$^{10}$ Physics Department, National Technical University of Athens, Zografou, Greece\\
$^{11}$ Department of Physics, The University of Texas at Austin, Austin TX, United States of America\\
$^{12}$ Institute of Physics, Azerbaijan Academy of Sciences, Baku, Azerbaijan\\
$^{13}$ Institut de F{\'\i}sica d'Altes Energies (IFAE), The Barcelona Institute of Science and Technology, Barcelona, Spain\\
$^{14}$ Institute of Physics, University of Belgrade, Belgrade, Serbia\\
$^{15}$ Department for Physics and Technology, University of Bergen, Bergen, Norway\\
$^{16}$ Physics Division, Lawrence Berkeley National Laboratory and University of California, Berkeley CA, United States of America\\
$^{17}$ Department of Physics, Humboldt University, Berlin, Germany\\
$^{18}$ Albert Einstein Center for Fundamental Physics and Laboratory for High Energy Physics, University of Bern, Bern, Switzerland\\
$^{19}$ School of Physics and Astronomy, University of Birmingham, Birmingham, United Kingdom\\
$^{20}$ $^{(a)}$ Department of Physics, Bogazici University, Istanbul; $^{(b)}$ Department of Physics Engineering, Gaziantep University, Gaziantep; $^{(d)}$ Istanbul Bilgi University, Faculty of Engineering and Natural Sciences, Istanbul,Turkey; $^{(e)}$ Bahcesehir University, Faculty of Engineering and Natural Sciences, Istanbul, Turkey, Turkey\\
$^{21}$ Centro de Investigaciones, Universidad Antonio Narino, Bogota, Colombia\\
$^{22}$ $^{(a)}$ INFN Sezione di Bologna; $^{(b)}$ Dipartimento di Fisica e Astronomia, Universit{\`a} di Bologna, Bologna, Italy\\
$^{23}$ Physikalisches Institut, University of Bonn, Bonn, Germany\\
$^{24}$ Department of Physics, Boston University, Boston MA, United States of America\\
$^{25}$ Department of Physics, Brandeis University, Waltham MA, United States of America\\
$^{26}$ $^{(a)}$ Universidade Federal do Rio De Janeiro COPPE/EE/IF, Rio de Janeiro; $^{(b)}$ Electrical Circuits Department, Federal University of Juiz de Fora (UFJF), Juiz de Fora; $^{(c)}$ Federal University of Sao Joao del Rei (UFSJ), Sao Joao del Rei; $^{(d)}$ Instituto de Fisica, Universidade de Sao Paulo, Sao Paulo, Brazil\\
$^{27}$ Physics Department, Brookhaven National Laboratory, Upton NY, United States of America\\
$^{28}$ $^{(a)}$ Transilvania University of Brasov, Brasov, Romania; $^{(b)}$ Horia Hulubei National Institute of Physics and Nuclear Engineering, Bucharest; $^{(c)}$ National Institute for Research and Development of Isotopic and Molecular Technologies, Physics Department, Cluj Napoca; $^{(d)}$ University Politehnica Bucharest, Bucharest; $^{(e)}$ West University in Timisoara, Timisoara, Romania\\
$^{29}$ Departamento de F{\'\i}sica, Universidad de Buenos Aires, Buenos Aires, Argentina\\
$^{30}$ Cavendish Laboratory, University of Cambridge, Cambridge, United Kingdom\\
$^{31}$ Department of Physics, Carleton University, Ottawa ON, Canada\\
$^{32}$ CERN, Geneva, Switzerland\\
$^{33}$ Enrico Fermi Institute, University of Chicago, Chicago IL, United States of America\\
$^{34}$ $^{(a)}$ Departamento de F{\'\i}sica, Pontificia Universidad Cat{\'o}lica de Chile, Santiago; $^{(b)}$ Departamento de F{\'\i}sica, Universidad T{\'e}cnica Federico Santa Mar{\'\i}a, Valpara{\'\i}so, Chile\\
$^{35}$ $^{(a)}$ Institute of High Energy Physics, Chinese Academy of Sciences, Beijing; $^{(b)}$ Department of Physics, Nanjing University, Jiangsu; $^{(c)}$ Physics Department, Tsinghua University, Beijing 100084, China\\
$^{36}$ $^{(a)}$ Department of Modern Physics, University of Science and Technology of China, Anhui; $^{(b)}$ School of Physics, Shandong University, Shandong; $^{(c)}$ Department of Physics and Astronomy, Key Laboratory for Particle Physics, Astrophysics and Cosmology, Ministry of Education; Shanghai Key Laboratory for Particle Physics and Cosmology, Shanghai Jiao Tong University, Shanghai(also at PKU-CHEP);, China\\
$^{37}$ Laboratoire de Physique Corpusculaire, Universit{\'e} Clermont Auvergne, Universit{\'e} Blaise Pascal, CNRS/IN2P3, Clermont-Ferrand, France\\
$^{38}$ Nevis Laboratory, Columbia University, Irvington NY, United States of America\\
$^{39}$ Niels Bohr Institute, University of Copenhagen, Kobenhavn, Denmark\\
$^{40}$ $^{(a)}$ INFN Gruppo Collegato di Cosenza, Laboratori Nazionali di Frascati; $^{(b)}$ Dipartimento di Fisica, Universit{\`a} della Calabria, Rende, Italy\\
$^{41}$ $^{(a)}$ AGH University of Science and Technology, Faculty of Physics and Applied Computer Science, Krakow; $^{(b)}$ Marian Smoluchowski Institute of Physics, Jagiellonian University, Krakow, Poland\\
$^{42}$ Institute of Nuclear Physics Polish Academy of Sciences, Krakow, Poland\\
$^{43}$ Physics Department, Southern Methodist University, Dallas TX, United States of America\\
$^{44}$ Physics Department, University of Texas at Dallas, Richardson TX, United States of America\\
$^{45}$ DESY, Hamburg and Zeuthen, Germany\\
$^{46}$ Lehrstuhl f{\"u}r Experimentelle Physik IV, Technische Universit{\"a}t Dortmund, Dortmund, Germany\\
$^{47}$ Institut f{\"u}r Kern-{~}und Teilchenphysik, Technische Universit{\"a}t Dresden, Dresden, Germany\\
$^{48}$ Department of Physics, Duke University, Durham NC, United States of America\\
$^{49}$ SUPA - School of Physics and Astronomy, University of Edinburgh, Edinburgh, United Kingdom\\
$^{50}$ INFN Laboratori Nazionali di Frascati, Frascati, Italy\\
$^{51}$ Fakult{\"a}t f{\"u}r Mathematik und Physik, Albert-Ludwigs-Universit{\"a}t, Freiburg, Germany\\
$^{52}$ Departement  de Physique Nucleaire et Corpusculaire, Universit{\'e} de Gen{\`e}ve, Geneva, Switzerland\\
$^{53}$ $^{(a)}$ INFN Sezione di Genova; $^{(b)}$ Dipartimento di Fisica, Universit{\`a} di Genova, Genova, Italy\\
$^{54}$ $^{(a)}$ E. Andronikashvili Institute of Physics, Iv. Javakhishvili Tbilisi State University, Tbilisi; $^{(b)}$ High Energy Physics Institute, Tbilisi State University, Tbilisi, Georgia\\
$^{55}$ II Physikalisches Institut, Justus-Liebig-Universit{\"a}t Giessen, Giessen, Germany\\
$^{56}$ SUPA - School of Physics and Astronomy, University of Glasgow, Glasgow, United Kingdom\\
$^{57}$ II Physikalisches Institut, Georg-August-Universit{\"a}t, G{\"o}ttingen, Germany\\
$^{58}$ Laboratoire de Physique Subatomique et de Cosmologie, Universit{\'e} Grenoble-Alpes, CNRS/IN2P3, Grenoble, France\\
$^{59}$ Laboratory for Particle Physics and Cosmology, Harvard University, Cambridge MA, United States of America\\
$^{60}$ $^{(a)}$ Kirchhoff-Institut f{\"u}r Physik, Ruprecht-Karls-Universit{\"a}t Heidelberg, Heidelberg; $^{(b)}$ Physikalisches Institut, Ruprecht-Karls-Universit{\"a}t Heidelberg, Heidelberg; $^{(c)}$ ZITI Institut f{\"u}r technische Informatik, Ruprecht-Karls-Universit{\"a}t Heidelberg, Mannheim, Germany\\
$^{61}$ Faculty of Applied Information Science, Hiroshima Institute of Technology, Hiroshima, Japan\\
$^{62}$ $^{(a)}$ Department of Physics, The Chinese University of Hong Kong, Shatin, N.T., Hong Kong; $^{(b)}$ Department of Physics, The University of Hong Kong, Hong Kong; $^{(c)}$ Department of Physics and Institute for Advanced Study, The Hong Kong University of Science and Technology, Clear Water Bay, Kowloon, Hong Kong, China\\
$^{63}$ Department of Physics, National Tsing Hua University, Taiwan, Taiwan\\
$^{64}$ Department of Physics, Indiana University, Bloomington IN, United States of America\\
$^{65}$ Institut f{\"u}r Astro-{~}und Teilchenphysik, Leopold-Franzens-Universit{\"a}t, Innsbruck, Austria\\
$^{66}$ University of Iowa, Iowa City IA, United States of America\\
$^{67}$ Department of Physics and Astronomy, Iowa State University, Ames IA, United States of America\\
$^{68}$ Joint Institute for Nuclear Research, JINR Dubna, Dubna, Russia\\
$^{69}$ KEK, High Energy Accelerator Research Organization, Tsukuba, Japan\\
$^{70}$ Graduate School of Science, Kobe University, Kobe, Japan\\
$^{71}$ Faculty of Science, Kyoto University, Kyoto, Japan\\
$^{72}$ Kyoto University of Education, Kyoto, Japan\\
$^{73}$ Department of Physics, Kyushu University, Fukuoka, Japan\\
$^{74}$ Instituto de F{\'\i}sica La Plata, Universidad Nacional de La Plata and CONICET, La Plata, Argentina\\
$^{75}$ Physics Department, Lancaster University, Lancaster, United Kingdom\\
$^{76}$ $^{(a)}$ INFN Sezione di Lecce; $^{(b)}$ Dipartimento di Matematica e Fisica, Universit{\`a} del Salento, Lecce, Italy\\
$^{77}$ Oliver Lodge Laboratory, University of Liverpool, Liverpool, United Kingdom\\
$^{78}$ Department of Experimental Particle Physics, Jo{\v{z}}ef Stefan Institute and Department of Physics, University of Ljubljana, Ljubljana, Slovenia\\
$^{79}$ School of Physics and Astronomy, Queen Mary University of London, London, United Kingdom\\
$^{80}$ Department of Physics, Royal Holloway University of London, Surrey, United Kingdom\\
$^{81}$ Department of Physics and Astronomy, University College London, London, United Kingdom\\
$^{82}$ Louisiana Tech University, Ruston LA, United States of America\\
$^{83}$ Laboratoire de Physique Nucl{\'e}aire et de Hautes Energies, UPMC and Universit{\'e} Paris-Diderot and CNRS/IN2P3, Paris, France\\
$^{84}$ Fysiska institutionen, Lunds universitet, Lund, Sweden\\
$^{85}$ Departamento de Fisica Teorica C-15, Universidad Autonoma de Madrid, Madrid, Spain\\
$^{86}$ Institut f{\"u}r Physik, Universit{\"a}t Mainz, Mainz, Germany\\
$^{87}$ School of Physics and Astronomy, University of Manchester, Manchester, United Kingdom\\
$^{88}$ CPPM, Aix-Marseille Universit{\'e} and CNRS/IN2P3, Marseille, France\\
$^{89}$ Department of Physics, University of Massachusetts, Amherst MA, United States of America\\
$^{90}$ Department of Physics, McGill University, Montreal QC, Canada\\
$^{91}$ School of Physics, University of Melbourne, Victoria, Australia\\
$^{92}$ Department of Physics, The University of Michigan, Ann Arbor MI, United States of America\\
$^{93}$ Department of Physics and Astronomy, Michigan State University, East Lansing MI, United States of America\\
$^{94}$ $^{(a)}$ INFN Sezione di Milano; $^{(b)}$ Dipartimento di Fisica, Universit{\`a} di Milano, Milano, Italy\\
$^{95}$ B.I. Stepanov Institute of Physics, National Academy of Sciences of Belarus, Minsk, Republic of Belarus\\
$^{96}$ Research Institute for Nuclear Problems of Byelorussian State University, Minsk, Republic of Belarus\\
$^{97}$ Group of Particle Physics, University of Montreal, Montreal QC, Canada\\
$^{98}$ P.N. Lebedev Physical Institute of the Russian Academy of Sciences, Moscow, Russia\\
$^{99}$ Institute for Theoretical and Experimental Physics (ITEP), Moscow, Russia\\
$^{100}$ National Research Nuclear University MEPhI, Moscow, Russia\\
$^{101}$ D.V. Skobeltsyn Institute of Nuclear Physics, M.V. Lomonosov Moscow State University, Moscow, Russia\\
$^{102}$ Fakult{\"a}t f{\"u}r Physik, Ludwig-Maximilians-Universit{\"a}t M{\"u}nchen, M{\"u}nchen, Germany\\
$^{103}$ Max-Planck-Institut f{\"u}r Physik (Werner-Heisenberg-Institut), M{\"u}nchen, Germany\\
$^{104}$ Nagasaki Institute of Applied Science, Nagasaki, Japan\\
$^{105}$ Graduate School of Science and Kobayashi-Maskawa Institute, Nagoya University, Nagoya, Japan\\
$^{106}$ $^{(a)}$ INFN Sezione di Napoli; $^{(b)}$ Dipartimento di Fisica, Universit{\`a} di Napoli, Napoli, Italy\\
$^{107}$ Department of Physics and Astronomy, University of New Mexico, Albuquerque NM, United States of America\\
$^{108}$ Institute for Mathematics, Astrophysics and Particle Physics, Radboud University Nijmegen/Nikhef, Nijmegen, Netherlands\\
$^{109}$ Nikhef National Institute for Subatomic Physics and University of Amsterdam, Amsterdam, Netherlands\\
$^{110}$ Department of Physics, Northern Illinois University, DeKalb IL, United States of America\\
$^{111}$ Budker Institute of Nuclear Physics, SB RAS, Novosibirsk, Russia\\
$^{112}$ Department of Physics, New York University, New York NY, United States of America\\
$^{113}$ Ohio State University, Columbus OH, United States of America\\
$^{114}$ Faculty of Science, Okayama University, Okayama, Japan\\
$^{115}$ Homer L. Dodge Department of Physics and Astronomy, University of Oklahoma, Norman OK, United States of America\\
$^{116}$ Department of Physics, Oklahoma State University, Stillwater OK, United States of America\\
$^{117}$ Palack{\'y} University, RCPTM, Olomouc, Czech Republic\\
$^{118}$ Center for High Energy Physics, University of Oregon, Eugene OR, United States of America\\
$^{119}$ LAL, Univ. Paris-Sud, CNRS/IN2P3, Universit{\'e} Paris-Saclay, Orsay, France\\
$^{120}$ Graduate School of Science, Osaka University, Osaka, Japan\\
$^{121}$ Department of Physics, University of Oslo, Oslo, Norway\\
$^{122}$ Department of Physics, Oxford University, Oxford, United Kingdom\\
$^{123}$ $^{(a)}$ INFN Sezione di Pavia; $^{(b)}$ Dipartimento di Fisica, Universit{\`a} di Pavia, Pavia, Italy\\
$^{124}$ Department of Physics, University of Pennsylvania, Philadelphia PA, United States of America\\
$^{125}$ National Research Centre "Kurchatov Institute" B.P.Konstantinov Petersburg Nuclear Physics Institute, St. Petersburg, Russia\\
$^{126}$ $^{(a)}$ INFN Sezione di Pisa; $^{(b)}$ Dipartimento di Fisica E. Fermi, Universit{\`a} di Pisa, Pisa, Italy\\
$^{127}$ Department of Physics and Astronomy, University of Pittsburgh, Pittsburgh PA, United States of America\\
$^{128}$ $^{(a)}$ Laborat{\'o}rio de Instrumenta{\c{c}}{\~a}o e F{\'\i}sica Experimental de Part{\'\i}culas - LIP, Lisboa; $^{(b)}$ Faculdade de Ci{\^e}ncias, Universidade de Lisboa, Lisboa; $^{(c)}$ Department of Physics, University of Coimbra, Coimbra; $^{(d)}$ Centro de F{\'\i}sica Nuclear da Universidade de Lisboa, Lisboa; $^{(e)}$ Departamento de Fisica, Universidade do Minho, Braga; $^{(f)}$ Departamento de Fisica Teorica y del Cosmos and CAFPE, Universidad de Granada, Granada (Spain); $^{(g)}$ Dep Fisica and CEFITEC of Faculdade de Ciencias e Tecnologia, Universidade Nova de Lisboa, Caparica, Portugal\\
$^{129}$ Institute of Physics, Academy of Sciences of the Czech Republic, Praha, Czech Republic\\
$^{130}$ Czech Technical University in Prague, Praha, Czech Republic\\
$^{131}$ Charles University, Faculty of Mathematics and Physics, Prague, Czech Republic\\
$^{132}$ State Research Center Institute for High Energy Physics (Protvino), NRC KI, Russia\\
$^{133}$ Particle Physics Department, Rutherford Appleton Laboratory, Didcot, United Kingdom\\
$^{134}$ $^{(a)}$ INFN Sezione di Roma; $^{(b)}$ Dipartimento di Fisica, Sapienza Universit{\`a} di Roma, Roma, Italy\\
$^{135}$ $^{(a)}$ INFN Sezione di Roma Tor Vergata; $^{(b)}$ Dipartimento di Fisica, Universit{\`a} di Roma Tor Vergata, Roma, Italy\\
$^{136}$ $^{(a)}$ INFN Sezione di Roma Tre; $^{(b)}$ Dipartimento di Matematica e Fisica, Universit{\`a} Roma Tre, Roma, Italy\\
$^{137}$ $^{(a)}$ Facult{\'e} des Sciences Ain Chock, R{\'e}seau Universitaire de Physique des Hautes Energies - Universit{\'e} Hassan II, Casablanca; $^{(b)}$ Centre National de l'Energie des Sciences Techniques Nucleaires, Rabat; $^{(c)}$ Facult{\'e} des Sciences Semlalia, Universit{\'e} Cadi Ayyad, LPHEA-Marrakech; $^{(d)}$ Facult{\'e} des Sciences, Universit{\'e} Mohamed Premier and LPTPM, Oujda; $^{(e)}$ Facult{\'e} des sciences, Universit{\'e} Mohammed V, Rabat, Morocco\\
$^{138}$ DSM/IRFU (Institut de Recherches sur les Lois Fondamentales de l'Univers), CEA Saclay (Commissariat {\`a} l'Energie Atomique et aux Energies Alternatives), Gif-sur-Yvette, France\\
$^{139}$ Santa Cruz Institute for Particle Physics, University of California Santa Cruz, Santa Cruz CA, United States of America\\
$^{140}$ Department of Physics, University of Washington, Seattle WA, United States of America\\
$^{141}$ Department of Physics and Astronomy, University of Sheffield, Sheffield, United Kingdom\\
$^{142}$ Department of Physics, Shinshu University, Nagano, Japan\\
$^{143}$ Fachbereich Physik, Universit{\"a}t Siegen, Siegen, Germany\\
$^{144}$ Department of Physics, Simon Fraser University, Burnaby BC, Canada\\
$^{145}$ SLAC National Accelerator Laboratory, Stanford CA, United States of America\\
$^{146}$ $^{(a)}$ Faculty of Mathematics, Physics {\&} Informatics, Comenius University, Bratislava; $^{(b)}$ Department of Subnuclear Physics, Institute of Experimental Physics of the Slovak Academy of Sciences, Kosice, Slovak Republic\\
$^{147}$ $^{(a)}$ Department of Physics, University of Cape Town, Cape Town; $^{(b)}$ Department of Physics, University of Johannesburg, Johannesburg; $^{(c)}$ School of Physics, University of the Witwatersrand, Johannesburg, South Africa\\
$^{148}$ $^{(a)}$ Department of Physics, Stockholm University; $^{(b)}$ The Oskar Klein Centre, Stockholm, Sweden\\
$^{149}$ Physics Department, Royal Institute of Technology, Stockholm, Sweden\\
$^{150}$ Departments of Physics {\&} Astronomy and Chemistry, Stony Brook University, Stony Brook NY, United States of America\\
$^{151}$ Department of Physics and Astronomy, University of Sussex, Brighton, United Kingdom\\
$^{152}$ School of Physics, University of Sydney, Sydney, Australia\\
$^{153}$ Institute of Physics, Academia Sinica, Taipei, Taiwan\\
$^{154}$ Department of Physics, Technion: Israel Institute of Technology, Haifa, Israel\\
$^{155}$ Raymond and Beverly Sackler School of Physics and Astronomy, Tel Aviv University, Tel Aviv, Israel\\
$^{156}$ Department of Physics, Aristotle University of Thessaloniki, Thessaloniki, Greece\\
$^{157}$ International Center for Elementary Particle Physics and Department of Physics, The University of Tokyo, Tokyo, Japan\\
$^{158}$ Graduate School of Science and Technology, Tokyo Metropolitan University, Tokyo, Japan\\
$^{159}$ Department of Physics, Tokyo Institute of Technology, Tokyo, Japan\\
$^{160}$ Tomsk State University, Tomsk, Russia, Russia\\
$^{161}$ Department of Physics, University of Toronto, Toronto ON, Canada\\
$^{162}$ $^{(a)}$ INFN-TIFPA; $^{(b)}$ University of Trento, Trento, Italy, Italy\\
$^{163}$ $^{(a)}$ TRIUMF, Vancouver BC; $^{(b)}$ Department of Physics and Astronomy, York University, Toronto ON, Canada\\
$^{164}$ Faculty of Pure and Applied Sciences, and Center for Integrated Research in Fundamental Science and Engineering, University of Tsukuba, Tsukuba, Japan\\
$^{165}$ Department of Physics and Astronomy, Tufts University, Medford MA, United States of America\\
$^{166}$ Department of Physics and Astronomy, University of California Irvine, Irvine CA, United States of America\\
$^{167}$ $^{(a)}$ INFN Gruppo Collegato di Udine, Sezione di Trieste, Udine; $^{(b)}$ ICTP, Trieste; $^{(c)}$ Dipartimento di Chimica, Fisica e Ambiente, Universit{\`a} di Udine, Udine, Italy\\
$^{168}$ Department of Physics and Astronomy, University of Uppsala, Uppsala, Sweden\\
$^{169}$ Department of Physics, University of Illinois, Urbana IL, United States of America\\
$^{170}$ Instituto de Fisica Corpuscular (IFIC) and Departamento de Fisica Atomica, Molecular y Nuclear and Departamento de Ingenier{\'\i}a Electr{\'o}nica and Instituto de Microelectr{\'o}nica de Barcelona (IMB-CNM), University of Valencia and CSIC, Valencia, Spain\\
$^{171}$ Department of Physics, University of British Columbia, Vancouver BC, Canada\\
$^{172}$ Department of Physics and Astronomy, University of Victoria, Victoria BC, Canada\\
$^{173}$ Department of Physics, University of Warwick, Coventry, United Kingdom\\
$^{174}$ Waseda University, Tokyo, Japan\\
$^{175}$ Department of Particle Physics, The Weizmann Institute of Science, Rehovot, Israel\\
$^{176}$ Department of Physics, University of Wisconsin, Madison WI, United States of America\\
$^{177}$ Fakult{\"a}t f{\"u}r Physik und Astronomie, Julius-Maximilians-Universit{\"a}t, W{\"u}rzburg, Germany\\
$^{178}$ Fakult{\"a}t f{\"u}r Mathematik und Naturwissenschaften, Fachgruppe Physik, Bergische Universit{\"a}t Wuppertal, Wuppertal, Germany\\
$^{179}$ Department of Physics, Yale University, New Haven CT, United States of America\\
$^{180}$ Yerevan Physics Institute, Yerevan, Armenia\\
$^{181}$ Centre de Calcul de l'Institut National de Physique Nucl{\'e}aire et de Physique des Particules (IN2P3), Villeurbanne, France\\
$^{a}$ Also at Department of Physics, King's College London, London, United Kingdom\\
$^{b}$ Also at Institute of Physics, Azerbaijan Academy of Sciences, Baku, Azerbaijan\\
$^{c}$ Also at Novosibirsk State University, Novosibirsk, Russia\\
$^{d}$ Also at TRIUMF, Vancouver BC, Canada\\
$^{e}$ Also at Department of Physics {\&} Astronomy, University of Louisville, Louisville, KY, United States of America\\
$^{f}$ Also at Physics Department, An-Najah National University, Nablus, Palestine\\
$^{g}$ Also at Department of Physics, California State University, Fresno CA, United States of America\\
$^{h}$ Also at Department of Physics, University of Fribourg, Fribourg, Switzerland\\
$^{i}$ Also at Departament de Fisica de la Universitat Autonoma de Barcelona, Barcelona, Spain\\
$^{j}$ Also at Departamento de Fisica e Astronomia, Faculdade de Ciencias, Universidade do Porto, Portugal\\
$^{k}$ Also at Tomsk State University, Tomsk, Russia, Russia\\
$^{l}$ Also at The Collaborative Innovation Center of Quantum Matter (CICQM), Beijing, China\\
$^{m}$ Also at Universita di Napoli Parthenope, Napoli, Italy\\
$^{n}$ Also at Institute of Particle Physics (IPP), Canada\\
$^{o}$ Also at Horia Hulubei National Institute of Physics and Nuclear Engineering, Bucharest, Romania\\
$^{p}$ Also at Department of Physics, St. Petersburg State Polytechnical University, St. Petersburg, Russia\\
$^{q}$ Also at Department of Physics, The University of Michigan, Ann Arbor MI, United States of America\\
$^{r}$ Also at Centre for High Performance Computing, CSIR Campus, Rosebank, Cape Town, South Africa\\
$^{s}$ Also at Louisiana Tech University, Ruston LA, United States of America\\
$^{t}$ Also at Institucio Catalana de Recerca i Estudis Avancats, ICREA, Barcelona, Spain\\
$^{u}$ Also at Graduate School of Science, Osaka University, Osaka, Japan\\
$^{v}$ Also at Institute for Mathematics, Astrophysics and Particle Physics, Radboud University Nijmegen/Nikhef, Nijmegen, Netherlands\\
$^{w}$ Also at Department of Physics, The University of Texas at Austin, Austin TX, United States of America\\
$^{x}$ Also at Institute of Theoretical Physics, Ilia State University, Tbilisi, Georgia\\
$^{y}$ Also at CERN, Geneva, Switzerland\\
$^{z}$ Also at Georgian Technical University (GTU),Tbilisi, Georgia\\
$^{aa}$ Also at Ochadai Academic Production, Ochanomizu University, Tokyo, Japan\\
$^{ab}$ Also at Manhattan College, New York NY, United States of America\\
$^{ac}$ Also at Academia Sinica Grid Computing, Institute of Physics, Academia Sinica, Taipei, Taiwan\\
$^{ad}$ Also at School of Physics, Shandong University, Shandong, China\\
$^{ae}$ Also at Departamento de Fisica Teorica y del Cosmos and CAFPE, Universidad de Granada, Granada (Spain), Portugal\\
$^{af}$ Also at Department of Physics, California State University, Sacramento CA, United States of America\\
$^{ag}$ Also at Moscow Institute of Physics and Technology State University, Dolgoprudny, Russia\\
$^{ah}$ Also at Departement  de Physique Nucleaire et Corpusculaire, Universit{\'e} de Gen{\`e}ve, Geneva, Switzerland\\
$^{ai}$ Also at Eotvos Lorand University, Budapest, Hungary\\
$^{aj}$ Also at Departments of Physics {\&} Astronomy and Chemistry, Stony Brook University, Stony Brook NY, United States of America\\
$^{ak}$ Also at International School for Advanced Studies (SISSA), Trieste, Italy\\
$^{al}$ Also at Department of Physics and Astronomy, University of South Carolina, Columbia SC, United States of America\\
$^{am}$ Also at Institut de F{\'\i}sica d'Altes Energies (IFAE), The Barcelona Institute of Science and Technology, Barcelona, Spain\\
$^{an}$ Also at School of Physics, Sun Yat-sen University, Guangzhou, China\\
$^{ao}$ Also at Institute for Nuclear Research and Nuclear Energy (INRNE) of the Bulgarian Academy of Sciences, Sofia, Bulgaria\\
$^{ap}$ Also at Faculty of Physics, M.V.Lomonosov Moscow State University, Moscow, Russia\\
$^{aq}$ Also at Institute of Physics, Academia Sinica, Taipei, Taiwan\\
$^{ar}$ Also at National Research Nuclear University MEPhI, Moscow, Russia\\
$^{as}$ Also at Department of Physics, Stanford University, Stanford CA, United States of America\\
$^{at}$ Also at Institute for Particle and Nuclear Physics, Wigner Research Centre for Physics, Budapest, Hungary\\
$^{au}$ Also at Giresun University, Faculty of Engineering, Turkey\\
$^{av}$ Also at Flensburg University of Applied Sciences, Flensburg, Germany\\
$^{aw}$ Also at CPPM, Aix-Marseille Universit{\'e} and CNRS/IN2P3, Marseille, France\\
$^{ax}$ Also at University of Malaya, Department of Physics, Kuala Lumpur, Malaysia\\
$^{ay}$ Also at LAL, Univ. Paris-Sud, CNRS/IN2P3, Universit{\'e} Paris-Saclay, Orsay, France\\
$^{*}$ Deceased
\end{flushleft}

%\end{document}
% Created with xml2latex.py

Combination_table.tex
\begin{table}[t]
%\renewcommand{\arraystretch}{1.5}
\centering
\begin{tabular}{|c|r@{\,}@{$\pm$}@{\;}r@{\,}@{$\pm$}@{\;}r@{\,}@{$\pm$}@{\;}r|}
\hline\hline
Jet multiplicity & \multicolumn{4}{c|}{Measured cross section} \\
                 & \multicolumn{4}{c|}{$\pm$\,(stat.)\,$\pm$\,(syst.)\,$\pm$\,(lumi.) [pb]} \\
\hline\hline
& \multicolumn{4}{c|}{$Z \to \ell\ell$}\\
\hline\hline
$\geq\mathrm{0~jets}$ & \numRP{739.8599854}{0} & \numRP{0.6764300}{0} & \numRP{22.9845414}{0} & \numRP{15.6192920}{0} \\
$\geq\mathrm{1~jets}$ & \numRP{116.0000000}{1} & \numRP{0.2803500}{1} &  \numRP{9.6737257}{1} &  \numRP{2.4914574}{1} \\
$\geq\mathrm{2~jets}$ &  \numRP{26.9850006}{1} & \numRP{0.1057000}{1} &  \numRP{2.8482613}{1} &  \numRP{0.6013228}{1} \\
$\geq\mathrm{3~jets}$ &   \numRP{6.2037001}{2} & \numRP{0.0424930}{2} &  \numRP{0.8174381}{2} &  \numRP{0.1440070}{2} \\
$\geq\mathrm{4~jets}$ &   \numRP{1.4823000}{2} & \numRP{0.0191580}{2} &  \numRP{0.2309641}{2} &  \numRP{0.0357457}{2} \\
$\geq\mathrm{5~jets}$ &   \numRP{0.3554200}{2} & \numRP{0.0089666}{2} &  \numRP{0.0669050}{2} &  \numRP{0.0088749}{2} \\
$\geq\mathrm{6~jets}$ &   \numRP{0.0787690}{3} & \numRP{0.0040509}{3} &  \numRP{0.0178664}{3} &  \numRP{0.0020621}{3} \\
$\geq\mathrm{7~jets}$ &   \numRP{0.0177740}{4} & \numRP{0.0018656}{4} &  \numRP{0.0049071}{4} &  \numRP{0.0004867}{4} \\
\hline\hline
\end{tabular}
\caption{Measured combined fiducial cross sections for successive inclusive jet multiplicities.
%The values are given with respect to the dressed definition.
The statistical, systematic, and luminosity uncertainties are given.}
\label{tab:zjets_njet_comb}
\end{table}

\begin{table}[t]
%\renewcommand{\arraystretch}{1.5}
\centering
\begin{tabular}{|c|l@{\,}@{$\pm$}@{\;}l@{\,}@{$\pm$}@{\;}l@{\,}@{$\pm$}@{\;}l|}
\hline\hline
Jet multiplicity & \multicolumn{4}{c|}{Measured cross-section ratio} \\
                 & \multicolumn{4}{c|}{$\pm$\,(stat.)\,$\pm$\,(syst.)\,$\pm$\,(lumi.)} \\
\hline\hline
& \multicolumn{4}{c|}{$Z \to \ell\ell$}\\
\hline\hline
$\geq\mathrm{1~jets}~/\geq\mathrm{0~jets}$ & \numRP{0.1567600}{4} & \numRP{0.0004068}{4} & \numRP{0.0130991}{4} & \numRP{0.0000575}{4} \\
$\geq\mathrm{2~jets}~/\geq\mathrm{1~jets}$ & \numRP{0.2326700}{4} & \numRP{0.0010731}{4} & \numRP{0.0092790}{4} & \numRP{0.0001873}{4} \\
$\geq\mathrm{3~jets}~/\geq\mathrm{2~jets}$ & \numRP{0.2299200}{4} & \numRP{0.0018116}{4} & \numRP{0.0094696}{4} & \numRP{0.0002136}{4} \\
$\geq\mathrm{4~jets}~/\geq\mathrm{3~jets}$ & \numRP{0.2389500}{4} & \numRP{0.0034898}{4} & \numRP{0.0094214}{4} & \numRP{0.0002154}{4} \\
$\geq\mathrm{5~jets}~/\geq\mathrm{4~jets}$ & \numRP{0.2396800}{4} & \numRP{0.0067851}{4} & \numRP{0.0110975}{4} & \numRP{0.0002050}{4} \\
$\geq\mathrm{6~jets}~/\geq\mathrm{5~jets}$ & \numRP{0.2213400}{4} & \numRP{0.0126790}{4} & \numRP{0.0122535}{4} & \numRP{0.0002669}{4} \\
$\geq\mathrm{7~jets}~/\geq\mathrm{6~jets}$ & \numRP{0.2240300}{4} & \numRP{0.0264230}{4} & \numRP{0.0222400}{4} & \numRP{0.0002521}{4} \\
\hline\hline
\end{tabular}
\caption{Measured combined ratios of the fiducial cross sections for successive inclusive jet multiplicities. 
%The values are given with respect to the dressed definition. 
The statistical, systematic, and luminosity uncertainties are given.}
\label{tab:zjets_njet_ratio_comb}
\end{table}

Results_table_single_cross_noratio.tex
\begin{table}[t]
%\renewcommand{\arraystretch}{1.5}
\centering
\begin{tabular}{|c|r@{\,}@{$\pm$}@{\;}r@{\,}@{$\pm$}@{\;}r@{\,}@{$\pm$}@{\;}r|r@{\,}@{$\pm$}@{\;}r@{\,}@{$\pm$}@{\;}r@{\,}@{$\pm$}@{\;}r|}
\hline\hline
Jet & \multicolumn{8}{c|}{Measured cross section $\pm$\,(stat.)\,$\pm$\,(syst.)\,$\pm$\,(lumi.)   [pb]} \\
\cline{2-9}\cline{2-9}
multiplicity & \multicolumn{4}{c|}{$Z \to ee$} & \multicolumn{4}{c|}{$Z \to \mu\mu$}\\ 
\hline\hline
$\geq\mathrm{0~jets}$ & \numRP{742.6131254}{0} & \numRP{0.6560087}{0} & \numRP{24.1232395}{0} & \numRP{15.6790915}{0}
                      & \numRP{738.4631887}{0} & \numRP{0.5785262}{0} & \numRP{23.4250717}{0} & \numRP{15.5881443}{0} \\
$\geq\mathrm{1~jets}$ & \numRP{116.6183205}{1} & \numRP{0.2697211}{1} &  \numRP{9.8539801}{1} &  \numRP{2.5056422}{1}
                      & \numRP{115.6865698}{1} & \numRP{0.2400960}{1} &  \numRP{9.7178793}{1} &  \numRP{2.4838357}{1} \\
$\geq\mathrm{2~jets}$ &  \numRP{27.0842355}{1} & \numRP{0.1258711}{1} &  \numRP{2.9171276}{1} &  \numRP{0.6042993}{1}
                      &  \numRP{26.9592355}{1} & \numRP{0.1120992}{1} &  \numRP{2.8405800}{1} &  \numRP{0.5999904}{1} \\
$\geq\mathrm{3~jets}$ &   \numRP{6.2010092}{2} & \numRP{0.0581154}{2} &  \numRP{0.8179384}{2} &  \numRP{0.1442643}{2}
                      &   \numRP{6.2192955}{2} & \numRP{0.0525592}{2} &  \numRP{0.8330854}{2} &  \numRP{0.1440473}{2} \\
$\geq\mathrm{4~jets}$ &   \numRP{1.4870271}{2} & \numRP{0.0277629}{2} &  \numRP{0.2341416}{2} &  \numRP{0.0360207}{2}
                      &   \numRP{1.4819739}{2} & \numRP{0.0251189}{2} &  \numRP{0.2338763}{2} &  \numRP{0.0355780}{2} \\
$\geq\mathrm{5~jets}$ &   \numRP{0.3566019}{3} & \numRP{0.0132320}{3} &  \numRP{0.0690235}{3} &  \numRP{0.0089792}{3}
                      &   \numRP{0.3544801}{3} & \numRP{0.0119510}{3} &  \numRP{0.0682254}{3} &  \numRP{0.0087775}{3} \\
$\geq\mathrm{6~jets}$ &   \numRP{0.0817674}{3} & \numRP{0.0062634}{3} &  \numRP{0.0191435}{3} &  \numRP{0.0021483}{3}
                      &   \numRP{0.0755170}{3} & \numRP{0.0054169}{3} &  \numRP{0.0185040}{3} &  \numRP{0.0019692}{3} \\
$\geq\mathrm{7~jets}$ &   \numRP{0.0179856}{4} & \numRP{0.0028686}{4} &  \numRP{0.0051447}{4} &  \numRP{0.0004971}{4}
                      &   \numRP{0.0165519}{4} & \numRP{0.0026949}{4} &  \numRP{0.0059834}{4} &  \numRP{0.0004460}{4} \\
\hline\hline
\end{tabular}
\caption{Measured fiducial cross sections in the electron and muon channels for successive inclusive jet multiplicities. 
%The values are given with respect to the dressed definition. 
The total statistical and systematic uncertainties are given, along with the uncertainty in the luminosity.}
\label{tab:zjets_njet}
\end{table}

Systematics_table.tex
\begin{table}[t]
\centering
\begin{footnotesize}
\begin{tabular}{|l|r|r|r|r|r|r|r|r|}
\hline\hline
\multicolumn{9}{|c|} {Relative uncertainty in $\sigma(\ZNj)$ [\%] }\\\hline
& \multicolumn{8}{c|}{\Ztoee}  \\\hline  
Systematic source &
$\texttt{+}\geq\text{0~jets}$ &
$\texttt{+}\geq\text{1~jets}$ &
$\texttt{+}\geq\text{2~jets}$ &
$\texttt{+}\geq\text{3~jets}$ &
$\texttt{+}\geq\text{4~jets}$ &
$\texttt{+}\geq\text{5~jets}$ &
$\texttt{+}\geq\text{6~jets}$ &
$\texttt{+}\geq\text{7~jets}$ \\\hline  
Electron trigger       & \numRP{0.0719}{1} & \numRP{0.0757}{1} & \numRP{0.0727}{1} & \numRP{0.1571}{1} & \numRP{0.2140}{1} & \numRP{0.1635}{1} & \numRP{0.2540}{1} & \numRP{0.2757}{1} \\
Electron selection     & \numRP{1.1546}{1} & \numRP{1.5635}{1} & \numRP{1.8100}{1} & \numRP{1.8707}{1} & \numRP{2.2542}{1} & \numRP{2.6626}{1} & \numRP{2.9421}{1} & \numRP{3.8011}{1} \\
%Jet energy scale       & \numRP{0.0485}{1} & \numRP{6.6330}{1} & \numRP{9.1967}{1} & \numRP{11.5040}{1} & \numRP{13.7779}{1} & \numRP{17.2934}{1} & \numRP{20.5630}{1} & \numRP{23.6686}{1} \\
%Jet energy resolution  & \numRP{0.0265}{1} & \numRP{3.7428}{1} & \numRP{3.7497}{1} & \numRP{4.4201}{1} & \numRP{5.2532}{1} & \numRP{5.1719}{1} & \numRP{6.1797}{1} & \numRP{7.2990}{1} \\
%Jet vertex tagger      & \numRP{0.0095}{1} & \numRP{1.2748}{1} & \numRP{2.1030}{1} & \numRP{2.8384}{1} & \numRP{3.6007}{1} & \numRP{4.5365}{1} & \numRP{5.5114}{1} & \numRP{6.3037}{1} \\
Jet energy scale       &            $<0.1$ & \numRP{6.6330}{1} & \numRP{9.1967}{1} & \numRP{11.5040}{1} & \numRP{13.7779}{1} & \numRP{17.2934}{1} & \numRP{20.5630}{1} & \numRP{23.6686}{1} \\
Jet energy resolution  &            $<0.1$ & \numRP{3.7428}{1} & \numRP{3.7497}{1} & \numRP{4.4201}{1} & \numRP{5.2532}{1} & \numRP{5.1719}{1} & \numRP{6.1797}{1} & \numRP{7.2990}{1} \\
Jet vertex tagger      &            $<0.1$ & \numRP{1.2748}{1} & \numRP{2.1030}{1} & \numRP{2.8384}{1} & \numRP{3.6007}{1} & \numRP{4.5365}{1} & \numRP{5.5114}{1} & \numRP{6.3037}{1} \\
Pile-up                & \numRP{0.4262}{1} & \numRP{0.1924}{1} & \numRP{0.0834}{1} & \numRP{0.1937}{1} & \numRP{0.1990}{1} & \numRP{0.0680}{1} & \numRP{0.4433}{1} & \numRP{0.7767}{1} \\
Luminosity             & \numRP{2.1113}{1} & \numRP{2.1486}{1} & \numRP{2.2312}{1} & \numRP{2.3265}{1} & \numRP{2.4223}{1} & \numRP{2.5180}{1} & \numRP{2.6274}{1} & \numRP{2.7638}{1} \\
Unfolding              & \numRP{3.0020}{1} & \numRP{3.0150}{1} & \numRP{3.0300}{1} & \numRP{3.0278}{1} & \numRP{3.0444}{1} & \numRP{3.0848}{1} & \numRP{3.1107}{1} & \numRP{3.2463}{1} \\
Background             & \numRP{0.1288}{1} & \numRP{0.3269}{1} & \numRP{0.5677}{1} & \numRP{1.0406}{1} & \numRP{1.6342}{1} & \numRP{3.2801}{1} & \numRP{5.9866}{1} & \numRP{11.6266}{1} \\
\hline
Total syst. uncertainty      & \numRP{3.8744}{1} & \numRP{8.7194}{1} & \numRP{10.9994}{1} & \numRP{13.3942}{1} & \numRP{15.9309}{1} & \numRP{19.5191}{1} & \numRP{23.5594}{1} & \numRP{28.7378}{1} \\
\hline
Stat. uncertainty      & \numRP{0.0883}{1} & \numRP{0.2313}{1} & \numRP{0.4647}{1} & \numRP{0.9372}{1} & \numRP{1.8670}{1} & \numRP{3.7106}{1} & \numRP{7.6600}{1} & \numRP{15.9497}{1} \\
\hline\hline
& \multicolumn{8}{c|}{\Ztomm}  \\\hline  
Systematic source &
$\texttt{+}\geq\text{0~jets}$ &
$\texttt{+}\geq\text{1~jets}$ &
$\texttt{+}\geq\text{2~jets}$ &
$\texttt{+}\geq\text{3~jets}$ &
$\texttt{+}\geq\text{4~jets}$ &
$\texttt{+}\geq\text{5~jets}$ &
$\texttt{+}\geq\text{6~jets}$ &
$\texttt{+}\geq\text{7~jets}$ \\\hline  
Muon trigger           & \numRP{0.4313}{1} & \numRP{0.4553}{1} & \numRP{0.3933}{1} & \numRP{0.4764}{1} & \numRP{0.3796}{1} & \numRP{0.4663}{1} & \numRP{0.8860}{1} & \numRP{0.6118}{1} \\
Muon selection         & \numRP{0.8130}{1} & \numRP{0.8879}{1} & \numRP{0.9501}{1} & \numRP{1.0017}{1} & \numRP{1.0252}{1} & \numRP{1.5282}{1} & \numRP{4.2222}{1} & \numRP{16.5887}{1} \\
%Jet energy scale       & \numRP{0.0213}{1} & \numRP{6.7575}{1} & \numRP{9.1080}{1} & \numRP{11.8950}{1} & \numRP{14.0308}{1} & \numRP{16.9759}{1} & \numRP{20.9403}{1} & \numRP{23.6833}{1} \\
%Jet energy resolution  & \numRP{0.0082}{1} & \numRP{3.6083}{1} & \numRP{3.6004}{1} & \numRP{4.1285}{1} & \numRP{5.0434}{1} & \numRP{5.8645}{1} & \numRP{6.1655}{1} & \numRP{9.3093}{1} \\
%Jet vertex tagger      & \numRP{0.0047}{1} & \numRP{1.2623}{1} & \numRP{2.1000}{1} & \numRP{3.0523}{1} & \numRP{3.5924}{1} & \numRP{4.3715}{1} & \numRP{5.6099}{1} & \numRP{6.5514}{1} \\
Jet energy scale       &            $<0.1$ & \numRP{6.7575}{1} & \numRP{9.1080}{1} & \numRP{11.8950}{1} & \numRP{14.0308}{1} & \numRP{16.9759}{1} & \numRP{20.9403}{1} & \numRP{23.6833}{1} \\
Jet energy resolution  &            $<0.1$ & \numRP{3.6083}{1} & \numRP{3.6004}{1} & \numRP{4.1285}{1} & \numRP{5.0434}{1} & \numRP{5.8645}{1} & \numRP{6.1655}{1} & \numRP{9.3093}{1} \\
Jet vertex tagger      &            $<0.1$ & \numRP{1.2623}{1} & \numRP{2.1000}{1} & \numRP{3.0523}{1} & \numRP{3.5924}{1} & \numRP{4.3715}{1} & \numRP{5.6099}{1} & \numRP{6.5514}{1} \\
Pile-up                & \numRP{0.4245}{1} & \numRP{0.0649}{1} & $<0.1$ & \numRP{0.2644}{1} & \numRP{0.5164}{1} & \numRP{0.0785}{1} & \numRP{0.4459}{1} & \numRP{0.9438}{1} \\
Luminosity             & \numRP{2.1109}{1} & \numRP{2.1470}{1} & \numRP{2.2255}{1} & \numRP{2.3161}{1} & \numRP{2.4007}{1} & \numRP{2.4762}{1} & \numRP{2.6076}{1} & \numRP{2.6945}{1} \\
Unfolding              & \numRP{3.0014}{1} & \numRP{3.0108}{1} & \numRP{3.0197}{1} & \numRP{3.0296}{1} & \numRP{3.0306}{1} & \numRP{3.0625}{1} & \numRP{3.0900}{1} & \numRP{3.2130}{1} \\
Background             & \numRP{0.1572}{1} & \numRP{0.4147}{1} & \numRP{0.6419}{1} & \numRP{0.9021}{1} & \numRP{1.6971}{1} & \numRP{4.0293}{1} & \numRP{7.4036}{1} & \numRP{12.8994}{1} \\
\hline
Total syst. uncertainty      & \numRP{3.8104}{1} & \numRP{8.6704}{1} & \numRP{10.7691}{1} & \numRP{13.5939}{1} & \numRP{15.9630}{1} & \numRP{19.4053}{1} & \numRP{24.6417}{1} & \numRP{36.2525}{1} \\
\hline
Stat. uncertainty      & \numRP{0.0783}{1} & \numRP{0.2075}{1} & \numRP{0.4158}{1} & \numRP{0.8451}{1} & \numRP{1.6950}{1} & \numRP{3.3714}{1} & \numRP{7.1731}{1} & \numRP{16.2815}{1} \\
\hline\hline
\end{tabular}
\end{footnotesize}
\caption{Relative statistical and systematic uncertainties (in \%) in the measured cross sections of $Z+\text{jets}$ production for successive inclusive jet multiplicities in the electron (top) and muon (bottom) channels.} \label{tab:systot_ell}
\end{table}

ZplusJetsPaper_merged.tex
%-------------------------------------------------------------------------------
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\documentclass[cernpreprint,UKenglish,texlive=2016,txfonts]{\ATLASLATEXPATH atlasdoc}
%\documentclass[UKenglish,texlive=2013,Paper,coverpage]{\ATLASLATEXPATH atlasdoc}

% The following command is needed by arXiv to ensure use of pdflatex.
% It should be included in the first 5 lines of the preamble.
\pdfoutput=1
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% british and american also work!
% Commonly used options:
%  texlive=YYYY          Specify TeX Live version (2013 is default).
%  atlasstyle=true|false Use ATLAS style for document (default).
%  coverpage             Create ATLAS draft cover page for collaboration circulation.
%                        See atlas-draft-cover.tex for a list of variables that should be defined.
%  cernpreprint          Create front page for a CERN preprint.
%                        See atlas-preprint-cover.tex for a list of variables that should be defined.
%  PAPER                 The document is an ATLAS paper (draft).
%  CONF                  The document is a CONF note (draft).
%  PUB                   The document is a PUB note (draft).
%  txfonts=true|false    Use txfonts rather than the default newtx - needed for arXiv submission.
%  paper=a4|letter       Set paper size to A4 (default) or letter.

%-------------------------------------------------------------------------------
% Extra packages:
\usepackage{\ATLASLATEXPATH atlaspackage}
% Commonly used options:
%  biblatex=true|false   Use biblatex (default) or bibtex for the bibliography.
%  backend=biber         Use the biber backend rather than bibtex.
%  subfigure|subfig|subcaption  to use one of these packages for figures in figures.
%  minimal               Minimal set of packages.
%  default               Standard set of packages.
%  full                  Full set of packages.
\usepackage{lscape}
%-------------------------------------------------------------------------------
\usepackage{verbatim}
%-------------------------------------------------------------------------------
% Style file with biblatex options for ATLAS documents.
\usepackage{\ATLASLATEXPATH atlasbiblatex}

% Package for creating list of authors and contributors to the analysis.
%\usepackage{\ATLASLATEXPATH atlascontribute}

% Useful macros
\usepackage{\ATLASLATEXPATH atlasphysics}
\usepackage{\ATLASLATEXPATH atlasprocess}
% See doc/atlas-physics.pdf for a list of the defined symbols.
% Default options are:
%   true:  journal, misc, particle, unit, xref
%   false: BSM, hion, math, process, other, texmf
% See the package for details on the options.

% Add you own definitions here (file ZplusJetsPaper-def.sty).
\usepackage{ZplusJetsPaper-def}
\usepackage{color}
\usepackage{atlas_tables-defs}
\usepackage{siunitx}
 
% Files with references for use with biblatex.
% Note that biber gives an error if it finds empty bib files.
\addbibresource{ZplusJetsPaper.bib}
\addbibresource{bibtex/bib/ATLAS.bib}
\addbibresource{bibtex/bib/ConfNotes.bib}

% Paths for figures - do not forget the / at the end of the directory name.
\graphicspath{{logos/}{figures/}}

%-------------------------------------------------------------------------------
% Generic document information
%-------------------------------------------------------------------------------

% Title, abstract and document 
%-------------------------------------------------------------------------------
% This file contains the title, author and abstract.
% It also contains all relevant document numbers used by the different cover pages.
%-------------------------------------------------------------------------------
 
% Title
\AtlasTitle{Measurements of the production cross section of a \Zboson boson in association
with jets in \textit{pp} collisions at $\sqrt{s} = 13$~TeV with the ATLAS detector}

% Author - this does not work with revtex (add it after \begin{document})
\author{The ATLAS Collaboration}

% Date: if not given, uses current date
%\date{\today}


% ATLAS reference code, to help ATLAS members to locate the paper
\AtlasRefCode{STDM-2016-01}

% CERN preprint number
\PreprintIdNumber{CERN-EP-2016-297}

\AtlasJournalRef{Eur. Phys. J. C77 (2017) 361} 
\AtlasDOI{10.1140/epjc/s10052-017-4900-z}

% ATLAS date - arXiv submission; to be filled in by the Physics Office
% \AtlasDate{\today}

% HepData record
% \HepDataRecord{ZZZZZZZZ}

% Abstract - % directly after { is important for correct indentation
\AtlasAbstract{
Measurements of the production cross section of a \Zboson boson in association with jets in proton--proton collisions at $\sqrt{s} = 13$~TeV are presented, using data corresponding to an integrated luminosity of $ 3.16$~fb$^{-1}$ collected by the ATLAS experiment at the CERN Large Hadron Collider in 2015. Inclusive and differential cross sections are measured for events containing a \Zboson boson decaying to electrons or muons and produced in association with up to seven jets with $\pT > 30$~GeV and $|y| <2.5$. Predictions from different Monte Carlo generators based on leading-order and next-to-leading-order matrix elements for up to two additional partons interfaced with parton shower and fixed-order predictions at next-to-leading order and next-to-next-to-leading order are compared with the measured cross sections. Good agreement within the uncertainties is observed for most of the modelled quantities, in particular with the generators which use next-to-leading-order matrix elements and the more recent next-to-next-to-leading-order fixed-order predictions.\\

 
}



% Author and title for the PDF file
\hypersetup{pdftitle={ATLAS draft},pdfauthor={The ATLAS Collaboration}}


 
%
\newcommand{\stotWp}{\mbox{$\sigma_{W^+}^{\textrm{tot}}$}}
\newcommand{\stotWm}{\mbox{$\sigma_{W^-}^{\textrm{tot}}$}}
\newcommand{\stotW}{\mbox{$\sigma_{W}^{\textrm{tot}}$}}
\newcommand{\stotWpm}{\mbox{$\sigma_{W^{\pm}}^{\textrm{tot}}$}}
\newcommand{\stotZ}{\mbox{$\sigma_{Z}^{\textrm{tot}}$}}
\newcommand{\stotZg}{\mbox{$\sigma_{Z/\gamma^*}^{\textrm{tot}}$}}
\newcommand{\stotWZ}{\mbox{$\sigma_{W(Z)}^{\textrm{tot}}$}}
\newcommand{\stot}{\mbox{$\sigma^{\textrm{tot}}$}}
\newcommand{\sigW}{\mbox{$\sigma_W$}}
\newcommand{\sigZ}{\mbox{$\sigma_Z$}}
%
\newcommand{\ZNj}{\mbox{$Z (\rightarrow \ell^{+}\ell^{-})+\ge N_{\mathrm{{jets}}}$}}
\newcommand{\sfidWp}{\mbox{$\sigma_{W^+}^{\mathrm{fid}}$}}
\newcommand{\sfidWm}{\mbox{$\sigma_{W^-}^{\mathrm{fid}}$}}
\newcommand{\sfidW}{\mbox{$\sigma_{W}^{\mathrm{fid}}$}}
\newcommand{\sfidWpm}{\mbox{$\sigma_{W^{\pm}}^{\mathrm{fid}}$}}
\newcommand{\sfidZ}{\mbox{$\sigma_{Z}^{\mathrm{fid}}$}}
\newcommand{\sfidZnj}{\mbox{$\sigma_\ZNj^{\mathrm{fid}}$}}
\newcommand{\sfidZg}{\mbox{$\sigma_{Z/\gamma^*}^{\mathrm{fid}}$}}
\newcommand{\sfidWZ}{\mbox{$\sigma_{W(Z)}^{\mathrm{fid}}$}}
\newcommand{\sfid}{\mbox{$\sigma^{\mathrm{fid}}$}}
\newcommand{\cw}{\mbox{$C_W$}}
\newcommand{\cz}{\mbox{$C_Z$}}
\newcommand{\czj}{\mbox{$C_{\scalebox{0.8}{\ZNj}}$}}
%

%-------------------------------------------------------------------------------
% Content
%-------------------------------------------------------------------------------
\begin{document}

\maketitle


\tableofcontents
\clearpage



%-------------------------------------------------------------------------------
\section{Introduction}\label{sec:intro}
%-------------------------------------------------------------------------------
 
The measurement of the production of a \Zboson boson\footnote{Throughout this paper, \Zg-boson production is denoted simply by \Zboson-boson production.}  in association with jets, \Zj,  constitutes a powerful test of perturbative quantum chromodynamics (QCD)~\cite{QCD1,QCD2}. The large production cross section and easily identifiable decays of the \Zboson boson to charged leptonic final states offer clean experimental signatures which can be precisely measured.  Such processes also constitute a non-negligible  background for studies of the Higgs boson and in searches for new phenomena; typically in these studies,  the multiplicity and kinematics of the jets are exploited  to achieve a separation of the signal of interest from the Standard Model (SM)  \Zj process. These quantities are often measured in control regions and subsequently extrapolated to the signal region with the use of Monte Carlo  (MC) generators, which are themselves subject to systematic uncertainty and must be tuned and validated using data. Predictions from the most recent generators combine next-to-leading-order (NLO) multi-leg matrix elements with a parton shower (PS) and a hadronisation model. Fixed-order parton-level predictions for \Zj production at next-to-next-to-leading order (NNLO) are also available~\cite{Boughezal:2015ded,Boughezal:2016isb,Ridder:2015dxa,Ridder:2016nkl}.

The \Zj production differential cross section was previously measured by the ATLAS~\cite{PERF-2007-01}, CMS~\cite{Chatrchyan:2008aa}, and LHCb~\cite{Alves:2008zz} collaborations at the CERN Large Hadron Collider (LHC)~\cite{1748-0221-3-08-S08001} at centre-of-mass energies of $\sqrt{s}=7$~TeV~\cite{Zjets2013,VjetsCms1,VjetsCms2,VjetsCms3,Aaij:2013nxa} and $8$~TeV~\cite{Khachatryan:2015ira,Khachatryan:2016crw,AbellanBeteta:2016ugk}, and by the CDF and D0 collaborations at the Tevatron collider at $\sqrt s = 1.96$~TeV~\cite{Aaltonen:2014vma,Abazov:2009pp}. In this paper, proton--proton ($pp$) collision data corresponding to an integrated luminosity of 3.16~fb$^{-1}$, collected at $\sqrt{s} = 13$~TeV with the ATLAS detector during 2015, are used for measurements of the \Zboson-boson production cross section in association with up to seven jets within a fiducial region defined by the detector acceptance. The \Zboson boson is identified using its decays to electron or muon pairs  (\Ztoee, \Ztomm). Cross sections are measured separately for these two channels, and for their combination, as a function of the inclusive and exclusive jet multiplicity $N_\mathrm{jets}$ and the ratio of successive inclusive jet multiplicities $(N_\mathrm{jets}+1)/N_\mathrm{jets}$, the transverse momentum  of the leading jet \pTj for several jet multiplicities, the jet rapidity \yj, the azimuthal separation between the two leading jets \Dphijj, the two leading jet invariant mass \mjj, and the scalar sum \HT of the transverse momenta of all selected leptons and jets. 

The paper is organised as follows. Section~\ref{sec:detector} contains a brief description of the ATLAS detector. The data and simulated samples as well as the \Zj predictions used in the analysis are described in Section~\ref{sec:dataMC}. The event selection and its associated uncertainties are presented in Section~\ref{sec:selection}, while the methods employed to estimate the backgrounds are shown in Section~\ref{sec:backgrounds}. Comparisons between data and Monte Carlo predictions for reconstructed distributions are found in Section~\ref{sec:kinematics}, while the unfolding procedure is described in Section~\ref{sec:unfolding}. Section~\ref{sec:results} presents the analysis results, the comparisons to predictions, and a discussion of their interpretation. Conclusions are provided in Section~\ref{sec:conclusion}.

%-------------------------------------------------------------------------------
\section{The ATLAS detector}
\label{sec:detector}
%-------------------------------------------------------------------------------


\newcommand{\AtlasCoordFootnote}{%
ATLAS uses a right-handed coordinate system with its origin at the nominal interaction point (IP)
in the centre of the detector and the $z$-axis along the beam pipe.
The $x$-axis points from the IP to the centre of the LHC ring,
and the $y$-axis points upwards.
Cylindrical coordinates $(r,\phi)$ are used in the transverse plane, 
$\phi$ being the azimuthal angle around the $z$-axis.
The pseudorapidity is defined in terms of the polar angle $\theta$ as $\eta = -\ln \tan(\theta/2)$.
Angular distance is measured in units of $\Delta R \equiv \sqrt{(\Delta\eta)^{2} + (\Delta\phi)^{2}}$.
When dealing with massive jets and particles, the rapidity $y = \frac{1}{2} \ln \left( \frac{E+p_z}{E-p_z} \right)$
is used, where $E$ is the jet/particle energy and $p_z$ is the $z$-component of
the jet/particle momentum. }


The ATLAS experiment at the LHC is a multi-purpose particle detector with a forward-backward symmetric cylindrical geometry and nearly $4\pi$ coverage in  solid angle.\footnote{\AtlasCoordFootnote} It consists of an inner tracking detector, electromagnetic and hadronic calorimeters, and a muon spectrometer. 
%
The inner tracker is surrounded by a thin superconducting solenoid magnet and provides precision tracking of charged particles and momentum measurements in the pseudorapidity range $|\eta| < 2.5$.  
%
This region is matched to a high-granularity 
electromagnetic (EM) sampling calorimeter covering the pseudorapidity range $|\eta| < 3.2$, and a coarser granularity calorimeter up to $|\eta| = 4.9$. 
The hadronic calorimeter system covers the entire pseudorapidity range up to  $|\eta| = 4.9$.
The muon spectrometer consists of three large superconducting toroids each containing eight coils, a system of trigger chambers, and precision tracking
chambers, which provide trigger and tracking capabilities in the range $|\eta| < 2.4$ and $|\eta| < 2.7$, respectively.
%
A two-level trigger system~\cite{Aaboud:2016leb} is used to select events. The first-level
trigger is implemented in hardware and uses a subset of the detector
information. This is followed by the software-based high-level trigger system,
which runs offline reconstruction, reducing the event rate to approximately \SI{1}{kHz}.


%-------------------------------------------------------------------------------
\section{Data set, simulated event samples, and predictions}
\label{sec:dataMC}
%-------------------------------------------------------------------------------

\subsection{Data set}

The data used in this analysis were collected by the ATLAS detector during August  to November 2015. During this period, the LHC circulated \SI{6.5}{\TeV} proton beams with a \SI{25}{ns} bunch spacing.  The peak delivered instantaneous luminosity was $L=\SI{5e33}{\per \cm \squared \per \s}$ and the mean number of $pp$ interactions per bunch crossing (hard scattering and pile-up events) was $\langle \mu \rangle = 13$.  The data set used in this measurement corresponds to a total integrated luminosity of 3.16~fb$^{-1}$.

\subsection{Simulated event samples}

Monte Carlo simulations, normalised to higher-order calculations,  are used to estimate most of the contributions from background events, to unfold the data to the particle level, and to compare with the unfolded data distributions. All  samples are processed with a {\textsc{Geant}4}-based simulation~\cite{Agostinelli:2002hh} of the ATLAS detector~\cite{SOFT-2010-01}. An overview of all signal and background processes considered and of the generators used for the simulation is given in Table~\ref{tab:MC}.  Total production cross sections for the samples, their respective uncertainties (mainly coming from parton distribution function (PDF) and factorisation and renormalisation scale variations), and references to higher-order QCD corrections, where available, are also listed in Table~\ref{tab:MC}. 


\begin{table}[t]
\begin{scriptsize}
\begin{center} 
\begin{tabular}{ |l|l|rl c|r|}
\hline
\hline
Process & Generator& $(\sigma \cdot \mathrm{BR})$ & Normalisation & Reference & Theory\\ 
        &          & [pb]                    & order &                   & uncert.\\
\hline
\hline
 \Ztollj ($\ell = e,\mu; m_{\ell\ell}>40$~GeV) &     \SHERPAtwotwo & $2106$  &NNLO &\cite{Anastasiou:2003ds,FEWZ2,FEWZ3,FEWZ4} & 5\% \\
 \Ztollj ($\ell = e,\mu,\tau; m_{\ell\ell}>40$~GeV) &     \MGaMCPyeight          & $2103$  &NNLO & \cite{Anastasiou:2003ds,FEWZ2,FEWZ3,FEWZ4} & 5\%  \\
 \Wln\ \;\;($\ell = e,\mu$)   	            &   \MGaMCPyeight    & $20080$  &NNLO &  \cite{Anastasiou:2003ds,FEWZ2,FEWZ3,FEWZ4} & 5\%   \\
$t\overline{t}$ \;\; ($m_{t}=172.5$~GeV) & & & & & \\           		
\;\;  \textsc{Perugia2012(radHi/radLo)}  &\POWHEGPysix   & $831$ &NNLO+NNLL &\cite{Czakon:2011xx} & 6\%\\
\;\; \textsc{UE-EE-5}                                        &\MGaMCHpp  & $831$ & NNLO+NNLL & \cite{Czakon:2011xx} & 6\%\\
Single top quark ($Wt$)                                   &\POWHEGPysix   & $72$         & NLO+NNLL &\cite{Kidonakis2010u} & 6\% \\
Single top quark ($t$-channel)                             &\POWHEGPysix   & $136$   & NLO+NNLL &\cite{Kidonakis2011} & 6\%\\
Single top anti-quark ($t$-channel)                             &\POWHEGPysix   & $81$   & NLO+NNLL &\cite{Kidonakis2011} & 6\%\\
Dibosons                                                      & \SHERPAtwoone& $97$ & NLO & \cite{Gleisberg:2008ta} & 6\% \\
\hline
\hline
\end{tabular}
\caption{Signal and background Monte Carlo samples and the generators used in the simulation. 
Each sample is normalised to the appropriate production cross section $\sigma$ and  multiplied by the relevant branching ratios (${\mathrm{BR}}$) per lepton flavour for this sample, as shown in the third column.  
For \Wboson-boson and top-quark production, contributions from higher-order QCD corrections were calculated  following the references given in the fifth column for the stated order. Similarly, for \Zboson-boson production, higher-order QCD corrections were evaluated in the dilepton invariant mass range $66<m_{\ell\ell}<116$~GeV following the references given in the fifth column for the stated order, and extrapolation scaling factors were applied to match mass ranges used by each simulation as given in the first column.  The theory uncertainties as given in the final column correspond to PDF and scale variations. The diboson samples include on-shell and off-shell $WW$, $WZ$ and $ZZ$ production. Recently, NNLO QCD predictions have been made available for the diboson processes~\cite{wznnlo,ggwwnnlo}. However, these higher-order corrections have a negligible impact on this analysis. }
\label{tab:MC}
\end{center}
\end{scriptsize}
\end{table}


Signal events (i.e. containing a \Zboson boson with associated jets) are simulated using the \SHERPA~v2.2.1~\cite{Gleisberg:2008ta} generator, denoted by \SHERPAtwotwo. Matrix elements (ME) are calculated for up to two additional partons at NLO and up to four partons at leading order (LO) using the  Comix~\cite{Gleisberg:2008fv} and OpenLoops~\cite{Cascioli:2011va} matrix element generators. They are merged with the \SHERPA parton shower~\cite{Schumann:2007mg} (with a matching scale of 20~GeV) using the \textsc{ME+PS@NLO} prescription~\cite{Hoeche:2012yf}. A five-flavour scheme is used for these predictions. The \NNPDFthree PDF set~\cite{Ball:2014uwa} is used in conjunction with a dedicated set of parton-shower-generator parameters (tune) developed by the \SHERPA authors.
This sample is used for the nominal unfolding of the data distributions, to compare to the cross-section measurements, and to estimate the systematic uncertainties.

A simulated sample of \Zj production is also produced with the \MADGRAPHaMC (denoted by \MGaMC)~v2.2.2 generator~\cite{Alwall:2014hca}, using matrix elements including up to four partons at leading order and employing the \NNPDFthree PDF set,  interfaced to \PYTHIA~v8.186~\cite{Sjostrand:2007gs} to model the parton shower, using the CKKWL merging scheme~\cite{Lonnblad:2001iq} (with a matching scale of 30~GeV).  A five-flavour scheme is used. The \textsc{A14}~\cite{ATL-PHYS-PUB-2014-021} parton-shower tune is used together with the \NNPDFtwothree PDF set~\cite{Ball:2012cx}. The sample is denoted by \MGaMCPyCKKWL and is used to provide cross-checks of the systematic uncertainty in the unfolding and to model the small $\Zboson \to \tau \tau$ background. In addition, a \MGaMC sample with matrix elements for up to two jets and with parton showers beyond this, employing the \NNPDFthree PDF set and interfaced to \PYTHIA~v8.186 to model the parton shower, is generated using the FxFx merging scheme~\cite{VjetFxFx}  (with a matching scale of 25~GeV~\cite{VjetFxFxold}) and is denoted by \MGaMCPyFxFx. This sample also uses a five-flavour scheme and the \textsc{A14} parton-shower tune  with the \NNPDFtwothree PDF set. Both \MGaMC samples are used for comparison with  the unfolded cross-section measurements.

The measured cross sections are also compared to predictions from the leading-order matrix element generator \ALPGEN~v2.14~\cite{Mangano:2002ea} interfaced to 
\PYTHIA~v6.426~\cite{Sjostrand:2006za} to model the parton shower, denoted by \ALPGENPysix, using the \textsc{Perugia2011C}~\cite{Skands:2010ak} parton-shower tune and 
the  \textsc{CTEQ6L1} PDF set~\cite{Pumplin:2002vw}. A four-flavour scheme is used. Up to five additional partons are modelled by the matrix elements merged with the MLM 
prescription~\cite{Mangano:2002ea} (with a matching scale of 20~GeV).  The matrix elements for the production of $Z+b\bar{b}$ and $Z+c\bar{c}$ events are
 explicitly included and a heavy-flavour  overlap procedure is used to remove the double counting of heavy quarks from gluon splitting in the parton shower. 


The \Zboson-boson samples are normalised to the NNLO prediction calculated with the {\textsc Fewz}~3.1 program~\cite{Anastasiou:2003ds,FEWZ2,FEWZ3,FEWZ4} with \textsc{CT10nnlo} PDFs~\cite{Lai:2010vv}. 
%

Contributions from the top-quark, single-boson, and diboson components of the background (described in Section~\ref{sec:backgrounds}) are estimated from the following Monte Carlo samples.
Samples of top-quark  pair and single top-quark production are generated at NLO with the \POWHEG-Box generator~\cite{Nason:2004rx,Frixione:2007vw,Alioli:2010xd} (versions~v2 (r3026) for top-quark pairs and~v1 for single top quarks (r2556 and r2819 for $t$-and $Wt$-channels, respectively)) and \PYTHIA~v6.428 (\textsc{Perugia2012} tune~\cite{Skands:2010ak}). Samples with enhanced or suppressed additional radiation are generated with the \textsc{Perugia2012radHi}/\textsc{Lo} tunes~\cite{Skands:2010ak}. An alternative top-quark pair sample is produced using the \MGaMC generator interfaced with \HERWIGpp~v2.7.1~\cite{Alwall:2014hca,herwigpp}, using the \textsc{UE-EE-5} tune~\cite{Gieseke:2012ft}. The samples are normalised to the cross section calculated at NNLO+NNLL (next-to-next-to-leading log) with the Top++2.0 program~\cite{Czakon:2011xx}.

The \Wboson-boson backgrounds are modelled using the \MGaMCPyCKKWL~v2.2.2 generator, interfaced to \PYTHIA~v8.186 and are normalised to the NNLO values given in Table~\ref{tab:MC}.
Diboson processes with fully leptonic and semileptonic decays are simulated~\cite{MultiBosonPub} using the \SHERPA~v2.1.1 generator with the \textsc{CT10nlo} PDF set. The matrix elements contain the doubly resonant $WW$, $WZ$ and $ZZ$ processes, and all other diagrams with four electroweak vertices. They are calculated for one or zero additional partons at NLO and up to three additional partons at LO and merged with the \SHERPA parton shower using the \textsc{ME+PS@NLO} prescription. 

Events involving semileptonic decays of heavy quarks, hadrons misidentified as leptons, and, in the case of the electron channel, electrons from photon conversions are referred to collectively as ``multijet events''.  The multijet background was estimated using data-driven techniques, as described in Section~\ref{sec:backgrounds}.

Multiple overlaid $pp$ collisions are simulated with the soft QCD processes of \PYTHIA~v.8.186 using the \textsc{A2} tune~\cite{ATLAS-PHYS-PUB-2012-003} and the \textsc{MSTW2008LO} PDF set~\cite{Martin:2009iq}. All Monte Carlo samples are reweighted so that the pile-up distribution matches that observed in the data.  

\subsection{Fixed-order predictions}
\label{sec:dataMCFO}
    
In addition to these Monte Carlo samples, parton-level fixed-order predictions at NLO are calculated by the \BLACKHATSHERPA collaboration for the production of \Zboson bosons with  up to  four partons~\cite{bhz3jets,bhz4jets}. 
%
The \BLACKHATSHERPA predictions use the \textsc{CT14} PDF set~\cite{Dulat:2015mca} including variations of its eigenvectors at the 68\% confidence level, rescaled from 90\% confidence level using a factor of $1/1.645$. 
%
The nominal predictions use a factorisation and renormalisation scale of $\HT/2$ with uncertainties derived from the envelope of a common variation of the scales by factors of $0.5, 1/\sqrt{2}, \sqrt{2},$ and 2.
%
The effects of PDF and scale uncertainties range from 1\% to 4\% and from 0.1\% to 10\%, respectively, for the cross sections of \Zboson-boson production in association with at least one to four partons, and are included in the predictions which are provided by the  \BLACKHATSHERPA authors for the fiducial phase space of this analysis. 
%
Since these predictions are defined before the decay leptons emit photons via final-state radiation (Born-level FSR), corrections to the dressed level (where all photons found within a cone of size $\Delta R = 0.1$ of the lepton from the decay of the \Zboson boson are included) are derived from \MGaMCPyCKKWL, separately for each kinematic observable used to measure cross sections,  with associated systematic uncertainties obtained by comparing to the \ALPGENPysix generator.
This correction is needed in order to match the prediction to the lepton definition used in the measurements. The average size of these corrections is approximately $-2$\%. 
%
To bring the prediction from parton to particle level, corrections for the non-perturbative effects of hadronisation and the underlying event are also calculated separately for each observable  using the \SHERPA~v2.2 generator by turning on and off in the simulation both the fragmentation and the interactions between the proton remnants. The net size of the corrections is up to approximately 10\% at small values of \pTj and vanishes for large values of \pTj. An uncertainty of approximately 2\% for this correction is included in  the total systematic uncertainty of the prediction. 
%


Calculations of cross sections at NNLO QCD have recently become available~\cite{Boughezal:2015ded,Boughezal:2016isb,Ridder:2015dxa,Ridder:2016nkl}. In this paper, the results are compared to the calculation, denoted by \Njetti\cite{Boughezal:2015ded,Boughezal:2016isb}, which uses a new subtraction technique based on $N$-{\em jettiness}~\cite{Boughezal:2015dva} 
 and relies on the theoretical formalism provided in soft-collinear effective theory. The predictions, which are provided by the authors of this calculation for the fiducial phase space of this analysis, use a factorisation and renormalisation scale of $\sqrt{m_{\ell\ell}^2 + \sum \left(p_{\text{T}}^{\text{jet}}\right)^2}$ (where $m_{\ell\ell}$ is the invariant mass of the dilepton system) and the \textsc{CT14} PDF set.  The QCD renormalisation and factorisation scales were jointly varied by a common factor of two, and are included in the uncertainties. Non-perturbative and FSR corrections and their associated uncertainties as discussed above are also included in the predictions. 


%-------------------------------------------------------------------------------
\section{Event selection}
\label{sec:selection}
%-------------------------------------------------------------------------------

Electron- and muon-candidate events are selected using triggers which require at least one electron or muon with transverse momentum thresholds of $\pT=\SI{24}{\GeV}$ or \SI{20}{\GeV}, respectively, with some isolation requirements for the muon trigger. To recover possible efficiency losses at high momenta, additional electron and muon triggers which do not make any isolation requirements are included with thresholds of $\pT \ge \SI{60}{\GeV}$ and $\pT = \SI{50}{\GeV}$, respectively.  Candidate events are required to have a primary vertex, defined as the vertex with the highest sum of track $\pT^2$, with at least two associated tracks with $\pT > \SI{400}{\MeV}$.

Electron candidates are required to have $\pT>\SI{25}{\GeV}$ and to pass ``medium'' likelihood-based identification requirements~\cite{elecperf,ATL-PHYS-PUB-2015-041} optimised for the 2015 operating conditions, within the fiducial region of $|\eta|<2.47$, excluding candidates in the transition region between the barrel and endcap electromagnetic calorimeters, $1.37<|\eta|<1.52$. Muons are reconstructed for $|\eta|<2.4$ with $\pT>\SI{25}{\GeV}$ and must pass ``medium'' identification requirements~\cite{Aad:2016jkr} also optimised for the 2015 operating conditions. At least one of the lepton candidates is required to match the lepton that triggered the event. The electrons and muons must also satisfy \pT-dependent cone-based isolation requirements, using both tracking detector and calorimeter information (described in Refs.~\cite{Aad:2015yja} and ~\cite{Aad:2014lwa}, respectively). The isolation requirements are tuned so that the lepton isolation efficiency is at least 90\% for $\pT>\SI{25}{\GeV}$, increasing to 99\% at 60~GeV.
Both the electron and muon tracks are required to be associated with the primary vertex, using constraints on the transverse impact parameter significance $|d_0|/\Delta d_0$, where $d_0$ is the transverse impact parameter and $\Delta d_0$ is its uncertainty, and on the longitudinal impact parameter $z_0$ corrected for the reconstructed position of the primary vertex. The transverse impact parameter significance is required to be less than five for electrons and three for muons, while the absolute value of the corrected $z_0$ multiplied by the sine of the track polar angle is required to be less than 0.5~mm.


Jets of hadrons are reconstructed with the anti-$k_t$ algorithm~\cite{Cacciari:2008} with radius parameter $R=0.4$ using  topological clusters of energy deposited in the calorimeters~\cite{Aad:2016upy}. Jets are calibrated using a simulation-based calibration scheme, followed by in situ corrections to account for differences between simulation and data~\cite{ATLAS-PHYS-PUB-2015-015}. In order to reduce the effects of pile-up contributions, jets with pseudorapidity  $|\eta|<2.4$ and  $\pT<\SI{60}{\GeV}$ are required to have a significant fraction of their tracks with an origin compatible with the primary vertex, as defined by the jet vertex tagger algorithm~\cite{ATLAS-CONF-2014-018}. In addition, the expected average energy contribution from pile-up clusters is subtracted according to the $\eta$--$\phi$ catchment area of the jet~\cite{Aad:2015ina}. Jets used in the analysis are required to have  \pT greater than $30$~GeV and  rapidity $|y|<2.5$. 

The overlap between leptons and jets is removed in a two-step process. The first step removes jets closer than $\Delta R  = 0.2$ to a selected electron, and jets closer than $\Delta R  = 0.2$ to a selected muon, if they are likely to be reconstructed from  photons radiated by the muon. 
In a second step,  electrons and muons are discarded if they are located closer than $\Delta R = 0.4$ to a remaining selected jet.
This requirement effectively removes events with leptons and jets which are not reliably simulated in the Monte Carlo simulation.

Events containing a \Zboson-boson candidate are selected by requiring exactly two leptons of the same flavour but of opposite charge with dilepton invariant mass in the range  $71 < m_{\ell\ell} < \SI{111}{GeV}$. The expected and observed numbers  of \Zboson-boson candidates selected for each inclusive jet multiplicity, for $N_{\mathrm{jets}} \ge 0-7$, are summarised in Table~\ref{tab:zjets_sigbak}, separately for the \Ztoee and the \Ztomm channels. The background evaluation that appears in this table is discussed in Section~\ref{sec:backgrounds}. After all requirements,  248,816   and  311,183  \Zonej events are selected in the electron and muon channels, respectively.



\begin{table}[t]
\centering
\begin{footnotesize}
\begin{tabular}{|l|r|r|r|r|r|r|r|r|}
\hline \hline
& \multicolumn{8}{c|}{Electron channel} \\ \hline
& $\texttt{+}\geq\mathrm{0~jets} $ & $\texttt{+}\geq\mathrm{1~jets}$ & $\texttt{+}\geq\mathrm{2~jets}$ & $\texttt{+}\geq\mathrm{3~jets}$ & $\texttt{+}\geq\mathrm{4~jets}$ & $\texttt{+}\geq\mathrm{5~jets}$ & $\texttt{+}\geq\mathrm{6~jets}$ & $\texttt{+}\geq\mathrm{7~jets}$ \\
\hline
\Ztoee\ [\%]               & 99.3 & 97.6 & 93.9 & 90.3 & 87.3 & 85.2 & 83.3 & 81.2\\
Top quark   [\%]           & 0.2  & 1.2 & 3.8  & 6.5  & 8.6  & 9.7 & 10.5 & 11.6\\
Diboson   [\%]             & 0.2  & 0.8  & 1.6  & 2.4  & 3.4  & 4.4  & 5.5  & 6.6\\
$Z\to\tau^{+}\tau^{-}$ [\%] & <0.1 & <0.1 & <0.1 & <0.1 & <0.1 & <0.1 & <0.1 & <0.1\\
$W \to e\nu$  [\%]         & <0.1 & <0.1 & <0.1 & <0.1 & <0.1 & <0.1 & <0.1 & <0.1\\ 
Multijet      [\%]         & 0.2  & 0.4  & 0.6  & 0.7  & 0.7  & 0.7  & 0.7  & 0.7\\
\hline  

Expected               & 1,327,900 & 239,500 & 57,310 & 14,080 & 3637 &  978 & 252 & 63 \\
Observed               & 1,347,900 & 248,816 & 59,998 & 14,377 & 3587 &  898 & 217 & 48 \\
\hline\hline
& \multicolumn{8}{c|}{Muon channel} \\ \hline
& $\texttt{+}\geq\mathrm{0~jets} $ & $\texttt{+}\geq\mathrm{1~jets}$ & $\texttt{+}\geq\mathrm{2~jets}$ & $\texttt{+}\geq\mathrm{3~jets}$ & $\texttt{+}\geq\mathrm{4~jets}$ & $\texttt{+}\geq\mathrm{5~jets}$ & $\texttt{+}\geq\mathrm{6~jets}$  & $\texttt{+}\geq\mathrm{7~jets}$\\
\hline
\Ztomm\  [\%]              & 99.3 & 97.5 & 94.0 & 90.7 & 88.3 & 86.7 & 84.8 & 84.6\\
Top quark [\%]             & 0.2  & 1.1  & 3.6  & 6.0  & 7.7  & 8.1  & 8.7 & 7.7\\
Diboson   [\%]             & 0.2  & 0.7  & 1.6  & 2.4  & 3.4  & 4.5  & 5.9  & 7.0\\
$Z\to\tau^{+}\tau^{-}$ [\%] & <0.1 & <0.1 & <0.1 & <0.1 & <0.1 & <0.1 & <0.1 & <0.1\\
$W \to \mu\nu$   [\%]      & <0.1 & <0.1 & <0.1 & <0.1 & <0.1 & <0.1 & <0.1 & <0.1\\
Multijet         [\%]      & 0.3  & 0.6  & 0.9  & 0.9  & 0.7  & 0.7  & 0.7  & 0.7\\
\hline
Expected               & 1,693,000 & 300,600 & 71,230 & 17,740 & 4523 & 1187 &  307  & 76 \\ 
Observed               & 1,708,602 & 311,183 & 74,510 & 17,865 & 4387 & 1081 &  240  & 57\\
\hline\hline
\end{tabular}
\end{footnotesize}
\caption{Fraction of signal and background processes in \% in the final selection and expected and observed numbers of events for the various inclusive jet multiplicities considered in the electron (top) and muon (bottom) channels.}
\label{tab:zjets_sigbak}
\end{table}
  
\subsection{Correction factors and related systematic uncertainties}
\label{sec:uncertainties}
Some of the object and event selection efficiencies as well as the energy and momentum calibrations modelled by the simulation must be corrected with simulation-to-data correction factors to better match those observed in the data. These corrections and their corresponding uncertainties fall into the following two categories: dependent and not dependent on lepton flavour.

The corrections and uncertainties specific to each leptonic final state (\Ztoee and \Ztomm) are as follows:
\begin{itemize}
\item \textbf{Trigger:} The lepton trigger efficiency is estimated in simulation, with a separate data-driven analysis
performed to obtain the simulation-to-data trigger correction factors and their corresponding uncertainties~\cite{Aaboud:2016leb}.
\item \textbf{Lepton reconstruction, identification, and isolation:} The lepton selection efficiencies as determined from simulation are also corrected with simulation-to-data correction factors, with corresponding uncertainties~\cite{ATL-PHYS-PUB-2015-041,Aad:2016jkr}. 
\item \textbf{Energy, momentum scale/resolution:} Uncertainties in the lepton calibrations are estimated~\cite{Aad:2016jkr} because they can cause a change of acceptance because of migration of events across the \pT threshold and $m_{\ell\ell}$ boundaries.
\end{itemize}     

The corrections and uncertainties common to the electron and muon final states are as follows:
\begin{itemize}
\item \textbf{Jet energy scale and resolution}:
Uncertainties in the jet energy-scale calibration and resolution have a significant impact on the measurements, especially for the higher jet multiplicities.  The jet energy-scale calibration is based on 13~TeV simulation and on in situ corrections obtained from data~\cite{ATLAS-PHYS-PUB-2015-015}. The uncertainties are estimated using a decorrelation scheme, resulting in a  set of 19 independent parameters which cover all of the relevant calibration uncertainties. The jet energy scale is the dominant systematic uncertainty for all bins with at least one jet.
The jet energy-resolution uncertainty is derived by over-smearing the jet energy in the simulation and using the symmetrised variations as the uncertainty.
\item \textbf{Jet vertex tagger}: The modelling of the output variable from the jet vertex tagger is validated using data events where the \Zboson boson recoils against a jet. A percent-level correction is derived and its statistical and systematic uncertainties are used as additional uncertainties in the efficiency to select jets from the primary vertex~\cite{ATLAS-CONF-2014-018}.  
\item \textbf{Pile-up}: The imperfect modelling of the effects of pile-up leads to acceptance changes at the percent level for different jet multiplicities. To assess this uncertainty, the average number of interactions per bunch crossing $\langle \mu \rangle$ is varied in simulation so that the behaviour of variables sensitive to pile-up matches that observed in data. 
\item \textbf{Luminosity}: The cross sections have a 2.1\% uncertainty from the measurement of the integrated luminosity, which is derived, following a methodology similar to that detailed in Refs.~\cite{DAPR-2011-01,Aaboud:2016hhf}, from a calibration of the luminosity using $x$--$y$ beam-separation scans performed in August 2015. 
\end{itemize}


%-------------------------------------------------------------------------------
\section{Background estimation}
\label{sec:backgrounds}
Contributions from the electroweak (single boson and diboson) and top-quark (single top-quark and top-quark pair) components of the background are estimated using the Monte Carlo samples described in Section~\ref{sec:dataMC} with corresponding uncertainties as listed in Table~\ref{tab:MC}. Contributions from multijet events are evaluated with data-driven techniques as described below. A summary of the composition and relative importance of the backgrounds in the candidate \Zj events is given in Table~\ref{tab:zjets_sigbak}. The overall purity of the  \Zj\ selections (fraction of signal events in the final selection) ranges from 99\% in the inclusive sample to 80-85\% in the $\geq\mathrm{7~jets}$ bin.


\subsection{Top-quark and electroweak backgrounds}
\label{sec:ew_bkg}

The dominant contribution to the background at high jet multiplicities comes from $t\overline{t}$ production, with the subsequent leptonic decays of the \Wboson bosons originating from the top quarks and is evaluated from simulation.   An overall uncertainty of 6\%, corresponding to the PDF and scale variations on the theoretical predictions of the inclusive cross sections, is assigned (see Table~\ref{tab:MC}).  The $t\overline{t}$ background estimate is validated through a  cross-section measurement of $t\overline{t}$ production in the dilepton channel at  $\sqrt s = 13$~TeV~\cite{ATLAS-CONF-2015-065} as a function of the jet multiplicity, and the modelling of the additional parton radiation in $t\overline{t}$ events by \POWHEGPysix was found to be in good agreement with this measurement. In addition, a systematic uncertainty in the modelling of the shape of the distributions is derived by modifying the parton-shower intensity  in the nominal simulation sample and by comparing to the predictions from the alternative generator \MGaMCHpp (both listed in  Table~\ref{tab:MC}).
%
The small contribution from single-top-quark events is also estimated using \POWHEGPysix samples and assigned a 6\% uncertainty.

Diboson production in leptonic and semileptonic final states with at least two leptons of the same flavour constitutes a co-dominant background for high jet multiplicities (see Table~\ref{tab:zjets_sigbak}). The production of $WZ$ bosons in association with jets at $\sqrt s=13$~TeV was found to be well modelled by the \SHERPAtwoone generator~\cite{Aaboud:2016yus}. A 6\% uncertainty, again corresponding to PDF and scale variations on the predictions, is assessed.
Since in Ref.~\cite{Aaboud:2016yus} the measurement is limited by the statistical precision for dibosons $+\geq 4$~jets (resulting in $\geq 6$~hadronic jets for semileptonic diboson decays), an additional systematic uncertainty of 50\% in the normalisation of the diboson background is added for \Zsixjs.

Minor background contributions also arise from single-\Wboson-boson production decaying to leptonic final states and from single-\Zboson-boson production in the \Ztotautau process, both estimated with simulation and assigned a 5\% uncertainty (as given in Table~\ref{tab:MC}). 



\subsection{Multijet background}
\label{sec:mj_bkg}


Background-enriched data control regions are used to estimate the multijet contribution in both the electron and muon channels. They are constructed by loosening the lepton identification and isolation requirements. Templates are built from the dilepton invariant mass distribution, a variable that shows discrimination between multijet background and other processes in regions of its kinematic range, but is largely uncorrelated with the variables used to build the multijet control regions. The templates are  subsequently normalised to events passing the \Zboson-boson signal selection. 

In the electron channel, the multijet templates are built for each jet multiplicity from  events with two same-charge leptons with no isolation requirement, whose identification criteria are looser than those of the signal selection, which the leptons must not satisfy. In the muon channel, the control region is similarly built from events with two leptons which are selected with looser identification requirements than the signal selection and also fail the nominal isolation requirement. In both cases, dedicated triggers better suited to this purpose are used to populate the templates. The small electroweak and top-quark contamination is  subtracted using simulated events. 

The normalisation of the multijet template is estimated with a log-likelihood fit to the measured dilepton invariant mass distribution for  the inclusive \Zboson selection, using  templates for  \Ztoll and for the electroweak and top-quark background derived from simulation. 
The fit is performed in the invariant mass windows of $52 < m_{ee} < 148$~GeV and $40 < m_{\mu\mu} < 80$~GeV for the electron and muon channels, respectively, in order to benefit from the larger multijet contribution in the mass sidebands. The normalisation of the multijet template is allowed to float freely while the remaining non-multijet templates are constrained to be within 6\% of the predicted cross sections for these processes as given in Table~\ref{tab:MC}. The multijet fractions are evaluated separately for each jet multiplicity, except for very high jet multiplicities where the templates are statistically limited, and so these fractions are taken from the estimates of the  $\geq\mathrm{5~jets}$ and $\geq\mathrm{4~jets}$ bins in the electron and muon channels, respectively.

The systematic uncertainties on the  multijet background are derived by varying the mass range and bin width of the nominal fit, using the lepton transverse impact parameter $d_{0}$ as the fitting variable instead of the invariant mass, using alternative simulation samples for the templates, allowing the normalisations of the non-multijet components to vary independently or within a wider range, and varying the lepton resolution and energy/momentum scales. In addition, given the multiple sources of multijet background in the electron channel, an alternative template is constructed by requiring that the electrons fail to meet an isolation criterion instead of failing to meet the nominal signal selection electron identification criterion. 

The resulting estimated multijet fractions in each jet multiplicity bin are given in Table~\ref{tab:zjets_sigbak}. Their corresponding total uncertainties are dominated by their systematic components. These systematic components are approximately 70\%  of the multijet fraction as estimated in the electron and muon channels. 


%\clearpage
%------------------------------------------------------------------------------- 
\section{Kinematic distributions}
\label{sec:kinematics}
The level of agreement between data and predictions is evaluated from the comparison of kinematic distributions.
Figure~\ref{fig:ZJetMass123j}, which presents the dilepton mass for the \Zonej topology and the inclusive jet multiplicity, shows how well the  
\SHERPAtwotwo and \MGaMCPyCKKWL predictions agree with data. 
The uncertainty bands shown in these distributions include the statistical uncertainties due to the simulation sample sizes, the event-selection uncertainties described in Section~\ref{sec:uncertainties} (omitting the common 2.1\% luminosity uncertainty), and the  background normalisation uncertainties described in Section~\ref{sec:backgrounds}.


\begin{figure}[p]
\centering
\includegraphics[width=0.49\textwidth]{./figures/Zee_zmass1j_log_3209pb}
\includegraphics[width=0.49\textwidth]{./figures/Zmm_zmass1j_log_3209pb}
\includegraphics[width=0.49\textwidth]{./figures/Zee_jetn_log_3209pb}
\includegraphics[width=0.49\textwidth]{./figures/Zmm_jetn_log_3209pb}
\caption{Dilepton invariant mass for \Zonej (top) and inclusive jet multiplicity (bottom) in the \Ztoeej (left) and the \Ztommj (right) channels.  All backgrounds and the signal samples are stacked to produce the figures.
Systematic uncertainties for the signal and background distributions are combined in the hatched band, and the statistical uncertainty is shown on the data points. The uncertainty in the luminosity and the theory uncertainty in the signal prediction are not included in the uncertainty band.}
\label{fig:ZJetMass123j}
\end{figure}

%-------------------------------------------------------------------------------
\section{Unfolding of detector effects}
\label{sec:unfolding}
The cross-section measurements presented in this paper are performed within the fiducial acceptance region defined by the following requirements:
\begin{itemize}
\item $\pT^{\ell}>25$~GeV, $|\eta^{\ell}|<2.5$
\item $\pTj > 30$~GeV, $|\yj|<2.5$  
\item $\Delta R(\ell,\text{jet}) > 0.4$
\item $71<m_{\ell\ell}<111$~GeV.
\end{itemize}
The  cross sections are defined at particle (``truth'') level, corresponding to dressed electrons and muons from the \Zboson bosons. The particle level also includes jets clustered  using the anti-$k_t$ algorithm~\cite{Cacciari:2008} with radius parameter $R=0.4$ for final-state particles with decay length $c\tau>10$~mm, excluding the dressed \Zboson-boson decay products. 


The fiducial cross sections are estimated from the reconstructed kinematic observables: jet multiplicity, \pTj for different jet multiplicities, \yj, \Dphijj,  \mjj, and \HT, for events that pass the selection described in Section~\ref{sec:selection}. The expected background components as described in Section~\ref{sec:backgrounds} are subtracted from the distributions in data.  A variable-width binning of these observables is used, such that the purity is at least 50\% in each bin and the size of the statistical uncertainty in most of the bins remains below 10\%. 

\begin{figure}[t]
\begin{center}
\vspace{10mm}
\includegraphics[width=0.49\textwidth]{./figures/sh_norm_el_h2JetNex0.pdf}
\includegraphics[width=0.49\textwidth]{./figures/sh_norm_mu_h2HT1j0.pdf}\\
\caption{Response matrices corresponding to the exclusive jet multiplicity for \Zj events in the electron channel (left)  and to the \HT for \Zonej events in the  muon channel (right). The sum of the entries in each row is normalised to unity. Both matrices are obtained from \SHERPAtwotwo.}
\label{fig:matrix_sh_1}
\end{center}
\end{figure}


An iterative Bayesian unfolding technique~\cite{D'Agostini:1994zf}, as implemented in the RooUnfold package~\cite{RooUnfold}, is used to unfold the measurements to the particle level, thereby accounting for detector effects related to inefficiencies, resolution, and systematic biases in the central values of the kinematic variables describing both the leptons and the jets. The iterative unfolding technique updates the initial estimators for the generated (``truth'') distribution in consecutive steps, using Bayes' theorem in each iteration to derive an unfolding matrix from the initial response matrix (which relates truth and reconstructed distributions of given observables) and the current truth estimator.

The response  matrices are constructed using the \SHERPAtwotwo \Ztollj samples. \SHERPAtwotwo is also used to derive the initial truth estimator. In order to enter the response matrix, events must pass the \Zboson-boson selection at generator level and at detector level and contain the  number of jets required by the preselection for a given observable at both generator and detector level. Reconstructed jets are required to match the corresponding generator-level jets within a cone of size $\Delta R=0.4$ for all distributions except global quantities such as the jet multiplicity and \HT. A given bin $(i,j)$ in the response matrix therefore corresponds to the probability that a true jet object in bin $j$ is reconstructed in bin $i$ of the distribution. 
Figure~\ref{fig:matrix_sh_1} illustrates two examples of response matrices.
The resulting ratios of detector-level  to truth-level event yields are typically 0.65 and 0.8 for the electron and muon channels, respectively.

The background-subtracted data are corrected for the expected fraction of events with reconstructed objects unmatched to any generator object before entering the iterative unfolding.
The number of iterations used for the iterative unfolding of each distribution (two) is chosen by unfolding the \SHERPAtwotwo samples reweighted to data and comparing to the generated reweighted distribution.
The unfolded event yields are divided by the integrated luminosity of the data sample and the bin width of the distribution in question to provide the final fiducial cross sections. The final result is given by

\begin{equation}
\sigma_i  = \frac{1}{\epsilon_i  L} \sum_j U_{ij} N_j^{\text{data}} \left(1-f_j^{\text{unmatched}}\right),
\end{equation}

where $L$ is the integrated luminosity, $\epsilon_i$ is the reconstruction efficiency for truth bin $i$, $N_j^{\text{data}}$ corresponds to the number of events observed in data in reconstructed bin $j$ and $f_j^{\text{unmatched}}$ is its fraction of unmatched events calculated from simulation, and $U_{ij}$ is the unfolding matrix calculated after two iterations, using the updated prior from the first iteration and the response matrix.

\subsection{Systematic uncertainties associated with the unfolding procedure}

The limited size of a simulation sample can create biases in the distributions. Systematic uncertainties  account for possible residual biases in the unfolding procedure due to, e.g. modelling of the hadronisation in the simulation, migrations into other kinematic distributions not explicitly part of the unfolding, or the finite bin width used in each distribution.  The following uncertainties arise from the unfolding procedure.

\begin{itemize}

\item The statistical uncertainties of the response matrices derived from \SHERPAtwotwo are propagated to the unfolded cross sections with a toy simulation method. A total of 5000 ensembles (pseudo-experiments) of unfolded samples are generated. For each sample, the number of reconstructed events in each bin is generated randomly according to a Gaussian distribution, where the mean is the nominal number of events before unfolding and the width is its corresponding statistical uncertainty. 
Unfolding is performed for each ensemble. The widths of resulting distributions are taken as a systematic uncertainty of the unfolding.

\item  The \SHERPAtwotwo samples are reweighted at  generator level, such that the distribution of the leading jet \pt at detector level matches that observed in the data. The modified \SHERPAtwotwo samples are then used to unfold the data again and the variations in the resulting cross sections are used to derive a systematic uncertainty.  

\item An additional check is performed by unfolding  reconstructed \MGaMCPyCKKWL events using \SHERPAtwotwo response matrices. The residual non-closure is accounted for by an additional flat uncertainty of  3\% for all distributions.


\end{itemize}




 

%-------------------------------------------------------------------------------
\section{Results}
\label{sec:results}

The measured cross sections, presented in Section~\ref{sec:results_channels}, are calculated in the electron and muon channels separately and the compatibility of the results of the two channels is evaluated.  In order to improve the precision of the measurement, these results are then combined, taking into account the correlations of the systematic uncertainties. 
The comparisons of the combined results to the predictions are presented in Section~\ref{sec:comparison}.

\subsection{Results in the individual channels and the combination}
\label{sec:results_channels} 


The fiducial cross-section measurements in the  \Ztoeej and  \Ztommj channels as a function of the inclusive jet multiplicities are presented in Table~\ref{tab:zjets_njet}. The data statistical uncertainties are propagated through the unfolding by using pseudo-experiments. As mentioned in Section~\ref{sec:unfolding}, the systematic uncertainties  are propagated through the unfolding via the migration matrices and via the variation of the subtracted background.  Table~\ref{tab:systot_ell} shows the resulting total relative statistical and systematic uncertainties as well as the systematic components (lepton trigger, lepton selection, jet energy scale and resolution, jet vertex tagging, pile-up, luminosity (all described in Section~\ref{sec:uncertainties})), unfolding (described in Section~\ref{sec:unfolding}), and background (described in Section~\ref{sec:backgrounds}) as a function of the inclusive jet multiplicity, presented separately for the electron and muon channels. 
The jet energy scale is the dominant systematic uncertainty for all bins with at least one jet.

\input{Results_table_single_cross_noratio}
\input{Systematics_table}


Figure~\ref{fig:comp_Nin} shows a comparison of the electron and muon channels for the measured fiducial cross section as a function of the inclusive jet multiplicity and of the leading jet \pt\ for inclusive \Zonej events. This figure demonstrates that the results in the electron and muon channels are compatible and hence can be combined to improve the precision of the measurement. This figure also shows the result of this combination described below.

\begin{figure}[p]
\begin{center}
\includegraphics[width=0.48\textwidth]{./figures/comp_hJetNTin_uncorr.pdf}
\includegraphics[width=0.48\textwidth]{./figures/comp_hJet1PtT_uncorr.pdf}
\caption{Measured fiducial cross section as a function of the inclusive jet multiplicity (left) and the leading jet \pt\ for inclusive \Zonej events (right) in the electron and the muon channels and compared to their combined value. The ratios of the two measurements to the combined results are also shown in the bottom panels. 
The error bars indicate the statistical uncertainty, and the hatched bands 
the statistical and the flavour-uncorrelated systematic uncertainties of the combined result, added in quadrature.}
\label{fig:comp_Nin}
\end{center}
\end{figure}


\clearpage

The results from the electron and muon channels are combined at dressed level for each distribution separately: inclusive and exclusive jet multiplicities, ratio for successive inclusive jet multiplicities, leading jet \pT for \Zonefourj events and jet \pT for exclusive  \Zexclj events, leading jet rapidity for inclusive \Zonej events, \HT,  \Dphijj, and \mjj. A $\chi^2$ function whose sum runs over all measurement sets (electrons and muons), measurement points, and some of the uncertainty sources, is used for the combination~\cite{Glazov:2005rn,Aaron:2009bp} and distinguishes between bin-to-bin correlated and uncorrelated sources of uncertainties, the latter comprising the statistical uncertainty of the data and the statistical unfolding uncertainty.  Uncertainties specific to the lepton flavour and to the background are included in the $\chi^2$ function, while the remaining, flavour-uncorrelated,  systematic uncertainties related to jets, pile-up, luminosity, and unfolding are averaged after the combination.


\begin{figure}[t]
\begin{center}
\includegraphics[width=0.48\textwidth]{./figures/results_comb_hJetNTin.pdf}
\includegraphics[width=0.48\textwidth]{./figures/results_comb_hJetNTratio.pdf}
\caption{Measured cross section as a function of the inclusive jet multiplicity (left) and ratio for successive  inclusive jet multiplicities (right) for inclusive \Zj events. 
The data are compared to the predictions from \BLACKHATSHERPA, \SHERPAtwotwo, \ALPGENPysix, \MGaMCPyCKKWL, and \MGaMCPyFxFx. The error bars correspond to the statistical uncertainty, and the hatched bands to the data statistical and systematic uncertainties (including luminosity) added in quadrature.
A constant  5\% theoretical uncertainty is used for \SHERPAtwotwo, \ALPGENPysix, \MGaMCPyCKKWL, and \MGaMCPyFxFx. Uncertainties from the parton distribution
 functions and QCD scale variations are included in the \BLACKHATSHERPA predictions, as described in Section~\ref{sec:dataMCFO}.}
\label{fig:xs_NinR_comb}
\end{center}
\end{figure} 
  
\subsection{Comparisons of results to predictions}
\label{sec:comparison}


The cross-section measurement for different inclusive \Zj multiplicities and their ratios obtained from the combination are found in Tables~\ref{tab:zjets_njet_comb} and~\ref{tab:zjets_njet_ratio_comb}. Figure~\ref{fig:xs_NinR_comb} shows the comparison of these results with the NLO QCD fixed-order calculations from \BLACKHATSHERPA and with the predictions from  \SHERPAtwotwo, \ALPGENPysix,  \MGaMCPyCKKWL, and \MGaMCPyFxFx. The plots show the particle-level cross section with the generator predictions normalised to the inclusive NNLO cross sections in the top panel, accompanied by the ratios of the various predictions with respect to the data in the bottom panels. Uncertainties from the parton distribution functions and QCD scale variations are included in the \BLACKHATSHERPA predictions, as described in Section~\ref{sec:dataMCFO}.
A constant  5\% theoretical uncertainty is used for \SHERPAtwotwo, \ALPGENPysix, \MGaMCPyCKKWL, and \MGaMCPyFxFx, as described in Table~\ref{tab:MC}.
The inclusive jet multiplicity decreases logarithmically while the ratio is flat in the presence of at least one jet.
The predictions are in agreement with the observed cross sections and their ratios, except for \SHERPAtwotwo, \ALPGENPysix and \MGaMCPyFxFx for high jet multiplicity, 
where a non-negligible fraction of the jets are produced by the parton shower.

\input{Combination_table}
    
\begin{figure}[t]
\begin{center}
\includegraphics[width=0.48\textwidth]{./figures/results_comb_hJet1Ptcomb.pdf}
\includegraphics[width=0.48\textwidth]{./figures/results_comb_hJet1EtaAbsT.pdf}
\caption{Measured cross section as a function of the leading jet \pt\ for inclusive \Zonefourj events (left) and absolute value of the leading jet rapidity for inclusive \Zonej events (right). 
The data are compared to the predictions from \Njetti, \BLACKHATSHERPA, \SHERPAtwotwo, \ALPGENPysix, \MGaMCPyCKKWL, and \MGaMCPyFxFx. 
The error bars correspond to the statistical uncertainty, and the hatched bands to the data statistical and systematic uncertainties (including luminosity) added in quadrature. 
The details of the prediction uncertainties are given in the text.
For clarity, uncertainty bands are not shown for the Monte Carlo predictions in the left-hand plot.
Uncertainties from the QCD scale variations for the \Njetti predictions are included, as described in Section~\ref{sec:dataMCFO}. }
\label{fig:xs_Jet1PtNj_comb}
\end{center}
\end{figure}

\begin{figure}[t]
\begin{center}
\includegraphics[width=0.48\textwidth]{./figures/results_comb_hJetPtT.pdf}
\includegraphics[width=0.48\textwidth]{./figures/results_comb_hJetNTex.pdf}
\caption{Measured cross section as a function of jet \pt\ for exclusive \Zexclj events (left) and exclusive jet multiplicity (right). 
The data are compared to the predictions from \BLACKHATSHERPA, \SHERPAtwotwo, \ALPGENPysix, \MGaMCPyCKKWL, and \MGaMCPyFxFx. The error bars correspond to the statistical uncertainty, and the hatched bands to the data statistical and systematic uncertainties (including luminosity) added in quadrature. 
The details of the prediction uncertainties are given in the text.}
\label{fig:xs_Jet1PtNjexcl_comb}
\end{center}  
\end{figure}

The jet transverse momentum is a fundamental observable of the \Zj process and probes pQCD over a wide range of scales. Moreover, understanding the kinematics of jets in events with vector bosons associated with several jets is essential for the modelling of backgrounds for other SM processes and searches beyond the SM.
The leading jet \pt\ distribution (which is correlated with the \pT of the \Zboson boson) in inclusive \Zonefourj events is shown in Figure~\ref{fig:xs_Jet1PtNj_comb} and ranges up to 700~GeV. The LO generator \MGaMCPyCKKWL models a too-hard  jet \pt\ spectrum. This feature is known from studies of LO generators in $pp$ collisions at lower centre-of-mass energies~\cite{Zjets2013}, and can be interpreted as an indication that the dynamic factorisation and renormalisation scale used in the generation is not appropriate for the full jet \pt\ range.
In contrast, the predictions from  \BLACKHATSHERPA, \SHERPAtwotwo, and \MGaMCPyFxFx, which are based on NLO matrix elements,  are in agreement  with the measured cross section within the systematic uncertainties over the full leading jet \pt\ range. \ALPGENPysix also shows good agreement with the measured data. The \Njetti prediction models the spectrum for the \Zonej events well. Uncertainties from the QCD scale variations for the \Njetti predictions are included in the uncertainty band, as described in Section~\ref{sec:dataMCFO}. 
For the leading jet rapidity distribution in inclusive \Zonej events, also shown in this figure, all predictions show good agreement with the measured data within the uncertainties.

The exclusive jet \pt\ distribution probes the validity of  \Zexclj predictions at increasing QCD scales represented by the jet \pT\ in the presence of a jet veto at a constant low scale; for a jet \pt\ range of several hundred GeV, accessible with the current data set, the jet scale is of order ten times larger than the veto scale (30~GeV).
Figure~\ref{fig:xs_Jet1PtNjexcl_comb} demonstrates that all predictions studied are consistent with the data within systematic uncertainties over the full jet \pt\ range (up to 500~GeV).
This figure also shows the measured cross section as a function of the exclusive jet multiplicity, which decreases logarithmically. 
Similar trends as for the inclusive jet multiplicity (Figure~\ref{fig:xs_NinR_comb}) are observed.

\begin{figure}[t]
\begin{center}
\includegraphics[width=0.48\textwidth]{./figures/results_comb_hHT1jT.pdf}
\caption{Measured cross section as a function of \HT for inclusive \Zonej events. 
The data are compared to the predictions from  \Njetti, \BLACKHATSHERPA, \SHERPAtwotwo, \ALPGENPysix, \MGaMCPyCKKWL, and \MGaMCPyFxFx. The error bars correspond to the statistical uncertainty, and the hatched bands to the data statistical and systematic uncertainties (including luminosity) added in quadrature. The details of the prediction uncertainties are given in the text.}
\label{fig:xs_HT1jY_comb}
\end{center}
\end{figure}

Quantities based on inclusive \pT sums of final-state objects, such as \HT, the scalar \pT sum of all visible objects in the final state, are often employed in searches for physics beyond the Standard Model, to enrich final states resulting from the decay of heavy particles. The values \HT or  \HT/2 are also commonly used choices for scales for higher-order perturbative QCD calculations.  Large values for this quantity can result either from a small number of very energetic particles or from a large number of less energetic particles.  Figure~\ref{fig:xs_HT1jY_comb} shows the measured cross sections as a function of the \HT distribution (up to 1400~GeV) in inclusive \Zonej events. The predictions from \SHERPAtwotwo, \ALPGENPysix  and \MGaMCPyFxFx describe well the \HT distribution. The prediction from \MGaMCPyCKKWL describes well the turn-over in the softer part of the \HT spectrum, but overestimates the contribution at large values of \HT, in line with the overestimate of the cross sections for hard jets. The fixed-order \Zonej prediction from \BLACKHATSHERPA underestimates the cross section for values of $\HT>300$~GeV, as observed in similar measurements at lower centre-of-mass energies~\cite{Zjets2013,mySTDM-2012-24}, due to the missing contributions from events with higher parton multiplicities, which for large values of \HT constitute a substantial portion of the data. Agreement is recovered by adding higher orders in perturbative QCD, as demonstrated by the good description of \HT by \Njetti.

 
\begin{figure}[t]
\begin{center}
\includegraphics[width=0.48\textwidth]{./figures/results_comb_hJetDPhiT.pdf}
\includegraphics[width=0.48\textwidth]{./figures/results_comb_hMjjT.pdf}
\caption{Measured cross section as a function of \Dphijj (left) and \mjj (right) for inclusive \Ztwoj events. 
The data are compared to the predictions from \BLACKHATSHERPA, \SHERPAtwotwo, \ALPGENPysix, \MGaMCPyCKKWL, and \MGaMCPyFxFx. The error bars correspond to the statistical uncertainty, and the hatched bands to the data statistical and systematic uncertainties (including luminosity) added in quadrature. The details of the prediction uncertainties are given in the text.}
\label{fig:xs_JetDphiM_comb}
\end{center}
\end{figure}

Angular relations between the two leading jets and the dijet mass are frequently used to separate either heavier SM particles or beyond-SM physics from the \Zj process. 
Figure~\ref{fig:xs_JetDphiM_comb} shows the differential cross section as a function of azimuthal angular difference between the two leading jets for \Ztwoj events, \Dphijj. The tendency of the two jets to be back-to-back in the transverse plane is well modelled by all predictions. This figure also shows the measured cross sections as a function of the invariant mass \mjj of the two leading jets for \Ztwoj events. The shape of the dijet mass is modelled well by \BLACKHATSHERPA, \SHERPAtwotwo, \ALPGENPysix, and \MGaMCPyFxFx, whereas \MGaMCPyCKKWL shows a harder spectrum.

\clearpage








%-------------------------------------------------------------------------------
\section{Conclusion}
\label{sec:conclusion}


Proton--proton collision data at $\sqrt{s}=13$~TeV  from the LHC, corresponding to a total integrated luminosity of 3.16~fb$^{-1}$, have been analysed by the ATLAS collaboration to study events with \Zboson bosons decaying to electron or muon pairs, produced in association with one or more jets.
The fiducial production cross sections for \Zzerosevenj have been measured, within the acceptance region defined by $\pT^{\ell}>25$~GeV, $|\eta^{\ell}|<2.5$, $71<m_{\ell\ell}<111$~GeV, $\pTj > 30$~GeV, $|\yj|<2.5$, and $\Delta R(\ell,\text{jet}) > 0.4$, with a precision ranging from 4\% to 30\%. Ratios of cross sections for successive jet multiplicities and cross-section measurements as a function of different key variables such as the jet multiplicities, jet \pt\ for exclusive $Z+1$~jet events, leading jet \pt\ for \Zonefourj events, leading jet rapidity for \Zonej events, $H_{\text{T}}$, $\Delta\phi_{\text{jj}}$ and $m_{\text{jj}}$ have also been derived.

The measurements have  been compared to fixed-order calculations at NLO from \BLACKHATSHERPA and at NNLO from the \Njetti calculation, and to predictions from the generators 
\SHERPAtwotwo, \ALPGENPysix, \MGaMCPyCKKWL, and \MGaMCPyFxFx.
In general, the predictions are in good agreement with the observed cross sections and cross-section ratios within the uncertainties.
Distributions which are dominated by a single jet multiplicity are modelled well by fixed-order NLO calculations, even in the presence of a jet veto at a low scale.
The \textsc{ME+PS} generator \MGaMCPyCKKWL, which is based on LO matrix elements, models a too-hard jet spectrum, as observed in $\sqrt{s}=7$~TeV $pp$ collisions. It however models well the inclusive jet multiplicity distribution over the full multiplicity range. The modelling of the jet \pt and related observables is significantly improved by the \textsc{ME+PS@NLO} generators \SHERPAtwotwo  and \MGaMCPyFxFx, which use NLO matrix elements for up to two additional partons. The recent \Njetti predictions describe well key distributions such as the leading jet \pt\ and \HT.

The results presented in this paper provide essential input for the further optimisation of the Monte Carlo generators of \Zj production and constitute a powerful test of perturbative QCD for processes with a higher number of partons in the final state.


 
%-------------------------------------------------------------------------------
\section*{Acknowledgements}
%-------------------------------------------------------------------------------

% Acknowledgements for papers with collision data
% Version 06-Mar-2017

% Standard acknowledgements start here
%----------------------------------------------
We thank CERN for the very successful operation of the LHC, as well as the
support staff from our institutions without whom ATLAS could not be
operated efficiently.

We acknowledge the support of ANPCyT, Argentina; YerPhI, Armenia; ARC, Australia; BMWFW and FWF, Austria; ANAS, Azerbaijan; SSTC, Belarus; CNPq and FAPESP, Brazil; NSERC, NRC and CFI, Canada; CERN; CONICYT, Chile; CAS, MOST and NSFC, China; COLCIENCIAS, Colombia; MSMT CR, MPO CR and VSC CR, Czech Republic; DNRF and DNSRC, Denmark; IN2P3-CNRS, CEA-DSM/IRFU, France; SRNSF, Georgia; BMBF, HGF, and MPG, Germany; GSRT, Greece; RGC, Hong Kong SAR, China; ISF, I-CORE and Benoziyo Center, Israel; INFN, Italy; MEXT and JSPS, Japan; CNRST, Morocco; NWO, Netherlands; RCN, Norway; MNiSW and NCN, Poland; FCT, Portugal; MNE/IFA, Romania; MES of Russia and NRC KI, Russian Federation; JINR; MESTD, Serbia; MSSR, Slovakia; ARRS and MIZ\v{S}, Slovenia; DST/NRF, South Africa; MINECO, Spain; SRC and Wallenberg Foundation, Sweden; SERI, SNSF and Cantons of Bern and Geneva, Switzerland; MOST, Taiwan; TAEK, Turkey; STFC, United Kingdom; DOE and NSF, United States of America. In addition, individual groups and members have received support from BCKDF, the Canada Council, CANARIE, CRC, Compute Canada, FQRNT, and the Ontario Innovation Trust, Canada; EPLANET, ERC, ERDF, FP7, Horizon 2020 and Marie Sk{\l}odowska-Curie Actions, European Union; Investissements d'Avenir Labex and Idex, ANR, R{\'e}gion Auvergne and Fondation Partager le Savoir, France; DFG and AvH Foundation, Germany; Herakleitos, Thales and Aristeia programmes co-financed by EU-ESF and the Greek NSRF; BSF, GIF and Minerva, Israel; BRF, Norway; CERCA Programme Generalitat de Catalunya, Generalitat Valenciana, Spain; the Royal Society and Leverhulme Trust, United Kingdom.

The crucial computing support from all WLCG partners is acknowledged gratefully, in particular from CERN, the ATLAS Tier-1 facilities at TRIUMF (Canada), NDGF (Denmark, Norway, Sweden), CC-IN2P3 (France), KIT/GridKA (Germany), INFN-CNAF (Italy), NL-T1 (Netherlands), PIC (Spain), ASGC (Taiwan), RAL (UK) and BNL (USA), the Tier-2 facilities worldwide and large non-WLCG resource providers. Major contributors of computing resources are listed in Ref.~\cite{ATL-GEN-PUB-2016-002}.
%----------------------------------------------


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\clearpage


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\newpage 
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\end{document}
 

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    \endverb
    \field{pages}{11}
    \field{title}{{Measurements of fiducial cross-sections for $t\bar{t}$
  production with one or two additional b-jets in pp collisions at $\sqrt{s} =
  8$~TeV using the ATLAS detector}}
    \field{volume}{76}
    \field{journaltitle}{Eur. Phys. J. C}
    \field{eprinttype}{arXiv}
    \field{eprintclass}{hep-ex}
    \field{year}{2016}
  \endentry

  \entry{Aad:2014lwa}{article}{}
    \name{author}{1}{}{%
      {{hash=A}{%
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         familyi={A\bibinitperiod},
      }}%
    }
    \strng{namehash}{A1}
    \strng{fullhash}{A1}
    \field{labelnamesource}{author}
    \field{labeltitlesource}{title}
    \verb{doi}
    \verb 10.1007/JHEP09(2014)112
    \endverb
    \verb{eprint}
    \verb 1407.4222
    \endverb
    \field{pages}{112}
    \field{title}{{Measurements of fiducial and differential cross sections for
  Higgs boson production in the diphoton decay channel at $\sqrt{s}=8$ TeV with
  ATLAS}}
    \field{volume}{09}
    \field{journaltitle}{JHEP}
    \field{eprinttype}{arXiv}
    \field{eprintclass}{hep-ex}
    \field{year}{2014}
  \endentry

  \entry{Cacciari:2008}{article}{}
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      {{hash=CM}{%
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         familyi={C\bibinitperiod},
         given={Matteo},
         giveni={M\bibinitperiod},
      }}%
      {{hash=SGP}{%
         family={Salam},
         familyi={S\bibinitperiod},
         given={Gavin\bibnamedelima P.},
         giveni={G\bibinitperiod\bibinitdelim P\bibinitperiod},
      }}%
      {{hash=SG}{%
         family={Soyez},
         familyi={S\bibinitperiod},
         given={Gregory},
         giveni={G\bibinitperiod},
      }}%
    }
    \strng{namehash}{CMSGPSG1}
    \strng{fullhash}{CMSGPSG1}
    \field{labelnamesource}{author}
    \field{labeltitlesource}{title}
    \verb{doi}
    \verb 10.1088/1126-6708/2008/04/063
    \endverb
    \verb{eprint}
    \verb 0802.1189
    \endverb
    \field{pages}{063}
    \field{title}{{The Anti-$k_t$ jet clustering algorithm}}
    \field{volume}{04}
    \field{journaltitle}{JHEP}
    \field{eprinttype}{arXiv}
    \field{eprintclass}{hep-ph}
    \field{year}{2008}
  \endentry

  \entry{Aad:2016upy}{article}{}
    \name{author}{1}{}{%
      {{hash=A}{%
         family={{ATLAS Collaboration}},
         familyi={A\bibinitperiod},
      }}%
    }
    \strng{namehash}{A1}
    \strng{fullhash}{A1}
    \field{labelnamesource}{author}
    \field{labeltitlesource}{title}
    \verb{eprint}
    \verb 1603.02934
    \endverb
    \field{title}{{Topological cell clustering in the ATLAS calorimeters and
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    \field{year}{2016}
  \endentry

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    \name{author}{1}{}{%
      {{hash=A}{%
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         familyi={A\bibinitperiod},
      }}%
    }
    \strng{namehash}{A1}
    \strng{fullhash}{A1}
    \field{labelnamesource}{author}
    \field{labeltitlesource}{title}
    \field{howpublished}{{ATL-PHYS-PUB-2015-015}}
    \field{title}{{Jet Calibration and Systematic Uncertainties for Jets
  Reconstructed in the ATLAS Detector at $\sqrt{s}=13\;\mbox{TeV}$}}
    \verb{url}
    \verb https://cdsweb.cern.ch/record/2028594
    \endverb
    \field{year}{2015}
  \endentry

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      {{hash=A}{%
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         familyi={A\bibinitperiod},
      }}%
    }
    \strng{namehash}{A1}
    \strng{fullhash}{A1}
    \field{labelnamesource}{author}
    \field{labeltitlesource}{title}
    \field{howpublished}{{ATLAS-CONF-2014-018}}
    \field{title}{{Tagging and suppression of pileup jets with the ATLAS
  detector}}
    \verb{url}
    \verb https://cds.cern.ch/record/1700870
    \endverb
    \field{year}{2014}
  \endentry

  \entry{Aad:2015ina}{article}{}
    \name{author}{1}{}{%
      {{hash=A}{%
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         familyi={A\bibinitperiod},
      }}%
    }
    \strng{namehash}{A1}
    \strng{fullhash}{A1}
    \field{labelnamesource}{author}
    \field{labeltitlesource}{title}
    \verb{doi}
    \verb 10.1140/epjc/s10052-016-4395-z
    \endverb
    \verb{eprint}
    \verb 1510.03823
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    \field{number}{11}
    \field{pages}{581}
    \field{title}{{Performance of pile-up mitigation techniques for jets in
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    \field{volume}{76}
    \field{journaltitle}{Eur. Phys. J. C}
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    \field{eprintclass}{hep-ex}
    \field{year}{2016}
  \endentry

  \entry{DAPR-2011-01}{article}{}
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      {{hash=A}{%
         family={{ATLAS Collaboration}},
         familyi={A\bibinitperiod},
      }}%
    }
    \strng{namehash}{A1}
    \strng{fullhash}{A1}
    \field{labelnamesource}{author}
    \field{labeltitlesource}{title}
    \verb{doi}
    \verb 10.1140/epjc/s10052-013-2518-3
    \endverb
    \verb{eprint}
    \verb 1302.4393
    \endverb
    \field{pages}{2518}
    \field{title}{{Improved luminosity determination in $pp$ collisions at
  $\sqrt{s} = 7\;\mbox{TeV}$ using the ATLAS detector at the LHC}}
    \field{volume}{73}
    \field{journaltitle}{Eur. Phys. J. C}
    \field{eprinttype}{arXiv}
    \field{eprintclass}{hep-ex}
    \field{year}{2013}
  \endentry

  \entry{Aaboud:2016hhf}{article}{}
    \name{author}{1}{}{%
      {{hash=A}{%
         family={{ATLAS Collaboration}},
         familyi={A\bibinitperiod},
      }}%
    }
    \strng{namehash}{A1}
    \strng{fullhash}{A1}
    \field{labelnamesource}{author}
    \field{labeltitlesource}{title}
    \verb{doi}
    \verb 10.1140/epjc/s10052-016-4466-1
    \endverb
    \verb{eprint}
    \verb 1608.03953
    \endverb
    \field{pages}{653}
    \field{title}{{Luminosity determination in pp collisions at $\sqrt{s}$ = 8
  TeV using the ATLAS detector at the LHC}}
    \field{volume}{76}
    \field{journaltitle}{Eur. Phys. J. C}
    \field{eprinttype}{arXiv}
    \field{eprintclass}{hep-ex}
    \field{year}{2016}
  \endentry

  \entry{ATLAS-CONF-2015-065}{booklet}{}
    \name{author}{1}{}{%
      {{hash=A}{%
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         familyi={A\bibinitperiod},
      }}%
    }
    \strng{namehash}{A1}
    \strng{fullhash}{A1}
    \field{labelnamesource}{author}
    \field{labeltitlesource}{title}
    \field{howpublished}{{ATLAS-CONF-2015-065}}
    \field{title}{{Measurement of jets produced in top quark events using the
  di-lepton final state with 2 $b$-tagged jets in $pp$ collisions at $\sqrt{s}
  = 13\;\mbox{TeV}$ with the ATLAS detector}}
    \verb{url}
    \verb https://cds.cern.ch/record/2114832
    \endverb
    \field{year}{2015}
  \endentry

  \entry{Aaboud:2016yus}{article}{}
    \name{author}{1}{}{%
      {{hash=A}{%
         family={{ATLAS Collaboration}},
         familyi={A\bibinitperiod},
      }}%
    }
    \strng{namehash}{A1}
    \strng{fullhash}{A1}
    \field{labelnamesource}{author}
    \field{labeltitlesource}{title}
    \verb{doi}
    \verb 10.1016/j.physletb.2016.08.052
    \endverb
    \verb{eprint}
    \verb 1606.04017
    \endverb
    \field{pages}{1}
    \field{title}{{Measurement of the $W^{\pm}Z$ boson pair-production cross
  section in $pp$ collisions at $\sqrt{s}=13$~TeV with the ATLAS Detector}}
    \field{volume}{762}
    \field{journaltitle}{Phys. Lett. B}
    \field{eprinttype}{arXiv}
    \field{eprintclass}{hep-ex}
    \field{year}{2016}
  \endentry

  \entry{D'Agostini:1994zf}{article}{}
    \name{author}{1}{}{%
      {{hash=DG}{%
         family={D'Agostini},
         familyi={D\bibinitperiod},
         given={G.},
         giveni={G\bibinitperiod},
      }}%
    }
    \strng{namehash}{DG1}
    \strng{fullhash}{DG1}
    \field{labelnamesource}{author}
    \field{labeltitlesource}{title}
    \verb{doi}
    \verb 10.1016/0168-9002(95)00274-X
    \endverb
    \field{pages}{487}
    \field{title}{{A Multidimensional unfolding method based on Bayes'
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    \field{volume}{362}
    \field{journaltitle}{Nucl. Instrum. Meth. A}
    \field{year}{1995}
  \endentry

  \entry{RooUnfold}{misc}{}
    \field{note}{The RooUnfold package and documentation are available from}
    \verb{url}
    \verb http://hepunx.rl.ac.uk/~adye/software/unfold/RooUnfold.html
    \endverb
  \endentry

  \entry{Glazov:2005rn}{article}{}
    \name{author}{1}{}{%
      {{hash=GA}{%
         family={Glazov},
         familyi={G\bibinitperiod},
         given={A.},
         giveni={A\bibinitperiod},
      }}%
    }
    \strng{namehash}{GA1}
    \strng{fullhash}{GA1}
    \field{labelnamesource}{author}
    \field{labeltitlesource}{title}
    \field{booktitle}{{Deep inelastic scattering, 13th International Workshop
  on Deep Inelastic Scattering, DIS 2005, Madison, Wisconsin, 27 April-1 May
  2005}}
    \verb{doi}
    \verb 10.1063/1.2122026
    \endverb
    \field{pages}{237\bibrangedash 240}
    \field{title}{{Averaging of DIS cross section data}}
    \field{volume}{792}
    \field{journaltitle}{AIP Conf. Proc.}
    \field{year}{2005}
  \endentry

  \entry{Aaron:2009bp}{article}{}
    \true{moreauthor}
    \name{author}{1}{}{%
      {{hash=AFD}{%
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         familyi={A\bibinitperiod},
         given={F.\bibnamedelima D.},
         giveni={F\bibinitperiod\bibinitdelim D\bibinitperiod},
      }}%
    }
    \strng{namehash}{AFD+1}
    \strng{fullhash}{AFD+1}
    \field{labelnamesource}{author}
    \field{labeltitlesource}{title}
    \verb{doi}
    \verb 10.1140/epjc/s10052-009-1128-6
    \endverb
    \verb{eprint}
    \verb 0904.0929
    \endverb
    \field{pages}{625\bibrangedash 678}
    \field{title}{\protect{Measurement of the Inclusive ep Scattering Cross
  Section at Low $Q^2$ and $x$ at HERA}}
    \field{volume}{63}
    \field{journaltitle}{Eur. Phys. J. C}
    \field{eprinttype}{arXiv}
    \field{eprintclass}{hep-ex}
    \field{year}{2009}
  \endentry

  \entry{mySTDM-2012-24}{article}{}
    \name{author}{1}{}{%
      {{hash=A}{%
         family={{ATLAS Collaboration}},
         familyi={A\bibinitperiod},
      }}%
    }
    \strng{namehash}{A1}
    \strng{fullhash}{A1}
    \field{labelnamesource}{author}
    \field{labeltitlesource}{title}
    \verb{doi}
    \verb 10.1140/epjc/s10052-015-3262-7
    \endverb
    \verb{eprint}
    \verb 1409.8639
    \endverb
    \field{pages}{82}
    \field{title}{{Measurements of the $W$ production cross sections in
  association with jets with the ATLAS detector}}
    \field{volume}{75}
    \field{journaltitle}{Eur. Phys. J. C}
    \field{eprinttype}{arXiv}
    \field{eprintclass}{hep-ex}
    \field{year}{2015}
  \endentry

  \entry{ATL-GEN-PUB-2016-002}{booklet}{}
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    \field{labelnamesource}{author}
    \field{labeltitlesource}{title}
    \field{howpublished}{{ATL-GEN-PUB-2016-002}}
    \field{title}{{ATLAS Computing Acknowledgements 2016--2017}}
    \verb{url}
    \verb https://cdsweb.cern.ch/record/2202407
    \endverb
  \endentry
\endsortlist
\endinput
