\noindent A measurement of the production cross-section for \PZ bosons that decay to muons is presented. The data were recorded by the \lhcb detector during $pp$ collisions at a centre-of-mass energy of 7 \tev, and correspond to an integrated luminosity of 1.0 fb$^{-1$. The cross-section is measured for muons in the pseudorapidity range $2.0 \nolinebreak<\nolinebreak \eta \nolinebreak<\nolinebreak 4.5$ with transverse momenta $\pt \nolinebreak>\nolinebreak 20\gevc$. The dimuon mass is restricted to $60 \nolinebreak<\nolinebreak M_{\mu^{+\mu^{- \nolinebreak<\nolinebreak 120\gevcc$. The measured cross-section is $$\sigma_{Z\rightarrow\mu^{+\mu^{- = (76.0 \pm 0.3 \pm 0.5 \pm 1.0 \pm 1.3) \, \text{pb$$ where the uncertainties are due to the sample size, systematic effects, the beam energy and the luminosity.\enspace This result is in good agreement with theoretical predictions at next-to-next-to-leading order in perturbative quantum chromodynamics. The cross-section is also measured differentially as a function of kinematic variables of the \PZ boson. Ratios of the production cross-sections of electroweak bosons are presented using updated \lhcb measurements of \PW boson production. A precise test of the Standard Model is provided by the measurement of the ratio $$\frac{\sigma_{W^{+\rightarrow\mu^{+\nu_{\mu + \sigma_{W^{-\rightarrow\mu^{-\bar{\nu_{\mu{\sigma_{\PZ\rightarrow\mu^{+\mu^{- = 20.63\pm0.09\pm0.12\pm0.05,$$ where the uncertainty due to luminosity cancels.
acknowledgements.tex
\section*{Acknowledgements}
\iffalse
The text below are the acknowledgements as approved by the collaboration
board. Extending the acknowledgements to include individuals from outside the
collaboration who have contributed to the analysis should be approved by the
EB. The extra acknowledgements are placed after the standard acknowledgements, 
unless it matches with the text of the standard acknowledgements.
They should be included in the draft of first circulation.
\fi
\noindent We thank B.F.L. Ward for providing \mc@nlo + \herwig and \mc@nlo + \herwiri predictions.
We express our gratitude to our colleagues in the CERN
accelerator departments for the excellent performance of the LHC. We
thank the technical and administrative staff at the LHCb
institutes. We acknowledge support from CERN and from the national
agencies: CAPES, CNPq, FAPERJ and FINEP (Brazil); NSFC (China);
CNRS/IN2P3 (France); BMBF, DFG, HGF and MPG (Germany); INFN (Italy); 
FOM and NWO (The Netherlands); MNiSW and NCN (Poland); MEN/IFA (Romania); 
MinES and FANO (Russia); MinECo (Spain); SNSF and SER (Switzerland); 
NASU (Ukraine); STFC (United Kingdom); NSF (USA).
The Tier1 computing centres are supported by IN2P3 (France), KIT and BMBF 
(Germany), INFN (Italy), NWO and SURF (The Netherlands), PIC (Spain), GridPP 
(United Kingdom).
We are indebted to the communities behind the multiple open 
source software packages on which we depend. We are also thankful for the 
computing resources and the access to software R\&D tools provided by Yandex LLC (Russia).
Individual groups or members have received support from 
EPLANET, Marie Sk\l{}odowska-Curie Actions and ERC (European Union), 
Conseil g\'{e}n\'{e}ral de Haute-Savoie, Labex ENIGMASS and OCEVU, 
R\'{e}gion Auvergne (France), RFBR (Russia), XuntaGal and GENCAT (Spain), Royal Society and Royal
Commission for the Exhibition of 1851 (United Kingdom). 

appendix.tex
% $Id: appendix.tex 72978 2015-05-26 13:39:03Z rwallace $
% ===============================================================================
% Purpose: appendix to the standard template: standard symbol alises from Ulrik
% Author: Tomasz Skwarnicki
% Created on: 2009-09-24
% ===============================================================================

\clearpage

{\noindent\bf\Large Appendices}

\appendix

\section{Cross-sections}
\label{sec:difftab}

\begin{table}[h]
\caption{Inclusive differential cross-sections for \PZ boson production as a function of 
$y_{Z}$. Uncertainties are due to the sample size, 
systematic effects,
the beam energy and the luminosity. No candidates are observed in the 4.250 -- 4.500 bin.}
\label{tab:csZY}
\begin{center}
\begin{tabular}{c | c | c}
$y_{Z}$ & $\sigma_{\PZ}$ [pb] & $f_{\rm FSR}$\\ \hline

2.000 -- 2.125 &     0.969        $\pm$     0.039 $\pm$ 0.032 $\pm$ 0.012 $\pm$ 0.017 & 1.050$\pm$0.020\\
2.125 -- 2.250 &     2.840        $\pm$     0.063 $\pm$ 0.050 $\pm$ 0.036 $\pm$ 0.049 & 1.032$\pm$0.008\\
2.250 -- 2.375 &     4.428        $\pm$     0.077 $\pm$ 0.078 $\pm$ 0.055 $\pm$ 0.076 & 1.027$\pm$0.006\\
2.375 -- 2.500 &     5.823        $\pm$     0.088 $\pm$ 0.060 $\pm$ 0.073 $\pm$ 0.100 & 1.026$\pm$0.004\\
2.500 -- 2.625 &     6.877        $\pm$     0.095 $\pm$ 0.068 $\pm$ 0.086 $\pm$ 0.118 & 1.025$\pm$0.004\\
2.625 -- 2.750 &     7.669        $\pm$     0.100 $\pm$ 0.069 $\pm$ 0.096 $\pm$ 0.132 & 1.026$\pm$0.004\\
2.750 -- 2.875 &     8.306        $\pm$     0.104 $\pm$ 0.070 $\pm$ 0.104 $\pm$ 0.143 & 1.026$\pm$0.003\\
2.875 -- 3.000 &     8.241        $\pm$     0.103 $\pm$ 0.066 $\pm$ 0.103 $\pm$ 0.142 & 1.025$\pm$0.003\\
3.000 -- 3.125 &     7.783        $\pm$     0.099 $\pm$ 0.059 $\pm$ 0.097 $\pm$ 0.134 & 1.026$\pm$0.003\\
3.125 -- 3.250 &     7.094        $\pm$     0.096 $\pm$ 0.058 $\pm$ 0.089 $\pm$ 0.122 & 1.028$\pm$0.004\\
3.250 -- 3.375 &     5.894        $\pm$     0.087 $\pm$ 0.049 $\pm$ 0.074 $\pm$ 0.101 & 1.026$\pm$0.004\\
3.375 -- 3.500 &     4.160        $\pm$     0.073 $\pm$ 0.041 $\pm$ 0.052 $\pm$ 0.072 & 1.027$\pm$0.005\\
3.500 -- 3.625 &     2.896        $\pm$     0.061 $\pm$ 0.030 $\pm$ 0.036 $\pm$ 0.050 & 1.026$\pm$0.005\\
3.625 -- 3.750 &     1.741        $\pm$     0.047 $\pm$ 0.023 $\pm$ 0.022 $\pm$ 0.030 & 1.021$\pm$0.007\\
3.750 -- 3.875 &     0.825        $\pm$     0.032 $\pm$ 0.014 $\pm$ 0.010 $\pm$ 0.014 & 1.025$\pm$0.010\\
3.875 -- 4.000 &     0.321        $\pm$     0.020 $\pm$ 0.008 $\pm$ 0.004 $\pm$ 0.006 & 1.011$\pm$0.015\\
4.000 -- 4.250 &     0.115        $\pm$     0.013 $\pm$ 0.006 $\pm$ 0.001 $\pm$ 0.002 & 1.018$\pm$0.033\\
4.250 -- 4.500 &     $-$ & $-$\\

\end{tabular}
\end{center}
\end{table}

\begin{table}[h]
\caption{Inclusive differential cross-sections for \PZ boson production as a function 
of $p_{T,Z}$. Uncertainties are due to the sample 
size, systematic effects,
the beam energy and the luminosity.}
\label{tab:csZPT}
\begin{center}
\begin{tabular}{c | c | c}
 $p_{T,Z} [\gevc]$ & $\sigma_{\PZ}$ [pb] & $f_{\rm FSR}$\\ \hline

$\phantom{0}$0.0 -- $\phantom{00}$2.2 & 6.454           $\pm$     0.105$\pm$ 0.129 $\pm$ 0.081 $\pm$ 0.111 & 1.090$\pm$0.006\\
$\phantom{0}$2.2 -- $\phantom{00}$3.4 & 6.520           $\pm$     0.106$\pm$ 0.150 $\pm$ 0.081 $\pm$ 0.112 & 1.080$\pm$0.004\\
$\phantom{0}$3.4 -- $\phantom{00}$4.6 & 6.209           $\pm$     0.102$\pm$ 0.221 $\pm$ 0.078 $\pm$ 0.107 & 1.063$\pm$0.004\\
$\phantom{0}$4.6 -- $\phantom{00}$5.8 & 5.868           $\pm$     0.099$\pm$ 0.208 $\pm$ 0.073 $\pm$ 0.101 & 1.049$\pm$0.004\\
$\phantom{0}$5.8 -- $\phantom{00}$7.2 & 5.749           $\pm$     0.098$\pm$ 0.154 $\pm$ 0.072 $\pm$ 0.099 & 1.034$\pm$0.004\\
$\phantom{0}$7.2 -- $\phantom{00}$8.7 & 5.607           $\pm$     0.098$\pm$ 0.083 $\pm$ 0.070 $\pm$ 0.096 & 1.021$\pm$0.004\\
$\phantom{0}$8.7 -- $\phantom{0}$10.5 & 5.637           $\pm$     0.098$\pm$ 0.054 $\pm$ 0.070 $\pm$ 0.097 & 1.002$\pm$0.004\\
            10.5 -- $\phantom{0}$12.8 & 5.524           $\pm$     0.096$\pm$ 0.081 $\pm$ 0.069 $\pm$ 0.095 & 0.996$\pm$0.004\\
            12.8 -- $\phantom{0}$15.4 & 5.158           $\pm$     0.092$\pm$ 0.067 $\pm$ 0.064 $\pm$ 0.089 & 0.984$\pm$0.005\\
            15.4 -- $\phantom{0}$19.0 & 4.963           $\pm$     0.087$\pm$ 0.053 $\pm$ 0.062 $\pm$ 0.085 & 0.978$\pm$0.005\\
            19.0 -- $\phantom{0}$24.5 & 5.517           $\pm$     0.088$\pm$ 0.055 $\pm$ 0.069 $\pm$ 0.095 & 0.985$\pm$0.004\\
            24.5 -- $\phantom{0}$34.0 & 5.465           $\pm$     0.085$\pm$ 0.067 $\pm$ 0.068 $\pm$ 0.094 & 1.013$\pm$0.004\\
            34.0 -- $\phantom{0}$63.0 & 5.789           $\pm$     0.085$\pm$ 0.076 $\pm$ 0.072 $\pm$ 0.100 & 1.038$\pm$0.004\\
                        63.0 -- 270.0 & 1.516           $\pm$     0.043$\pm$ 0.044 $\pm$ 0.019 $\pm$ 0.026 & 1.060$\pm$0.007\\

\end{tabular}
\end{center}
\end{table}

\begin{table}[h]
\caption{Inclusive differential cross-sections for \PZ boson production as a function 
of $\phi^{*}_{Z}$. Uncertainties are due to the sample 
size, systematic effects, the beam energy and the luminosity.}
\label{tab:csZPHI}
\begin{center}
\begin{tabular}{c | c | c}
$\phi^{*}_{Z}$ & $\sigma_{\PZ}$ [pb] & $f_{\rm FSR}$\\ \hline

0.00 -- 0.01 & $\phantom{0}$8.549           $\pm$ 0.099 $\pm$ 0.088 $\pm$ 0.107 $\pm$ 0.147 & 1.034$\pm$0.004\\
0.01 -- 0.02 & $\phantom{0}$7.805           $\pm$ 0.096 $\pm$ 0.106 $\pm$ 0.098 $\pm$ 0.134 & 1.035$\pm$0.003\\
0.02 -- 0.03 & $\phantom{0}$7.051           $\pm$ 0.091 $\pm$ 0.083 $\pm$ 0.088 $\pm$ 0.121 & 1.034$\pm$0.004\\
0.03 -- 0.05 &             11.362           $\pm$ 0.114 $\pm$ 0.108 $\pm$ 0.142 $\pm$ 0.195 & 1.029$\pm$0.003\\
0.05 -- 0.07 & $\phantom{0}$8.124           $\pm$ 0.097 $\pm$ 0.120 $\pm$ 0.102 $\pm$ 0.140 & 1.026$\pm$0.003\\
0.07 -- 0.10 & $\phantom{0}$8.436           $\pm$ 0.097 $\pm$ 0.074 $\pm$ 0.105 $\pm$ 0.145 & 1.021$\pm$0.003\\
0.10 -- 0.15 & $\phantom{0}$8.611           $\pm$ 0.098 $\pm$ 0.131 $\pm$ 0.108 $\pm$ 0.148 & 1.020$\pm$0.003\\
0.15 -- 0.20 & $\phantom{0}$4.819           $\pm$ 0.073 $\pm$ 0.092 $\pm$ 0.060 $\pm$ 0.083 & 1.018$\pm$0.004\\
0.20 -- 0.30 & $\phantom{0}$5.206           $\pm$ 0.076 $\pm$ 0.058 $\pm$ 0.065 $\pm$ 0.090 & 1.019$\pm$0.004\\
0.30 -- 0.40 & $\phantom{0}$2.541           $\pm$ 0.054 $\pm$ 0.051 $\pm$ 0.032 $\pm$ 0.044 & 1.022$\pm$0.006\\
0.40 -- 0.60 & $\phantom{0}$2.018           $\pm$ 0.048 $\pm$ 0.060 $\pm$ 0.025 $\pm$ 0.035 & 1.024$\pm$0.007\\
0.60 -- 0.80 & $\phantom{0}$0.755           $\pm$ 0.029 $\pm$ 0.035 $\pm$ 0.009 $\pm$ 0.013 & 1.029$\pm$0.011\\
0.80 -- 1.20 & $\phantom{0}$0.457           $\pm$ 0.023 $\pm$ 0.018 $\pm$ 0.006 $\pm$ 0.008 & 1.025$\pm$0.014\\
1.20 -- 2.00 & $\phantom{0}$0.166           $\pm$ 0.014 $\pm$ 0.011 $\pm$ 0.002 $\pm$ 0.003 & 1.030$\pm$0.023\\
2.00 -- 4.00 & $\phantom{0}$0.045           $\pm$ 0.008 $\pm$ 0.017 $\pm$ 0.001 $\pm$ 0.001 & 1.031$\pm$0.041\\

\end{tabular}
\end{center}
\end{table}

\begin{sidewaystable}[h]
\caption{Inclusive differential cross-sections for \Wp (left) and \Wm (right) boson 
production as a function of muon $\eta$. Uncertainties 
are due to the sample size, systematic effects, the beam energy
and the luminosity. These supersede the results in Ref.~\cite{wmu}.}
\label{tab:csWETA}
\begin{center}
\begin{tabular}{c|c|c|c|c}

$\eta^{\mu}$ & $\sigma_{\Wp}$ [pb] & $f_{\rm FSR}^{\Wp}$ & $\sigma_{\Wm}$ [pb] & $f_{\rm FSR}^{\Wm}$ \\ \hline
2.00 -- 2.25 & $192.2 \pm 1.2 \pm 3.5 \pm 2.0 \pm 3.3$ & $1.016 \pm 0.004$ & $111.1 \pm 0.9 \pm 2.1 \pm 1.0 \pm 1.9$ & $1.019 \pm 0.003$ \\
2.25 -- 2.50 & $178.8 \pm 0.9 \pm 3.1 \pm 1.9 \pm 3.1$ & $1.018 \pm 0.004$ & $104.9 \pm 0.7 \pm 1.9 \pm 1.0 \pm 1.8$ & $1.015 \pm 0.003$ \\
2.50 -- 2.75 & $154.3 \pm 0.8 \pm 2.1 \pm 1.6 \pm 2.6$ & $1.025 \pm 0.005$ & $\phantom{0}96.1 \pm 0.7 \pm 1.3 \pm 0.9 \pm 1.6$ & $1.010 \pm 0.003$ \\
2.75 -- 3.00 & $122.8 \pm 0.7 \pm 1.6 \pm 1.3 \pm 2.1$ & $1.015 \pm 0.004$ & $\phantom{0}88.4 \pm 0.7 \pm 1.5 \pm 0.8 \pm 1.5$ & $1.007 \pm 0.002$ \\
3.00 -- 3.25 & $\phantom{0}94.3 \pm 0.6 \pm 1.3 \pm 1.0 \pm 1.6$ & $1.021 \pm 0.005$ & $\phantom{0}80.6 \pm 0.6 \pm 1.4 \pm 0.7 \pm 1.4$ & $1.009 \pm 0.003$ \\
3.25 -- 3.50 & $\phantom{0}61.6 \pm 0.5 \pm 0.9 \pm 0.7 \pm 1.1$ & $1.015 \pm 0.005$ & $\phantom{0}68.6 \pm 0.6 \pm 1.5 \pm 0.6 \pm 1.2$ & $1.017 \pm 0.005$ \\
3.50 -- 4.00 & $\phantom{0}60.0 \pm 0.5 \pm 0.7 \pm 0.6 \pm 1.0$ & $1.024 \pm 0.005$ & $\phantom{0}95.9 \pm 0.7 \pm 1.2 \pm 0.9 \pm 1.6$ & $1.012 \pm 0.005$ \\
4.00 -- 4.50 & $\phantom{0}14.3 \pm 0.4 \pm 0.4 \pm 0.2 \pm 0.2$ & $1.021 \pm 0.005$ & $\phantom{0}43.8 \pm 0.8 \pm 1.2 \pm 0.4 \pm 0.7$ & $1.000 \pm 0.000$ \\

\end{tabular}
\end{center}
\end{sidewaystable}

\clearpage

\begin{table}[h]
\caption{\Wp to \Wm boson production cross-section ratios as a function of
muon $\eta$. Uncertainties are due to the
sample size, systematic effects and the beam energy. These supersede the results in Ref.~\cite{wmu}.}
\label{tab:csrw}
\begin{center}
\begin{tabular}{c|c}
$\eta^{\mu}$ & $R_{W}$ \\ \hline
2.00 -- 2.25 & $1.730 \pm 0.018 \pm 0.030 \pm 0.003$ \\
2.25 -- 2.50 & $1.706 \pm 0.015 \pm 0.040 \pm 0.003$ \\
2.50 -- 2.75 & $1.606 \pm 0.014 \pm 0.021 \pm 0.002$ \\
2.75 -- 3.00 & $1.388 \pm 0.013 \pm 0.024 \pm 0.002$ \\
3.00 -- 3.25 & $1.169 \pm 0.012 \pm 0.021 \pm 0.002$ \\
3.25 -- 3.50 & $0.898 \pm 0.010 \pm 0.025 \pm 0.001$ \\
3.50 -- 4.00 & $0.626 \pm 0.007 \pm 0.006 \pm 0.001$ \\
4.00 -- 4.50 & $0.328 \pm 0.011 \pm 0.011 \pm 0.000$ \\
\end{tabular}
\end{center}
\end{table}


\begin{table}[h]
\caption{Lepton charge asymmetries as a function of muon $\eta$.
Uncertainties are due to the sample size, systematic  
effects and the beam energy. These supersede the results in Ref.~\cite{wmu}.}
\label{tab:csaw}
\begin{center}
\begin{tabular}{c|c}
$\eta^{\mu}$ & $A_{\mu}$ [\%] \\ \hline
2.00 -- 2.25 & \phantom{$-$}$26.74 \pm 0.48 \pm 0.82 \pm 0.07$ \\
2.25 -- 2.50 & \phantom{$-$}$26.08 \pm 0.41 \pm 1.09 \pm 0.07$ \\
2.50 -- 2.75 & \phantom{$-$}$23.25 \pm 0.42 \pm 0.60 \pm 0.07$ \\
2.75 -- 3.00 & \phantom{$-$}$16.26 \pm 0.46 \pm 0.84 \pm 0.07$ \\
3.00 -- 3.25 & \phantom{$-0$}$7.81 \pm 0.50 \pm 0.90 \pm 0.08$ \\
3.25 -- 3.50 & \phantom{$0$}$-5.37 \pm 0.57 \pm 1.35 \pm 0.08$ \\
3.50 -- 4.00 &                      $-23.04 \pm 0.52 \pm 0.49 \pm 0.07$ \\
4.00 -- 4.50 &                      $-50.65 \pm 1.22 \pm 1.30 \pm 0.06$ \\
\end{tabular}
\end{center}
\end{table}

\clearpage

\section{Correlation Matrices}
\label{sec:correlation}

\begin{sidewaystable}
 \caption{Correlation coefficients of differential cross-section 
measurements as a function of $y_{Z}$. The beam energy and luminosity 
uncertainties, which are 
fully correlated between cross-section measurements, are excluded.}
 \resizebox{25cm}{5cm}{
  \begin{tabular}{c | c c c c c c c c c c c c c c c c c c}

$y_{\PZ}$& \scriptsize{2--2.125} & \scriptsize{2.125--2.25} & \scriptsize{2.25--2.375} & \scriptsize{2.375--2.5} & \scriptsize{2.5--2.625} & \scriptsize{2.625--2.75} & 
\scriptsize{2.75--2.875} & \scriptsize{2.875--3} & \scriptsize{3--3.125} &
\scriptsize{3.125--3.25} & \scriptsize{3.25--3.375} & \scriptsize{3.375--3.5} & \scriptsize{3.5--3.625} &
\scriptsize{3.625--3.75} &
\scriptsize{3.75--3.875} & \scriptsize{3.875--4} & \scriptsize{4--4.25}  & \scriptsize{4.25--4.5} \\ \hline

\scriptsize{2--2.125} &1& & & & & & & & & & & & & & & & & \\   
\scriptsize{2.125--2.25} &0.18& 1& & & & & & & & & & & & & & & &  \\
\scriptsize{2.25--2.375} &0.14& 0.19& 1& & & & & & & & & & & & & & &  \\
\scriptsize{2.375--2.5} &0.14& 0.19& 0.18& 1&  & & & & & & & & & & & & & \\
\scriptsize{2.5--2.625} &0.13& 0.18& 0.16& 0.19& 1& & & & & & & & & & & & & \\ 
\scriptsize{2.625--2.75} &0.12& 0.16& 0.15& 0.18& 0.18& 1& & & & & & & & & & & & \\
\scriptsize{2.75--2.875} &0.11& 0.15& 0.14& 0.17& 0.17& 0.18& 1&   & & & & & & & & & & \\
\scriptsize{2.875--3} &0.10& 0.13& 0.13& 0.16& 0.16& 0.17& 0.17& 1& & & & & & & & & &  \\
\scriptsize{3--3.125} &0.09& 0.12& 0.12& 0.14& 0.15& 0.15& 0.16& 0.16& 1&  & & & & & & & & \\  
\scriptsize{3.125--3.25} &0.08& 0.1& 0.10& 0.12& 0.13& 0.14& 0.14& 0.14& 0.14& 1&   & & & & & & & \\ 
\scriptsize{3.25--3.375} &0.06& 0.08& 0.08& 0.11& 0.11& 0.12& 0.12& 0.13& 0.13& 0.13& 1&  & & & & & & \\
\scriptsize{3.375--3.5} &0.05& 0.06& 0.06& 0.08& 0.09& 0.09& 0.10& 0.10& 0.11& 0.11& 0.11& 1&  & & & & & \\
\scriptsize{3.5--3.625} &0.04& 0.05& 0.05& 0.06& 0.07& 0.08& 0.08& 0.09& 0.09& 0.10& 0.10& 0.10& 1& & & & &  \\ 
\scriptsize{3.625--3.75} &0.03& 0.04& 0.03& 0.04& 0.05& 0.06& 0.06& 0.07& 0.07& 0.08& 0.09& 0.08& 0.08& 1&  & & & \\
\scriptsize{3.75--3.875} &0.02& 0.03& 0.02& 0.03& 0.03& 0.04& 0.04& 0.05& 0.05& 0.06& 0.06& 0.06& 0.06& 0.06& 1&  & & \\
\scriptsize{3.875--4} &0.02& 0.02& 0.02& 0.02& 0.02& 0.02& 0.02& 0.03& 0.03& 0.04& 0.04& 0.04& 0.04& 0.04& 0.03& 1& & \\
\scriptsize{4--4.25} &0.01& 0.01& 0.01& 0.01& 0.01& 0.01& 0.01& 0.02& 0.02& 0.02& 0.03& 0.03& 0.03& 0.03& 0.02& 0.02& 1& \\
\scriptsize{4.25--4.5} &$-$& $-$& $-$& $-$& $-$& $-$& $-$& $-$& $-$& $-$& $-$& $-$& $-$& $-$& $-$& $-$& $-$& $-$ \\ \hline

\label{tab:correlY}
      \end{tabular}
}
\end{sidewaystable}

\begin{sidewaystable}
 \caption{Correlation coefficients of differential cross-section 
measurements as a function of $p_{T,Z}$. The beam energy and 
luminosity uncertainties, which 
are fully correlated between cross-section measurements, are excluded.}
 \resizebox{25cm}{5cm}{
  \begin{tabular}{c | c c c c c c c c c c c c c c }

$p_{T,Z}$ [GeV/c]& \scriptsize{0.0--2.2} & \scriptsize{2.2--3.4} & \scriptsize{3.4--4.6} & \scriptsize{4.6--5.8} & \scriptsize{5.8--7.2} & \scriptsize{7.2--8.7} 
& \scriptsize{8.7--10.5} & \scriptsize{10.5--12.8} &
\scriptsize{12.8--15.4} &
\scriptsize{15.4--19} & \scriptsize{19--24.5} & \scriptsize{24.5--34} & \scriptsize{34--63} &
\scriptsize{63--270} \\ \hline

\scriptsize{0.0--2.2} &1& & & & & & & & & & & & & \\
\scriptsize{2.2--3.4} &-0.01& 1& & & & & & & & & & & & \\
\scriptsize{3.4--4.6} &0.00& 0.03& 1& & & & & & & & & & & \\
\scriptsize{4.6--5.8} &0.04& 0.00& 0.02& 1& & & & & & & & & & \\
\scriptsize{5.8--7.2} &0.05& 0.05& 0.00& 0.03& 1& & & & & & & & & \\
\scriptsize{7.2--8.7} &0.07& 0.07& 0.05& 0.00& 0.03& 1& & & & & & & & \\
\scriptsize{8.7--10.5} &0.08& 0.08& 0.06& 0.06& 0.02& 0.02& 1& & & & & & & \\
\scriptsize{10.5--12.8} &0.07& 0.06& 0.05& 0.05& 0.07& 0.04& 0.00& 1& & & & & & \\
\scriptsize{12.8--15.4} &0.07& 0.07& 0.05& 0.05& 0.06& 0.09& 0.07& -0.01& 1& & & & & \\
\scriptsize{15.4--19} &0.08& 0.08& 0.05& 0.06& 0.07& 0.10& 0.12& 0.08& -0.01& 1& & & & \\
\scriptsize{19--24.5} &0.08& 0.08& 0.06& 0.06& 0.07& 0.10& 0.12& 0.10& 0.10& 0.02& 1& & &\\
\scriptsize{24.5--34} &0.08& 0.07& 0.05& 0.06& 0.07& 0.10& 0.11& 0.09& 0.10& 0.11& 0.05& 1& &\\
\scriptsize{34--63} &0.07& 0.06& 0.05& 0.05& 0.06& 0.08& 0.09& 0.08& 0.08& 0.09& 0.10& 0.06& 1& \\
\scriptsize{63--270} &0.20& 0.20& 0.15& 0.15& 0.19& 0.26& 0.30& 0.26& 0.27& 0.30& 0.32& 0.31& 0.30& 1\\ \hline

\label{tab:correlPt}
      \end{tabular}
}
\end{sidewaystable}

\begin{sidewaystable}
 \caption{Correlation coefficients of differential cross-section 
measurements as a function of $\phi^{*}_{Z}$. The beam energy and 
luminosity uncertainties, 
which are fully correlated between cross-section measurements, are excluded.}
 \resizebox{25cm}{5cm}{
  \begin{tabular}{c | c c c c c c c c c c c c c c c }
$\phi^{*}_{\PZ}$& \scriptsize{0.00--0.01} & \scriptsize{0.01--0.02} & \scriptsize{0.02--0.03} & \scriptsize{0.03--0.05}
& \scriptsize{0.05--0.07} & \scriptsize{0.07--0.10} & \scriptsize{0.10--0.15} & \scriptsize{0.15--0.20} &\scriptsize{0.20--0.30}
& \scriptsize{0.30--0.40} & \scriptsize{0.40--0.60} & \scriptsize{0.60--0.80} & \scriptsize{0.80--1.20} & \scriptsize{1.20--2.00} & \scriptsize{2.00--4.00} \\ \hline

\scriptsize{0.00--0.01} &1& & & & & & & & & & & & & & \\  
\scriptsize{0.01--0.02} &0.14& 1& & & & & & & & & & & & & \\
\scriptsize{0.02--0.03} &0.16& 0.12& 1& & & & & & & & & & & & \\
\scriptsize{0.03--0.05} &0.20& 0.17& 0.17& 1& & & & & & & & & & & \\
\scriptsize{0.05--0.07} &0.15& 0.12& 0.13& 0.16& 1& & & & & & & & & & \\
\scriptsize{0.07--0.10} &0.19& 0.16& 0.17& 0.21& 0.15& 1& & & & & & & & & \\
\scriptsize{0.10--0.15} &0.14& 0.12& 0.13& 0.16& 0.12& 0.15& 1& & & & & & & & \\
\scriptsize{0.15--0.20} &0.11& 0.10& 0.10& 0.13& 0.10& 0.12& 0.09& 1& & & & & & &\\
\scriptsize{0.20--0.30} &0.15& 0.13& 0.13& 0.17& 0.13& 0.16& 0.13& 0.10& 1& & & & & &\\
\scriptsize{0.30--0.40} &0.10& 0.08& 0.09& 0.11& 0.08& 0.10& 0.08& 0.06& 0.08& 1& & & & &\\
\scriptsize{0.40--0.60} &0.07& 0.06& 0.07& 0.08& 0.06& 0.08& 0.06& 0.05& 0.07& 0.04& 1& & & &\\
\scriptsize{0.60--0.80} &0.05& 0.04& 0.04& 0.05& 0.04& 0.05& 0.04& 0.03& 0.04& 0.03& 0.02& 1& & &\\
\scriptsize{0.80--1.20} &0.05& 0.04& 0.04& 0.05& 0.04& 0.05& 0.04& 0.03& 0.04& 0.03& 0.02& 0.01& 1& &\\
\scriptsize{1.20--2.00} &0.02& 0.02& 0.02& 0.03& 0.02& 0.03& 0.02& 0.02& 0.02& 0.01& 0.01& 0.01& 0.00& 1&\\
\scriptsize{2.00--4.00} &0.005& 0.004& 0.005& 0.006& 0.004& 0.005& 0.004& 0.004& 0.004& 0.002& 0.002& 0.002& 0.002& 0.001& 1\\ \hline

\label{tab:correlPhi}
      \end{tabular}
}
\end{sidewaystable}

\begin{sidewaystable}
 \caption{Correlation coefficients between differential cross-section 
measurements as a function of \PW boson muon $\eta$. The beam energy 
and luminosity 
uncertainties, which are fully correlated between cross-section measurements, are excluded.}
 \resizebox{25cm}{5cm}{
  \begin{tabular}{l l | c c c c c c c c c c c c c c c c | r}

 %&& \multicolumn{16}{c}{$\eta^{\mu}$} & \\
 &$\eta^{\mu}$& \multicolumn{2}{c}{\footnotesize{2--2.25}} & \multicolumn{2}{c}{\footnotesize{2.25--2.5}} & \multicolumn{2}{c}{\footnotesize{2.5--2.75}} & \multicolumn{2}{c}{\footnotesize{2.75--3}} & \multicolumn{2}{c}{\footnotesize{3--3.25}} &\multicolumn{2}{c}{\footnotesize{3.25--3.5}} & \multicolumn{2}{c}{\footnotesize{3.5--4}} & \multicolumn{2}{c}{\footnotesize{4--4.5}}  &  \\ \hline

%\multirow{16}{*}{\rotatebox[origin=c]{0}{$\eta^{\mu}$}}&\multirow{2}{*}{\rotatebox[origin=c]{0}{\scriptsize{2--2.25}}}&1& & & & & & & & & & & & & & & & $W^{+}$\\
&\multirow{2}{*}{\rotatebox[origin=c]{0}{\scriptsize{2--2.25}}}&1& & & & & & & & & & & & & & & & $W^{+}$\\
&&0.46& 1& & & & & & & & & & & & & & &  $W^{-}$\\ 
&\multirow{2}{*}{\rotatebox[origin=c]{0}{\scriptsize{2.25--2.5}}}&-0.15& 0.34& 1& & & & & & & & & & & & & & $W^{+}$\\
&&0.30& -0.24& 0.09& 1& & & & & & & & & & & & &  $W^{-}$\\ 
&\multirow{2}{*}{\rotatebox[origin=c]{0}{\scriptsize{2.5--2.75}}}&-0.03& 0.23& 0.27& -0.13& 1& & & & & & & & & & & & $W^{+}$\\
&&0.24& -0.14& -0.21& 0.35& 0.41& 1& & & & & & & & & & & $W^{-}$\\ 
&\multirow{2}{*}{\rotatebox[origin=c]{0}{\scriptsize{2.75--3}}}&0.20& -0.07& -0.10& 0.25& -0.00& 0.21& 1& & & & & & & & & & $W^{+}$\\
&&-0.19& 0.39& 0.46& -0.37& 0.27& -0.24& 0.28& 1& & & & & & & & & $W^{-}$\\ 
&\multirow{2}{*}{\rotatebox[origin=c]{0}{\scriptsize{3--3.25}}}&-0.03& 0.24& 0.28& -0.16& 0.20& -0.08& -0.01& 0.29& 1& & & & & & & & $W^{+}$\\
&&0.31& -0.23& -0.32& 0.46& -0.13& 0.35& 0.25& -0.37& 0.27& 1& & & & & & & $W^{-}$\\ 
&\multirow{2}{*}{\rotatebox[origin=c]{0}{\scriptsize{3.25--3.5}}}&-0.12& 0.29& 0.36& -0.27& 0.22& -0.17& -0.07& 0.40& 0.24& -0.27& 1& & & & & & $W^{+}$\\
&&0.33& -0.32& -0.41& 0.52& -0.19& 0.40& 0.28& -0.47& -0.21& 0.53& -0.07& 1& & & & & $W^{-}$\\ 
&\multirow{2}{*}{\rotatebox[origin=c]{0}{\scriptsize{3.5--4}}}&0.02& 0.15& 0.18& -0.05& 0.15& -0.01& 0.04& 0.17& 0.14& -0.04& 0.15& -0.08& 1& & & & $W^{+}$\\
&&0.21& -0.09& -0.14& 0.30& -0.02& 0.25& 0.19& -0.17& -0.04& 0.30& -0.12& 0.33& 0.45& 1& & & $W^{-}$\\ 
&\multirow{2}{*}{\rotatebox[origin=c]{0}{\scriptsize{4--4.5}}}&-0.01& 0.13& 0.17& -0.08& 0.14& -0.05& -0.01& 0.15& 0.11& -0.07& 0.11& -0.12& 0.09& 0.02& 1& & $W^{+}$\\
&&0.08& 0.01& -0.01& 0.09& 0.03& 0.08& 0.07& -0.02& 0.02& 0.10& -0.02& 0.09& 0.03& 0.10& 0.11& 1& $W^{-}$\\ \hline
&&$W^{+}$ & $W^{-}$ & $W^{+}$ & $W^{-}$ & $W^{+}$ & $W^{-}$ & $W^{+}$ & $W^{-}$ & $W^{+}$ & $W^{-}$ & $W^{+}$ & $W^{-}$ & $W^{+}$ & $W^{-}$ & $W^{+}$ & $W^{-}$ & \\

\label{tab:correlEta}
      \end{tabular}
}
\end{sidewaystable}

\begin{sidewaystable}
 \caption{Correlation coefficients between differential cross-section 
measurements as a function of $y_{Z}$ and \PW boson muon $\eta$. The \lhc 
beam energy and luminosity 
uncertainties, which are fully correlated between cross-section measurements, are excluded.}
 \resizebox{25cm}{4cm}{
  \begin{tabular}{l l | c c c c c c c c c c c c c c c c c c | r}

 && \multicolumn{18}{c}{$y_{\PZ}$} & \\
 && \scriptsize{2--2.125} & \scriptsize{2.125--2.25} & \scriptsize{2.25--2.375} & \scriptsize{2.375--2.5} & \scriptsize{2.5--2.625} & \scriptsize{2.625--2.75} & 
\scriptsize{2.75--2.875} & \scriptsize{2.875--3} & \scriptsize{3--3.125} &
\scriptsize{3.125--3.25} & \scriptsize{3.25--3.375} & \scriptsize{3.375--3.5} & \scriptsize{3.5--3.625} &
\scriptsize{3.625--3.75} &
\scriptsize{3.75--3.875} & \scriptsize{3.875--4} & \scriptsize{4--4.25}  & \scriptsize{4.25--4.5} &  \\ \hline


\multirow{16}{*}{\rotatebox[origin=c]{0}{$\eta^{\mu}$}}&\multirow{2}{*}{\rotatebox[origin=c]{0}{\scriptsize{2--2.25}}}&0.24& 0.25& 0.19& 0.19& 0.17& 0.16& 0.15& 0.13& 0.12& 0.10& 0.08& 0.06& 0.05& 0.04& 0.03& 0.02& 0.01& $-$& $W^{+}$\\
&&0.22& 0.23& 0.17& 0.17& 0.16& 0.15& 0.13& 0.12& 0.11& 0.09& 0.07& 0.05& 0.04& 0.04& 0.03& 0.02& 0.01& $-$& $W^{-}$\\ 
&\multirow{2}{*}{\rotatebox[origin=c]{0}{\scriptsize{2.25--2.5}}}&0.03& 0.11& 0.13& 0.14& 0.12& 0.11& 0.10& 0.10& 0.09& 0.07& 0.06& 0.04& 0.03& 0.02& 0.01& 0.01& 0.01& $-$& $W^{+}$\\
&&0.03& 0.10& 0.12& 0.13& 0.11& 0.10& 0.10& 0.09& 0.08& 0.07& 0.06& 0.04& 0.03& 0.02& 0.01& 0.01& 0.00& $-$& $W^{-}$\\ 
&\multirow{2}{*}{\rotatebox[origin=c]{0}{\scriptsize{2.5--2.75}}}&0.03& 0.04& 0.06& 0.10& 0.10& 0.10& 0.09& 0.09& 0.08& 0.07& 0.07& 0.05& 0.04& 0.03& 0.02& 0.01& 0.01& $-$& $W^{+}$\\
&&0.03& 0.03& 0.06& 0.10& 0.09& 0.09& 0.08& 0.08& 0.08& 0.07& 0.06& 0.05& 0.04& 0.02& 0.02& 0.01& 0.01& $-$& $W^{-}$\\ 
&\multirow{2}{*}{\rotatebox[origin=c]{0}{\scriptsize{2.75--3}}}&0.03& 0.04& 0.04& 0.07& 0.09& 0.10& 0.09& 0.09& 0.09& 0.08& 0.07& 0.06& 0.05& 0.04& 0.02& 0.01& 0.01& $-$& $W^{+}$\\
&&0.02& 0.03& 0.03& 0.05& 0.07& 0.07& 0.07& 0.07& 0.06& 0.06& 0.05& 0.04& 0.04& 0.03& 0.01& 0.01& 0.01& $-$& $W^{-}$\\ 
&\multirow{2}{*}{\rotatebox[origin=c]{0}{\scriptsize{3--3.25}}}&0.04& 0.04& 0.04& 0.06& 0.08& 0.10& 0.10& 0.10& 0.09& 0.09& 0.08& 0.07& 0.06& 0.05& 0.03& 0.01& 0.01& $-$& $W^{+}$\\
&&0.03& 0.04& 0.03& 0.05& 0.06& 0.08& 0.08& 0.08& 0.08& 0.07& 0.07& 0.06& 0.05& 0.04& 0.02& 0.01& 0.01& $-$& $W^{-}$\\ 
&\multirow{2}{*}{\rotatebox[origin=c]{0}{\scriptsize{3.25--3.5}}}&0.02& 0.03& 0.03& 0.04& 0.04& 0.05& 0.06& 0.06& 0.06& 0.06& 0.05& 0.05& 0.04& 0.03& 0.02& 0.01& 0.01& $-$& $W^{+}$\\
&&0.02& 0.02& 0.02& 0.03& 0.03& 0.04& 0.05& 0.05& 0.05& 0.04& 0.04& 0.03& 0.03& 0.02& 0.02& 0.01& 0.00& $-$& $W^{-}$\\ 
&\multirow{2}{*}{\rotatebox[origin=c]{0}{\scriptsize{3.5--4}}}&0.03& 0.03& 0.03& 0.04& 0.04& 0.05& 0.06& 0.08& 0.09& 0.08& 0.08& 0.07& 0.07& 0.05& 0.04& 0.03& 0.02& $-$& $W^{+}$\\
&&0.03& 0.03& 0.03& 0.04& 0.04& 0.05& 0.06& 0.08& 0.09& 0.09& 0.08& 0.07& 0.07& 0.05& 0.04& 0.03& 0.02& $-$& $W^{-}$\\ 
&\multirow{2}{*}{\rotatebox[origin=c]{0}{\scriptsize{4--4.5}}}&0.02& 0.02& 0.02& 0.02& 0.02& 0.02& 0.02& 0.02& 0.03& 0.04& 0.05& 0.05& 0.06& 0.06& 0.04& 0.03& 0.03& $-$& $W^{+}$\\
&&0.02& 0.02& 0.02& 0.03& 0.03& 0.03& 0.03& 0.03& 0.04& 0.05& 0.07& 0.07& 0.07& 0.07& 0.05& 0.04& 0.03& $-$& $W^{-}$\\ \hline


\hline

\label{tab:correlWZ}
      \end{tabular}
}
\end{sidewaystable}

\clearpage


detector.tex
\section{Detector and data set}
\label{sec:Detector}

The \lhcb detector~\cite{Alves:2008zz,LHCb-DP-2014-002} is a single-arm forward
spectrometer covering the \mbox{pseudorapidity} range $2<\eta <5$,
designed for the study of particles containing \bquark or \cquark
quarks. The detector includes a high-precision tracking system
consisting of a silicon-strip vertex detector surrounding the $pp$
interaction region~\cite{LHCb-DP-2014-001}, a large-area silicon-strip detector located
upstream of a dipole magnet with a bending power of about
$4{\rm\,Tm}$, and three stations of silicon-strip detectors and straw
drift tubes~\cite{LHCb-DP-2013-003} placed downstream of the magnet.
The tracking system provides a measurement of momentum, \ptot, of charged particles with
a relative uncertainty that varies from 0.5\% at low momentum to 1.0\% at 200\gevc.
The minimum distance of a track to a primary vertex, the impact parameter, is measured with a resolution of $(15+29/\pt)\mum$,
where \pt is the component of the momentum transverse to the beam, in \gevc.
Different types of charged hadrons are distinguished using information
from two ring-imaging Cherenkov detectors~\cite{LHCb-DP-2012-003}.
Photons, electrons and hadrons are identified by a calorimeter system consisting of a
scintillating-pad detector (SPD), preshower detectors, an electromagnetic
calorimeter and a hadronic calorimeter. Muons are identified by a
system composed of alternating layers of iron and multiwire
proportional chambers~\cite{LHCb-DP-2012-002}.
The online event selection is performed by a trigger~\cite{LHCb-DP-2012-004},
which consists of a hardware stage, based on information from the calorimeter and muon
systems, followed by a software stage, which applies a full event 
reconstruction. A requirement that prevents events with high
occupancy from dominating the processing time of the software trigger is 
also applied.
This is referred to as the global event cut (GEC) in this article.

The measurement presented here is based on $pp$ collision data collected at a centre-of-mass energy of 7 \tev. 
The integrated luminosity amounts to 975 $\pm$ 17 pb$^{-1}$.
The absolute luminosity scale was measured during dedicated data taking periods,
using both Van der Meer scans~\cite{vandermeer} 
and beam-gas imaging methods~\cite{beamgas}. Both
methods give similar results, which are combined to give the final luminosity estimate with an uncertainty of 
$1.7\%$~\cite{lumi2}. 
This analysis uses the same data set as in Ref.~\cite{wmu}.

Several samples of simulated data are produced to estimate contributions from background processes, to cross-check efficiencies and to unfold data
for detector-related effects. The \pythia generator~\cite{pythia,pythia8}, configured as in Ref.~\cite{gauss}
with the CTEQ6L1~\cite{cteq,cteq1} parameterisation for the PDFs, is used to simulate $b\bar{b}$, $c\bar{c}$, $WW$, $t\bar{t}$ 
and \PZ production. All generated events are passed
through a detector simulation based on \geant~\cite{geant}, followed by 
\lhcb-specific trigger emulation and event 
reconstruction.
 
The results of the analysis are compared to theoretical predictions calculated with the \fewz~\cite{fewz,fewzold} generator at NNLO for the 
PDF sets ABM12~\cite{abm12},
CT10~\cite{ct10}, HERA1.5~\cite{h1zeus}, JR09~\cite{jr09}, MSTW08~\cite{mstw08}, and NNPDF3.0~\cite{PDF-NNPDF30}. 
Comparisons are also made to the \resbos~\cite{resbos1,resbos2,resbos3} and \powheg~\cite{powheg} generators 
configured with the CT10 PDF set. \resbos includes 
an approximate NNLO calculation, plus a next-to-next-to-leading logarithm approximation for the resummation of the soft gluon radiation.
\powheg provides a next-to-leading order (NLO) calculation interfaced to a parton shower, in this case performed by \herwig~\cite{GEN-HERWIG1,GEN-HERWIG2}.
The results are also compared to the predictions from \mc@nlo ~\cite{mcnlo1,mcnlo2}, which is interfaced 
with different generators to simulate 
the parton shower. Parton showering is performed using 
\herwig~\cite{GEN-HERWIG1,GEN-HERWIG2}, with different values for the root 
mean-square-deviation  of the intrinsic $k_{T}$, 
and \herwiri~\cite{herwiri1,herwiri2,herwiri3}, which is based on infrared-improved~\cite{IRimp1} DGLAP-CS~\cite{dglap1,dglap2,dglap3,dglap4,cs1,cs2} 
theory. All calculations are performed with the renormalisation and factorisation scales set to the electroweak boson mass. 
Scale uncertainties are estimated by varying these scales by factors of two around the boson 
mass~\cite{scaleUnc}.
Total uncertainties 
correspond to the PDF and $\alpha_{s}$ uncertainties at 68.3$\%$ confidence 
level and scale uncertainties, added in quadrature.


figures.tex
% $Id: figures.tex 61168 2014-09-25 23:10:50Z roldeman $
% ===============================================================================
% Purpose: including figures in the standard template
% Author: Tomasz Skwarnicki, Ulrik Egede
% Created on: 2010-09-24
% ===============================================================================

\section{Figures}
\label{sec:Figures}

A standard \lhcb style file for use in production of figures in \root
is in the \urania package \texttt{RootTools/LHCbStyle} or directly in
\svn at
\texttt{svn+ssh://svn.cern.ch/reps/lhcb/Urania/trunk/RootTools/LHCbStyle}. It
is not mandatory to use this style, but it makes it easier to follow
the recommendations below.

Figure~\ref{fig:example} shows an example of how to include an eps
or pdf figure with the \texttt{\textbackslash includegraphics} command
(eps figures will not work with \texttt{pdflatex}). Note that if the
graphics sits in \texttt{figs/myfig.pdf}, you can just write
\texttt{\textbackslash includegraphics\{myfig\}} as the \texttt{figs}
subdirectory is searched automatically and the extension \texttt{.pdf}
(\texttt{.eps}) is automatically added for \texttt{pdflatex}
(\texttt{latex}).
\begin{figure}[tb]
  \begin{center}
    \includegraphics[width=0.49\linewidth]{Example1DPlot-python-1}\put(-32,133){(a)}
    \includegraphics[width=0.49\linewidth]{Example1DPlot-python-1_sim}\put(-32,133){(b)}
    \vspace*{-1.0cm}
  \end{center}
  \caption{
    %\small %captions should be a little bit smaller than main text
    Example plots for (a) data and (b) simulation using the \lhcb style from the \urania package
    \texttt{RootTools/LHCbStyle}. The signal data is shown as points
    with the signal component as yellow (light shaded), background 1 as green
    (medium shaded) and background 2 as blue (dark shaded).}
  \label{fig:example}
\end{figure}

\begin{enumerate}

\item Figures should be legible at the size they will appear in the
  publication, with suitable line width.  Their axes should be
  labelled, and have suitable units (e.g. avoid a mass plot with
  labels in \mevcc if the region of interest covers a few \gevcc
  and all the numbers then run together).  Spurious background shading
  and boxes around text should be avoided.

\item For the $y$-axis, ``Entries'' or ``Candidates'' is approriate in case no
background subtraction has been applied. Otherwise ``Yield'' or ``Decays''
may be more appropriate. If the unit on the $y$-axis corresponds to 
the yield per bin, indicate so, for example ``Entries / ( 5\mevcc )'' or ``Entries per 5\mevcc''.


\item Fit curves should not obscure the data points, and
   data points are best (re)drawn over the fit curves.

\item Colour may be used in figures, but the distinction between
  differently coloured areas or lines should be clear also when the
  document is printed in black and white, for example through
  differently dashed lines. The \lhcb style mentioned above implements
  a colour scheme that works well but individual adjustments might be
  required.

\item Using different hatching styles helps to disinguished filled areas, 
also in black and white prints. Hatching styles 3001-3025 should be
avoided since they behave unpredictably under zooming and scaling. 
Good styles for ``falling hatched'' and ``rising hatched'' are 3345 and 3354.


\item Figures with more than one part should have the parts labelled
  (a), (b) \etc, with a corresponding description in the caption;
  alternatively they should be clearly referred to by their position,
  e.g. Fig.~1\,(left). In the caption, the labels (a), (b) \etc should
  precede their description. When referencing specific sub-figures,
  use ``see Fig. 1(a)'' or ``see Figs. 2(b)-(e)''.

\item All figures containing \lhcb data should have \lhcb written on
  them. For preliminary
  results, that should be replaced by ``LHCb preliminary''.
  Figures that only have simulated data should display ``LHCb simulation''.
  Figures that do not depend on LHCb-specific software (\eg only on \pythia)
  should not have any label.


\end{enumerate}

introduction.tex
% $Id: introduction.tex 72974 2015-05-26 13:38:50Z rwallace $

\section{Introduction}
\label{sec:Introduction}

Measurements of the total and differential cross-sections for the production of \PZ 
bosons
in $pp$ collisions test the Standard Model (SM) and 
provide constraints on parton density functions (PDFs) of the proton.\footnote{Throughout this article \PZ represents both 
resonant production of \PZ bosons and off-mass-shell photons.}
Theoretical predictions for these cross-sections are available at 
next-to-next-to-leading order (NNLO) 
in perturbative quantum chromodynamics (pQCD)~\cite{nnlopQCD1,nnlopQCD2,nnlopQCD3,nnlopQCD4,nnlopQCD5}. The dominant uncertainty on these predictions 
reflects the uncertainties on the PDFs, 
which vary as functions of the kinematic variables studied. 
The forward acceptance of the \lhcb detector allows the PDFs to be 
constrained at Bjorken-$x$ values down to 10$^{-4}$~\cite{LHCbPDF}.
Ratios of the \PW and \PZ cross-sections provide precise tests of the SM as the sensitivity to the PDFs in the theoretical calculations is reduced 
and many of the experimental uncertainties cancel.

\lhcb has measured the \PZ boson production cross-section at $\sqrt{s}$= 7 \tev using decays to muon pairs in a data set 
corresponding to
37 pb$^{-1}$~\cite{lhcbwz}, and using electron~\cite{ze} and tau lepton~\cite{ztau} pairs in a data set of 1.0 fb$^{-1}$. 
Production cross-sections of \PW bosons and the $W^{+}$/$W^{-}$ cross-section ratio
have been measured in the muon channel~\cite{wmu} with the  $1.0\nolinebreak\text{ fb}^{-1}$ data set. Similar measurements 
have also been performed by the \atlas~\cite{atlaswz} 
and \cms~\cite{cmswz} collaborations.

The analysis described here is an update of the one described in Ref.~\cite{lhcbwz}, 
using a total integrated luminosity of about 1.0 fb$^{-1}$. 
This increases statistical precision and allows better control of systematic 
uncertainties, with the result that the 
total uncertainties on the measurements are 
significantly reduced.
Measurements are performed for muons with transverse momentum 
$\pt > 20\gevc$ and pseudorapidity in the range $2.0 < \eta < 4.5$. In the case of 
\PZ boson measurements, the invariant 
mass of the two muons is required to be in the range $60 < M_{\mu^{+}\mu^{-}} < 120\gevcc$. 
These kinematic requirements define the fiducial region of the measurement and 
in this article are referred to as the fiducial requirements. 
Total cross-sections are presented as well as differential 
cross-sections as functions of the \PZ boson 
rapidity $y_{Z}$, $p_{T,Z}$ and $\phi^{*}_{Z}$. Here 
$\phi^{*}_{Z}$ is defined as~\cite{phistar}
\begin{equation}
 \phi^{*}_{Z} \equiv \frac{\tan{(\phi_{\rm acop}/2)}}{\cosh{(\Delta\eta}/2)}.
\end{equation}
The angle $\phi_{\rm acop} = \pi - |\Delta\phi|$ depends on the  
difference $\Delta\phi$ in azimuthal angle between the two muon momenta, 
while the difference between their pseudorapidities is denoted by $\Delta\eta$.

The \PW boson cross-sections given in Ref.~\cite{wmu} are re-evaluated using a more precise 
determination of the event trigger efficiency. The cross-sections are presented as a function of the $\eta$ of 
the muon from the \PW boson decay. The values presented here supersede those of Ref.~\cite{wmu}. 

This paper is organised as follows:
Section~\ref{sec:Detector} describes the \lhcb detector;
Sections~\ref{sec:selection} and~\ref{sec:cs} detail the selection of \PZ boson candidates,
the \PZ boson cross-section definition and relevant sources of systematic uncertainty;
Section~\ref{sec:results} presents the results
and Section~\ref{sec:conclusions} concludes the paper.
Appendices~\ref{sec:difftab} and~\ref{sec:correlation} provide tables of differential cross-sections and 
correlations between these measurements.


layout.tex
\section{Layout}

\begin{enumerate}

\item Unnecessary blank space should be avoided, between paragraphs or
  around figures and tables.

\item Figure and table captions should be concise and use a somewhat smaller typeface
  than the main text, to help distinguish them. This is achieved by 
  inserting \verb!\small! at the beginning of the caption.
  (NB with the latest version of the file \verb!premable.tex! this is automatic)
  Figure captions go below the figure, table captions go above the
  table.

\item Captions and footnotes should be punctuated correctly, like
  normal text. The use of too many footnotes should be avoided:
  typically they are used for giving commercial details of companies,
  or standard items like coordinate system definition or the implicit
  inclusion of charge-conjugate processes.\footnote{If placed at the end
    of a sentence, the footnote symbol normally follows the
    punctuation; if placed in the middle of an equation, take care to
    avoid any possible confusion with an index.}$^,$\footnote{The standard footnote reads: The inclusion of charge-conjugate processes is implied.}

\item Tables should be formatted in a simple fashion, without
  excessive use of horizontal and vertical lines. See
  Table~\ref{tab:example} for an example.

\item Figures and tables should normally be placed so that they appear
  on the same page as their first reference, but at the top or bottom
  of the page; if this is not possible, they should come as soon as
  possible afterwards.  They must all be referred to from the text.

\item If one or more equations are referenced, all equations should be numbered using parentheses as shown in
  Eq.~\ref{eq:CKM},
  \begin{equation}
    \label{eq:CKM}
    V_{\uquark\squark}V_{\uquark\bquark}^* + 
    V_{\cquark\squark}V_{\cquark\bquark}^* + 
    V_{\tquark\squark}V_{\tquark\bquark}^* = 0 \ . 
  \end{equation}
  
\item Displayed results like
  \begin{equation*}
    \BF(\decay{\Bs}{\mumu}) < 1.5 \times 10^{-8} \text{ at 95\% CL}
  \end{equation*}
  should in general not be numbered.

\item Numbered equations should be avoided in captions and footnotes.

\item Displayed equations are part of the normal grammar of the
  text. This means that the equation should end in full stop or comma if
  required when reading aloud. The line after the equation should only
  be indented if it starts a new paragraph.

\item Sub-sectioning should not be excessive: sections with more than three
levels of index (1.1.1) should be avoided.

%\item It is generally preferable to itemize a list using numbers rather
%than bullets.

\item Acronyms should be defined the first time they are used,
  \eg ``Monte Carlo~(MC) events containing a doubly
  Cabibbo-suppressed~(DCS) decay have been generated.''
  The abbreviated words should not be capitalised if it is not naturally
  written with capitals, \eg quantum chromodynamics (QCD),
  impact parameter (IP), boosted decision tree (BDT).
  Avoid acronyms if they are used three times or less.
  A sentence should never start with an acronym and its better to
  avoid it as the last word of a sentence as well.

\end{enumerate}

\begin{table}[t]
  \caption{
    %\small %captions should be a little bit smaller than main text
    Background-to-signal ratio estimated in a $\pm 50\mevcc$ 
    mass window for the prompt and long-lived backgrounds, and the 
    minimum bias rate.}
\begin{center}\begin{tabular}{lccc}
    \hline
    Channel                           & $B_{\rm pr}/S$ & $B_{\rm LL}/S$   & MB rate       \\ 
    \hline
    \BsToJPsiPhi              & $ 1.6 \pm 0.6$ & $ 0.51 \pm 0.08$ & $\sim 0.3$ Hz \\
    \BdToJPsiKst              & $ 5.2 \pm 0.3$ & $1.53 \pm 0.08 $ & $\sim 8.1$ Hz \\
    \decay{\Bp}{\jpsi\Kstarp} & $ 1.6 \pm 0.2$ & $0.29 \pm 0.06$  & $\sim 1.4$ Hz \\
    \hline
  \end{tabular}\end{center}
\label{tab:example}
\end{table}

% old table with vertical lines
%\begin{table}[t]
%  \caption{
%    \small %captions should be a little bit smaller than main text
%    Background-to-signal ratio estimated in a $\pm 50\mevcc$ 
%    mass window for the prompt and long-lived backgrounds, and the 
%    minimum bias rate.}
%\begin{center}\begin{tabular}{l|c|c|c}
%    Channel                           & $B_{\rm pr}/S$ & $B_{\rm LL}/S$   & MB rate       \\ 
%    \hline
%    \BsToJPsiPhi              & $ 1.6 \pm 0.6$ & $ 0.51 \pm 0.08$ & $\sim 0.3$ Hz \\
%    \BdToJPsiKst              & $ 5.2 \pm 0.3$ & $1.53 \pm 0.08 $ & $\sim 8.1$ Hz \\
%    \decay{\Bp}{\jpsi\Kstarp} & $ 1.6 \pm 0.2$ & $0.29 \pm 0.06$  & $\sim 1.4$ Hz \\
%  \end{tabular}\end{center}
%\label{tab:example}
%\end{table}

LHCb_authorlist.tex
% $Id: LHCb_authorlist.tex 18784 2012-04-30 14:45:53Z uegede $
% ===============================================================================
% Purpose: example of authorlist for LHCb template
% Author:
% Created on: 2009-09-24
% ===============================================================================

%\documentclass[a4paper]{article}
%\setlength{\oddsidemargin}{0cm}
%\setlength{\evensidemargin}{0cm}
%\setlength{\textwidth}{16.5cm}
%\setlength{\parindent}{0cm}
%\begin{document}
\centerline{\large\bf LHCb collaboration}
\begin{flushleft}
\small
%-- LHCb Authorlist, Example typesetting
%-- 
A.~N.~Other$^{1}$.\bigskip\newline{\it
\footnotesize
$ ^{1}$University of nowhere\\
}
%-- 
%-- 
\end{flushleft}
%\end{document}

LHCb_HD_authorlist_2015-01-13.tex
%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
\centerline{\large\bf LHCb collaboration}
\begin{flushleft}
\small
R.~Aaij$^{38}$, 
B.~Adeva$^{37}$, 
M.~Adinolfi$^{46}$, 
A.~Affolder$^{52}$, 
Z.~Ajaltouni$^{5}$, 
S.~Akar$^{6}$, 
J.~Albrecht$^{9}$, 
F.~Alessio$^{38}$, 
M.~Alexander$^{51}$, 
S.~Ali$^{41}$, 
G.~Alkhazov$^{30}$, 
P.~Alvarez~Cartelle$^{53}$, 
A.A.~Alves~Jr$^{57}$, 
S.~Amato$^{2}$, 
S.~Amerio$^{22}$, 
Y.~Amhis$^{7}$, 
L.~An$^{3}$, 
L.~Anderlini$^{17,g}$, 
J.~Anderson$^{40}$, 
M.~Andreotti$^{16,f}$, 
J.E.~Andrews$^{58}$, 
R.B.~Appleby$^{54}$, 
O.~Aquines~Gutierrez$^{10}$, 
F.~Archilli$^{38}$, 
P.~d'Argent$^{11}$, 
A.~Artamonov$^{35}$, 
M.~Artuso$^{59}$, 
E.~Aslanides$^{6}$, 
G.~Auriemma$^{25,n}$, 
M.~Baalouch$^{5}$, 
S.~Bachmann$^{11}$, 
J.J.~Back$^{48}$, 
A.~Badalov$^{36}$, 
C.~Baesso$^{60}$, 
W.~Baldini$^{16,38}$, 
R.J.~Barlow$^{54}$, 
C.~Barschel$^{38}$, 
S.~Barsuk$^{7}$, 
W.~Barter$^{38}$, 
V.~Batozskaya$^{28}$, 
V.~Battista$^{39}$, 
A.~Bay$^{39}$, 
L.~Beaucourt$^{4}$, 
J.~Beddow$^{51}$, 
F.~Bedeschi$^{23}$, 
I.~Bediaga$^{1}$, 
L.J.~Bel$^{41}$, 
I.~Belyaev$^{31}$, 
E.~Ben-Haim$^{8}$, 
G.~Bencivenni$^{18}$, 
S.~Benson$^{38}$, 
J.~Benton$^{46}$, 
A.~Berezhnoy$^{32}$, 
R.~Bernet$^{40}$, 
A.~Bertolin$^{22}$, 
M.-O.~Bettler$^{38}$, 
M.~van~Beuzekom$^{41}$, 
A.~Bien$^{11}$, 
S.~Bifani$^{45}$, 
T.~Bird$^{54}$, 
A.~Birnkraut$^{9}$, 
A.~Bizzeti$^{17,i}$, 
T.~Blake$^{48}$, 
F.~Blanc$^{39}$, 
J.~Blouw$^{10}$, 
S.~Blusk$^{59}$, 
V.~Bocci$^{25}$, 
A.~Bondar$^{34}$, 
N.~Bondar$^{30,38}$, 
W.~Bonivento$^{15}$, 
S.~Borghi$^{54}$, 
A.~Borgia$^{59}$, 
M.~Borsato$^{7}$, 
T.J.V.~Bowcock$^{52}$, 
E.~Bowen$^{40}$, 
C.~Bozzi$^{16}$, 
D.~Brett$^{54}$, 
M.~Britsch$^{10}$, 
T.~Britton$^{59}$, 
J.~Brodzicka$^{54}$, 
N.H.~Brook$^{46}$, 
A.~Bursche$^{40}$, 
J.~Buytaert$^{38}$, 
S.~Cadeddu$^{15}$, 
R.~Calabrese$^{16,f}$, 
M.~Calvi$^{20,k}$, 
M.~Calvo~Gomez$^{36,p}$, 
P.~Campana$^{18}$, 
D.~Campora~Perez$^{38}$, 
L.~Capriotti$^{54}$, 
A.~Carbone$^{14,d}$, 
G.~Carboni$^{24,l}$, 
R.~Cardinale$^{19,j}$, 
A.~Cardini$^{15}$, 
P.~Carniti$^{20}$, 
L.~Carson$^{50}$, 
K.~Carvalho~Akiba$^{2,38}$, 
R.~Casanova~Mohr$^{36}$, 
G.~Casse$^{52}$, 
L.~Cassina$^{20,k}$, 
L.~Castillo~Garcia$^{38}$, 
M.~Cattaneo$^{38}$, 
Ch.~Cauet$^{9}$, 
G.~Cavallero$^{19}$, 
R.~Cenci$^{23,t}$, 
M.~Charles$^{8}$, 
Ph.~Charpentier$^{38}$, 
M.~Chefdeville$^{4}$, 
S.~Chen$^{54}$, 
S.-F.~Cheung$^{55}$, 
N.~Chiapolini$^{40}$, 
M.~Chrzaszcz$^{40,26}$, 
X.~Cid~Vidal$^{38}$, 
G.~Ciezarek$^{41}$, 
P.E.L.~Clarke$^{50}$, 
M.~Clemencic$^{38}$, 
H.V.~Cliff$^{47}$, 
J.~Closier$^{38}$, 
V.~Coco$^{38}$, 
J.~Cogan$^{6}$, 
E.~Cogneras$^{5}$, 
V.~Cogoni$^{15,e}$, 
L.~Cojocariu$^{29}$, 
G.~Collazuol$^{22}$, 
P.~Collins$^{38}$, 
A.~Comerma-Montells$^{11}$, 
A.~Contu$^{15,38}$, 
A.~Cook$^{46}$, 
M.~Coombes$^{46}$, 
S.~Coquereau$^{8}$, 
G.~Corti$^{38}$, 
M.~Corvo$^{16,f}$, 
I.~Counts$^{56}$, 
B.~Couturier$^{38}$, 
G.A.~Cowan$^{50}$, 
D.C.~Craik$^{48}$, 
A.~Crocombe$^{48}$, 
M.~Cruz~Torres$^{60}$, 
S.~Cunliffe$^{53}$, 
R.~Currie$^{53}$, 
C.~D'Ambrosio$^{38}$, 
J.~Dalseno$^{46}$, 
P.N.Y.~David$^{41}$, 
A.~Davis$^{57}$, 
K.~De~Bruyn$^{41}$, 
S.~De~Capua$^{54}$, 
M.~De~Cian$^{11}$, 
J.M.~De~Miranda$^{1}$, 
L.~De~Paula$^{2}$, 
W.~De~Silva$^{57}$, 
P.~De~Simone$^{18}$, 
C.-T.~Dean$^{51}$, 
D.~Decamp$^{4}$, 
M.~Deckenhoff$^{9}$, 
L.~Del~Buono$^{8}$, 
N.~D\'{e}l\'{e}age$^{4}$, 
D.~Derkach$^{55}$, 
O.~Deschamps$^{5}$, 
F.~Dettori$^{38}$, 
B.~Dey$^{40}$, 
A.~Di~Canto$^{38}$, 
F.~Di~Ruscio$^{24}$, 
H.~Dijkstra$^{38}$, 
S.~Donleavy$^{52}$, 
F.~Dordei$^{11}$, 
M.~Dorigo$^{39}$, 
A.~Dosil~Su\'{a}rez$^{37}$, 
D.~Dossett$^{48}$, 
A.~Dovbnya$^{43}$, 
K.~Dreimanis$^{52}$, 
G.~Dujany$^{54}$, 
F.~Dupertuis$^{39}$, 
P.~Durante$^{38}$, 
R.~Dzhelyadin$^{35}$, 
A.~Dziurda$^{26}$, 
A.~Dzyuba$^{30}$, 
S.~Easo$^{49,38}$, 
U.~Egede$^{53}$, 
V.~Egorychev$^{31}$, 
S.~Eidelman$^{34}$, 
S.~Eisenhardt$^{50}$, 
U.~Eitschberger$^{9}$, 
R.~Ekelhof$^{9}$, 
L.~Eklund$^{51}$, 
I.~El~Rifai$^{5}$, 
Ch.~Elsasser$^{40}$, 
S.~Ely$^{59}$, 
S.~Esen$^{11}$, 
H.M.~Evans$^{47}$, 
T.~Evans$^{55}$, 
A.~Falabella$^{14}$, 
C.~F\"{a}rber$^{11}$, 
C.~Farinelli$^{41}$, 
N.~Farley$^{45}$, 
S.~Farry$^{52}$, 
R.~Fay$^{52}$, 
D.~Ferguson$^{50}$, 
V.~Fernandez~Albor$^{37}$, 
F.~Ferrari$^{14}$, 
F.~Ferreira~Rodrigues$^{1}$, 
M.~Ferro-Luzzi$^{38}$, 
S.~Filippov$^{33}$, 
M.~Fiore$^{16,38,f}$, 
M.~Fiorini$^{16,f}$, 
M.~Firlej$^{27}$, 
C.~Fitzpatrick$^{39}$, 
T.~Fiutowski$^{27}$, 
P.~Fol$^{53}$, 
M.~Fontana$^{10}$, 
F.~Fontanelli$^{19,j}$, 
R.~Forty$^{38}$, 
O.~Francisco$^{2}$, 
M.~Frank$^{38}$, 
C.~Frei$^{38}$, 
M.~Frosini$^{17}$, 
J.~Fu$^{21,38}$, 
E.~Furfaro$^{24,l}$, 
A.~Gallas~Torreira$^{37}$, 
D.~Galli$^{14,d}$, 
S.~Gallorini$^{22,38}$, 
S.~Gambetta$^{19,j}$, 
M.~Gandelman$^{2}$, 
P.~Gandini$^{59}$, 
Y.~Gao$^{3}$, 
J.~Garc\'{i}a~Pardi\~{n}as$^{37}$, 
J.~Garofoli$^{59}$, 
J.~Garra~Tico$^{47}$, 
L.~Garrido$^{36}$, 
D.~Gascon$^{36}$, 
C.~Gaspar$^{38}$, 
U.~Gastaldi$^{16}$, 
R.~Gauld$^{55}$, 
L.~Gavardi$^{9}$, 
G.~Gazzoni$^{5}$, 
A.~Geraci$^{21,v}$, 
D.~Gerick$^{11}$, 
E.~Gersabeck$^{11}$, 
M.~Gersabeck$^{54}$, 
T.~Gershon$^{48}$, 
Ph.~Ghez$^{4}$, 
A.~Gianelle$^{22}$, 
S.~Gian\`{i}$^{39}$, 
V.~Gibson$^{47}$, 
L.~Giubega$^{29}$, 
V.V.~Gligorov$^{38}$, 
C.~G\"{o}bel$^{60}$, 
D.~Golubkov$^{31}$, 
A.~Golutvin$^{53,31,38}$, 
A.~Gomes$^{1,a}$, 
C.~Gotti$^{20,k}$, 
M.~Grabalosa~G\'{a}ndara$^{5}$, 
R.~Graciani~Diaz$^{36}$, 
L.A.~Granado~Cardoso$^{38}$, 
E.~Graug\'{e}s$^{36}$, 
E.~Graverini$^{40}$, 
G.~Graziani$^{17}$, 
A.~Grecu$^{29}$, 
E.~Greening$^{55}$, 
S.~Gregson$^{47}$, 
P.~Griffith$^{45}$, 
L.~Grillo$^{11}$, 
O.~Gr\"{u}nberg$^{63}$, 
B.~Gui$^{59}$, 
E.~Gushchin$^{33}$, 
Yu.~Guz$^{35,38}$, 
T.~Gys$^{38}$, 
C.~Hadjivasiliou$^{59}$, 
G.~Haefeli$^{39}$, 
C.~Haen$^{38}$, 
S.C.~Haines$^{47}$, 
S.~Hall$^{53}$, 
B.~Hamilton$^{58}$, 
T.~Hampson$^{46}$, 
X.~Han$^{11}$, 
S.~Hansmann-Menzemer$^{11}$, 
N.~Harnew$^{55}$, 
S.T.~Harnew$^{46}$, 
J.~Harrison$^{54}$, 
J.~He$^{38}$, 
T.~Head$^{39}$, 
V.~Heijne$^{41}$, 
K.~Hennessy$^{52}$, 
P.~Henrard$^{5}$, 
L.~Henry$^{8}$, 
J.A.~Hernando~Morata$^{37}$, 
E.~van~Herwijnen$^{38}$, 
M.~He\ss$^{63}$, 
A.~Hicheur$^{2}$, 
D.~Hill$^{55}$, 
M.~Hoballah$^{5}$, 
C.~Hombach$^{54}$, 
W.~Hulsbergen$^{41}$, 
T.~Humair$^{53}$, 
N.~Hussain$^{55}$, 
D.~Hutchcroft$^{52}$, 
D.~Hynds$^{51}$, 
M.~Idzik$^{27}$, 
P.~Ilten$^{56}$, 
R.~Jacobsson$^{38}$, 
A.~Jaeger$^{11}$, 
J.~Jalocha$^{55}$, 
E.~Jans$^{41}$, 
A.~Jawahery$^{58}$, 
F.~Jing$^{3}$, 
M.~John$^{55}$, 
D.~Johnson$^{38}$, 
C.R.~Jones$^{47}$, 
C.~Joram$^{38}$, 
B.~Jost$^{38}$, 
N.~Jurik$^{59}$, 
S.~Kandybei$^{43}$, 
W.~Kanso$^{6}$, 
M.~Karacson$^{38}$, 
T.M.~Karbach$^{38,\dagger}$,
S.~Karodia$^{51}$, 
M.~Kelsey$^{59}$, 
I.R.~Kenyon$^{45}$, 
M.~Kenzie$^{38}$, 
T.~Ketel$^{42}$, 
B.~Khanji$^{20,38,k}$, 
C.~Khurewathanakul$^{39}$, 
S.~Klaver$^{54}$, 
K.~Klimaszewski$^{28}$, 
O.~Kochebina$^{7}$, 
M.~Kolpin$^{11}$, 
I.~Komarov$^{39}$, 
R.F.~Koopman$^{42}$, 
P.~Koppenburg$^{41,38}$, 
M.~Korolev$^{32}$, 
L.~Kravchuk$^{33}$, 
K.~Kreplin$^{11}$, 
M.~Kreps$^{48}$, 
G.~Krocker$^{11}$, 
P.~Krokovny$^{34}$, 
F.~Kruse$^{9}$, 
W.~Kucewicz$^{26,o}$, 
M.~Kucharczyk$^{26}$, 
V.~Kudryavtsev$^{34}$, 
K.~Kurek$^{28}$, 
T.~Kvaratskheliya$^{31}$, 
V.N.~La~Thi$^{39}$, 
D.~Lacarrere$^{38}$, 
G.~Lafferty$^{54}$, 
A.~Lai$^{15}$, 
D.~Lambert$^{50}$, 
R.W.~Lambert$^{42}$, 
G.~Lanfranchi$^{18}$, 
C.~Langenbruch$^{48}$, 
B.~Langhans$^{38}$, 
T.~Latham$^{48}$, 
C.~Lazzeroni$^{45}$, 
R.~Le~Gac$^{6}$, 
J.~van~Leerdam$^{41}$, 
J.-P.~Lees$^{4}$, 
R.~Lef\`{e}vre$^{5}$, 
A.~Leflat$^{32}$, 
J.~Lefran\c{c}ois$^{7}$, 
O.~Leroy$^{6}$, 
T.~Lesiak$^{26}$, 
B.~Leverington$^{11}$, 
Y.~Li$^{7}$, 
T.~Likhomanenko$^{64}$, 
M.~Liles$^{52}$, 
R.~Lindner$^{38}$, 
C.~Linn$^{38}$, 
F.~Lionetto$^{40}$, 
B.~Liu$^{15}$, 
S.~Lohn$^{38}$, 
I.~Longstaff$^{51}$, 
J.H.~Lopes$^{2}$, 
P.~Lowdon$^{40}$, 
D.~Lucchesi$^{22,r}$, 
H.~Luo$^{50}$, 
A.~Lupato$^{22}$, 
E.~Luppi$^{16,f}$, 
O.~Lupton$^{55}$, 
F.~Machefert$^{7}$, 
I.V.~Machikhiliyan$^{31}$, 
F.~Maciuc$^{29}$, 
O.~Maev$^{30}$, 
S.~Malde$^{55}$, 
A.~Malinin$^{64}$, 
G.~Manca$^{15,e}$, 
G.~Mancinelli$^{6}$, 
P.~Manning$^{59}$, 
A.~Mapelli$^{38}$, 
J.~Maratas$^{5}$, 
J.F.~Marchand$^{4}$, 
U.~Marconi$^{14}$, 
C.~Marin~Benito$^{36}$, 
P.~Marino$^{23,38,t}$, 
R.~M\"{a}rki$^{39}$, 
J.~Marks$^{11}$, 
G.~Martellotti$^{25}$, 
M.~Martinelli$^{39}$, 
D.~Martinez~Santos$^{42}$, 
F.~Martinez~Vidal$^{66}$, 
D.~Martins~Tostes$^{2}$, 
A.~Massafferri$^{1}$, 
R.~Matev$^{38}$, 
Z.~Mathe$^{38}$, 
C.~Matteuzzi$^{20}$, 
A.~Mauri$^{40}$, 
B.~Maurin$^{39}$, 
A.~Mazurov$^{45}$, 
M.~McCann$^{53}$, 
J.~McCarthy$^{45}$, 
A.~McNab$^{54}$, 
R.~McNulty$^{12}$, 
B.~McSkelly$^{52}$, 
B.~Meadows$^{57}$, 
F.~Meier$^{9}$, 
M.~Meissner$^{11}$, 
M.~Merk$^{41}$, 
D.A.~Milanes$^{62}$, 
M.-N.~Minard$^{4}$, 
D.S.~Mitzel$^{11}$, 
J.~Molina~Rodriguez$^{60}$, 
S.~Monteil$^{5}$, 
M.~Morandin$^{22}$, 
P.~Morawski$^{27}$, 
A.~Mord\`{a}$^{6}$, 
M.J.~Morello$^{23,t}$, 
J.~Moron$^{27}$, 
A.B.~Morris$^{50}$, 
R.~Mountain$^{59}$, 
F.~Muheim$^{50}$, 
J.~M\"{u}ller$^{9}$, 
K.~M\"{u}ller$^{40}$, 
V.~M\"{u}ller$^{9}$, 
M.~Mussini$^{14}$, 
B.~Muster$^{39}$, 
P.~Naik$^{46}$, 
T.~Nakada$^{39}$, 
R.~Nandakumar$^{49}$, 
I.~Nasteva$^{2}$, 
M.~Needham$^{50}$, 
N.~Neri$^{21}$, 
S.~Neubert$^{11}$, 
N.~Neufeld$^{38}$, 
M.~Neuner$^{11}$, 
A.D.~Nguyen$^{39}$, 
T.D.~Nguyen$^{39}$, 
C.~Nguyen-Mau$^{39,q}$, 
V.~Niess$^{5}$, 
R.~Niet$^{9}$, 
N.~Nikitin$^{32}$, 
T.~Nikodem$^{11}$, 
A.~Novoselov$^{35}$, 
D.P.~O'Hanlon$^{48}$, 
A.~Oblakowska-Mucha$^{27}$, 
V.~Obraztsov$^{35}$, 
S.~Ogilvy$^{51}$, 
O.~Okhrimenko$^{44}$, 
R.~Oldeman$^{15,e}$, 
C.J.G.~Onderwater$^{67}$, 
B.~Osorio~Rodrigues$^{1}$, 
J.M.~Otalora~Goicochea$^{2}$, 
A.~Otto$^{38}$, 
P.~Owen$^{53}$, 
A.~Oyanguren$^{66}$, 
A.~Palano$^{13,c}$, 
F.~Palombo$^{21,u}$, 
M.~Palutan$^{18}$, 
J.~Panman$^{38}$, 
A.~Papanestis$^{49}$, 
M.~Pappagallo$^{51}$, 
L.L.~Pappalardo$^{16,f}$, 
C.~Parkes$^{54}$, 
G.~Passaleva$^{17}$, 
G.D.~Patel$^{52}$, 
M.~Patel$^{53}$, 
C.~Patrignani$^{19,j}$, 
A.~Pearce$^{54,49}$, 
A.~Pellegrino$^{41}$, 
G.~Penso$^{25,m}$, 
M.~Pepe~Altarelli$^{38}$, 
S.~Perazzini$^{14,d}$, 
P.~Perret$^{5}$, 
L.~Pescatore$^{45}$, 
K.~Petridis$^{46}$, 
A.~Petrolini$^{19,j}$, 
M.~Petruzzo$^{21}$, 
E.~Picatoste~Olloqui$^{36}$, 
B.~Pietrzyk$^{4}$, 
T.~Pila\v{r}$^{48}$, 
D.~Pinci$^{25}$, 
A.~Pistone$^{19}$, 
S.~Playfer$^{50}$, 
M.~Plo~Casasus$^{37}$, 
T.~Poikela$^{38}$, 
F.~Polci$^{8}$, 
A.~Poluektov$^{48,34}$, 
I.~Polyakov$^{31}$, 
E.~Polycarpo$^{2}$, 
A.~Popov$^{35}$, 
D.~Popov$^{10}$, 
B.~Popovici$^{29}$, 
C.~Potterat$^{2}$, 
E.~Price$^{46}$, 
J.D.~Price$^{52}$, 
J.~Prisciandaro$^{39}$, 
A.~Pritchard$^{52}$, 
C.~Prouve$^{46}$, 
V.~Pugatch$^{44}$, 
A.~Puig~Navarro$^{39}$, 
G.~Punzi$^{23,s}$, 
W.~Qian$^{4}$, 
R.~Quagliani$^{7,46}$, 
B.~Rachwal$^{26}$, 
J.H.~Rademacker$^{46}$, 
B.~Rakotomiaramanana$^{39}$, 
M.~Rama$^{23}$, 
M.S.~Rangel$^{2}$, 
I.~Raniuk$^{43}$, 
N.~Rauschmayr$^{38}$, 
G.~Raven$^{42}$, 
F.~Redi$^{53}$, 
S.~Reichert$^{54}$, 
M.M.~Reid$^{48}$, 
A.C.~dos~Reis$^{1}$, 
S.~Ricciardi$^{49}$, 
S.~Richards$^{46}$, 
M.~Rihl$^{38}$, 
K.~Rinnert$^{52}$, 
V.~Rives~Molina$^{36}$, 
P.~Robbe$^{7,38}$, 
A.B.~Rodrigues$^{1}$, 
E.~Rodrigues$^{54}$, 
P.~Rodriguez~Perez$^{54}$, 
S.~Roiser$^{38}$, 
V.~Romanovsky$^{35}$, 
A.~Romero~Vidal$^{37}$, 
M.~Rotondo$^{22}$, 
J.~Rouvinet$^{39}$, 
T.~Ruf$^{38}$, 
H.~Ruiz$^{36}$, 
P.~Ruiz~Valls$^{66}$, 
J.J.~Saborido~Silva$^{37}$, 
N.~Sagidova$^{30}$, 
P.~Sail$^{51}$, 
B.~Saitta$^{15,e}$, 
V.~Salustino~Guimaraes$^{2}$, 
C.~Sanchez~Mayordomo$^{66}$, 
B.~Sanmartin~Sedes$^{37}$, 
R.~Santacesaria$^{25}$, 
C.~Santamarina~Rios$^{37}$, 
E.~Santovetti$^{24,l}$, 
A.~Sarti$^{18,m}$, 
C.~Satriano$^{25,n}$, 
A.~Satta$^{24}$, 
D.M.~Saunders$^{46}$, 
D.~Savrina$^{31,32}$, 
M.~Schiller$^{38}$, 
H.~Schindler$^{38}$, 
M.~Schlupp$^{9}$, 
M.~Schmelling$^{10}$, 
T.~Schmelzer$^{9}$, 
B.~Schmidt$^{38}$, 
O.~Schneider$^{39}$, 
A.~Schopper$^{38}$, 
M.-H.~Schune$^{7}$, 
R.~Schwemmer$^{38}$, 
B.~Sciascia$^{18}$, 
A.~Sciubba$^{25,m}$, 
A.~Semennikov$^{31}$, 
I.~Sepp$^{53}$, 
N.~Serra$^{40}$, 
J.~Serrano$^{6}$, 
L.~Sestini$^{22}$, 
P.~Seyfert$^{11}$, 
M.~Shapkin$^{35}$, 
I.~Shapoval$^{16,43,f}$, 
Y.~Shcheglov$^{30}$, 
T.~Shears$^{52}$, 
L.~Shekhtman$^{34}$, 
V.~Shevchenko$^{64}$, 
A.~Shires$^{9}$, 
R.~Silva~Coutinho$^{48}$, 
G.~Simi$^{22}$, 
M.~Sirendi$^{47}$, 
N.~Skidmore$^{46}$, 
I.~Skillicorn$^{51}$, 
T.~Skwarnicki$^{59}$, 
E.~Smith$^{55,49}$, 
E.~Smith$^{53}$, 
J.~Smith$^{47}$, 
M.~Smith$^{54}$, 
H.~Snoek$^{41}$, 
M.D.~Sokoloff$^{57,38}$, 
F.J.P.~Soler$^{51}$, 
F.~Soomro$^{39}$, 
D.~Souza$^{46}$, 
B.~Souza~De~Paula$^{2}$, 
B.~Spaan$^{9}$, 
P.~Spradlin$^{51}$, 
S.~Sridharan$^{38}$, 
F.~Stagni$^{38}$, 
M.~Stahl$^{11}$, 
S.~Stahl$^{38}$, 
O.~Steinkamp$^{40}$, 
O.~Stenyakin$^{35}$, 
F.~Sterpka$^{59}$, 
S.~Stevenson$^{55}$, 
S.~Stoica$^{29}$, 
S.~Stone$^{59}$, 
B.~Storaci$^{40}$, 
S.~Stracka$^{23,t}$, 
M.~Straticiuc$^{29}$, 
U.~Straumann$^{40}$, 
R.~Stroili$^{22}$, 
L.~Sun$^{57}$, 
W.~Sutcliffe$^{53}$, 
K.~Swientek$^{27}$, 
S.~Swientek$^{9}$, 
V.~Syropoulos$^{42}$, 
M.~Szczekowski$^{28}$, 
P.~Szczypka$^{39,38}$, 
T.~Szumlak$^{27}$, 
S.~T'Jampens$^{4}$, 
T.~Tekampe$^{9}$, 
M.~Teklishyn$^{7}$, 
G.~Tellarini$^{16,f}$, 
F.~Teubert$^{38}$, 
C.~Thomas$^{55}$, 
E.~Thomas$^{38}$, 
J.~van~Tilburg$^{41}$, 
V.~Tisserand$^{4}$, 
M.~Tobin$^{39}$, 
J.~Todd$^{57}$, 
S.~Tolk$^{42}$, 
L.~Tomassetti$^{16,f}$, 
D.~Tonelli$^{38}$, 
S.~Topp-Joergensen$^{55}$, 
N.~Torr$^{55}$, 
E.~Tournefier$^{4}$, 
S.~Tourneur$^{39}$, 
K.~Trabelsi$^{39}$, 
M.T.~Tran$^{39}$, 
M.~Tresch$^{40}$, 
A.~Trisovic$^{38}$, 
A.~Tsaregorodtsev$^{6}$, 
P.~Tsopelas$^{41}$, 
N.~Tuning$^{41,38}$, 
M.~Ubeda~Garcia$^{38}$, 
A.~Ukleja$^{28}$, 
A.~Ustyuzhanin$^{65,64}$, 
U.~Uwer$^{11}$, 
C.~Vacca$^{15,e}$, 
V.~Vagnoni$^{14}$, 
G.~Valenti$^{14}$, 
A.~Vallier$^{7}$, 
R.~Vazquez~Gomez$^{18}$, 
P.~Vazquez~Regueiro$^{37}$, 
C.~V\'{a}zquez~Sierra$^{37}$, 
S.~Vecchi$^{16}$, 
J.J.~Velthuis$^{46}$, 
M.~Veltri$^{17,h}$, 
G.~Veneziano$^{39}$, 
M.~Vesterinen$^{11}$, 
B.~Viaud$^{7}$, 
D.~Vieira$^{2}$, 
M.~Vieites~Diaz$^{37}$, 
X.~Vilasis-Cardona$^{36,p}$, 
A.~Vollhardt$^{40}$, 
D.~Volyanskyy$^{10}$, 
D.~Voong$^{46}$, 
A.~Vorobyev$^{30}$, 
V.~Vorobyev$^{34}$, 
C.~Vo\ss$^{63}$, 
J.A.~de~Vries$^{41}$, 
R.~Waldi$^{63}$, 
C.~Wallace$^{48}$, 
R.~Wallace$^{12}$, 
J.~Walsh$^{23}$, 
S.~Wandernoth$^{11}$, 
J.~Wang$^{59}$, 
D.R.~Ward$^{47}$, 
N.K.~Watson$^{45}$, 
D.~Websdale$^{53}$, 
A.~Weiden$^{40}$, 
M.~Whitehead$^{48}$, 
D.~Wiedner$^{11}$, 
G.~Wilkinson$^{55,38}$, 
M.~Wilkinson$^{59}$, 
M.~Williams$^{38}$, 
M.P.~Williams$^{45}$, 
M.~Williams$^{56}$, 
F.F.~Wilson$^{49}$, 
J.~Wimberley$^{58}$, 
J.~Wishahi$^{9}$, 
W.~Wislicki$^{28}$, 
M.~Witek$^{26}$, 
G.~Wormser$^{7}$, 
S.A.~Wotton$^{47}$, 
S.~Wright$^{47}$, 
K.~Wyllie$^{38}$, 
Y.~Xie$^{61}$, 
Z.~Xu$^{39}$, 
Z.~Yang$^{3}$, 
X.~Yuan$^{34}$, 
O.~Yushchenko$^{35}$, 
M.~Zangoli$^{14}$, 
M.~Zavertyaev$^{10,b}$, 
L.~Zhang$^{3}$, 
Y.~Zhang$^{3}$, 
A.~Zhelezov$^{11}$, 
A.~Zhokhov$^{31}$, 
L.~Zhong$^{3}$.\bigskip

{\footnotesize \it
%$\dagger$ deceased.\\[1ex]
$ ^{1}$Centro Brasileiro de Pesquisas F\'{i}sicas (CBPF), Rio de Janeiro, Brazil\\
$ ^{2}$Universidade Federal do Rio de Janeiro (UFRJ), Rio de Janeiro, Brazil\\
$ ^{3}$Center for High Energy Physics, Tsinghua University, Beijing, China\\
$ ^{4}$LAPP, Universit\'{e} Savoie Mont-Blanc, CNRS/IN2P3, Annecy-Le-Vieux, France\\
$ ^{5}$Clermont Universit\'{e}, Universit\'{e} Blaise Pascal, CNRS/IN2P3, LPC, Clermont-Ferrand, France\\
$ ^{6}$CPPM, Aix-Marseille Universit\'{e}, CNRS/IN2P3, Marseille, France\\
$ ^{7}$LAL, Universit\'{e} Paris-Sud, CNRS/IN2P3, Orsay, France\\
$ ^{8}$LPNHE, Universit\'{e} Pierre et Marie Curie, Universit\'{e} Paris Diderot, CNRS/IN2P3, Paris, France\\
$ ^{9}$Fakult\"{a}t Physik, Technische Universit\"{a}t Dortmund, Dortmund, Germany\\
$ ^{10}$Max-Planck-Institut f\"{u}r Kernphysik (MPIK), Heidelberg, Germany\\
$ ^{11}$Physikalisches Institut, Ruprecht-Karls-Universit\"{a}t Heidelberg, Heidelberg, Germany\\
$ ^{12}$School of Physics, University College Dublin, Dublin, Ireland\\
$ ^{13}$Sezione INFN di Bari, Bari, Italy\\
$ ^{14}$Sezione INFN di Bologna, Bologna, Italy\\
$ ^{15}$Sezione INFN di Cagliari, Cagliari, Italy\\
$ ^{16}$Sezione INFN di Ferrara, Ferrara, Italy\\
$ ^{17}$Sezione INFN di Firenze, Firenze, Italy\\
$ ^{18}$Laboratori Nazionali dell'INFN di Frascati, Frascati, Italy\\
$ ^{19}$Sezione INFN di Genova, Genova, Italy\\
$ ^{20}$Sezione INFN di Milano Bicocca, Milano, Italy\\
$ ^{21}$Sezione INFN di Milano, Milano, Italy\\
$ ^{22}$Sezione INFN di Padova, Padova, Italy\\
$ ^{23}$Sezione INFN di Pisa, Pisa, Italy\\
$ ^{24}$Sezione INFN di Roma Tor Vergata, Roma, Italy\\
$ ^{25}$Sezione INFN di Roma La Sapienza, Roma, Italy\\
$ ^{26}$Henryk Niewodniczanski Institute of Nuclear Physics  Polish Academy of Sciences, Krak\'{o}w, Poland\\
$ ^{27}$AGH - University of Science and Technology, Faculty of Physics and Applied Computer Science, Krak\'{o}w, Poland\\
$ ^{28}$National Center for Nuclear Research (NCBJ), Warsaw, Poland\\
$ ^{29}$Horia Hulubei National Institute of Physics and Nuclear Engineering, Bucharest-Magurele, Romania\\
$ ^{30}$Petersburg Nuclear Physics Institute (PNPI), Gatchina, Russia\\
$ ^{31}$Institute of Theoretical and Experimental Physics (ITEP), Moscow, Russia\\
$ ^{32}$Institute of Nuclear Physics, Moscow State University (SINP MSU), Moscow, Russia\\
$ ^{33}$Institute for Nuclear Research of the Russian Academy of Sciences (INR RAN), Moscow, Russia\\
$ ^{34}$Budker Institute of Nuclear Physics (SB RAS) and Novosibirsk State University, Novosibirsk, Russia\\
$ ^{35}$Institute for High Energy Physics (IHEP), Protvino, Russia\\
$ ^{36}$Universitat de Barcelona, Barcelona, Spain\\
$ ^{37}$Universidad de Santiago de Compostela, Santiago de Compostela, Spain\\
$ ^{38}$European Organization for Nuclear Research (CERN), Geneva, Switzerland\\
$ ^{39}$Ecole Polytechnique F\'{e}d\'{e}rale de Lausanne (EPFL), Lausanne, Switzerland\\
$ ^{40}$Physik-Institut, Universit\"{a}t Z\"{u}rich, Z\"{u}rich, Switzerland\\
$ ^{41}$Nikhef National Institute for Subatomic Physics, Amsterdam, The Netherlands\\
$ ^{42}$Nikhef National Institute for Subatomic Physics and VU University Amsterdam, Amsterdam, The Netherlands\\
$ ^{43}$NSC Kharkiv Institute of Physics and Technology (NSC KIPT), Kharkiv, Ukraine\\
$ ^{44}$Institute for Nuclear Research of the National Academy of Sciences (KINR), Kyiv, Ukraine\\
$ ^{45}$University of Birmingham, Birmingham, United Kingdom\\
$ ^{46}$H.H. Wills Physics Laboratory, University of Bristol, Bristol, United Kingdom\\
$ ^{47}$Cavendish Laboratory, University of Cambridge, Cambridge, United Kingdom\\
$ ^{48}$Department of Physics, University of Warwick, Coventry, United Kingdom\\
$ ^{49}$STFC Rutherford Appleton Laboratory, Didcot, United Kingdom\\
$ ^{50}$School of Physics and Astronomy, University of Edinburgh, Edinburgh, United Kingdom\\
$ ^{51}$School of Physics and Astronomy, University of Glasgow, Glasgow, United Kingdom\\
$ ^{52}$Oliver Lodge Laboratory, University of Liverpool, Liverpool, United Kingdom\\
$ ^{53}$Imperial College London, London, United Kingdom\\
$ ^{54}$School of Physics and Astronomy, University of Manchester, Manchester, United Kingdom\\
$ ^{55}$Department of Physics, University of Oxford, Oxford, United Kingdom\\
$ ^{56}$Massachusetts Institute of Technology, Cambridge, MA, United States\\
$ ^{57}$University of Cincinnati, Cincinnati, OH, United States\\
$ ^{58}$University of Maryland, College Park, MD, United States\\
$ ^{59}$Syracuse University, Syracuse, NY, United States\\
$ ^{60}$Pontif\'{i}cia Universidade Cat\'{o}lica do Rio de Janeiro (PUC-Rio), Rio de Janeiro, Brazil, associated to $^{2}$\\
$ ^{61}$Institute of Particle Physics, Central China Normal University, Wuhan, Hubei, China, associated to $^{3}$\\
$ ^{62}$Departamento de Fisica , Universidad Nacional de Colombia, Bogota, Colombia, associated to $^{8}$\\
$ ^{63}$Institut f\"{u}r Physik, Universit\"{a}t Rostock, Rostock, Germany, associated to $^{11}$\\
$ ^{64}$National Research Centre Kurchatov Institute, Moscow, Russia, associated to $^{31}$\\
$ ^{65}$Yandex School of Data Analysis, Moscow, Russia, associated to $^{31}$\\
$ ^{66}$Instituto de Fisica Corpuscular (IFIC), Universitat de Valencia-CSIC, Valencia, Spain, associated to $^{36}$\\
$ ^{67}$Van Swinderen Institute, University of Groningen, Groningen, The Netherlands, associated to $^{41}$\\
\bigskip
$ ^{a}$Universidade Federal do Tri\^{a}ngulo Mineiro (UFTM), Uberaba-MG, Brazil\\
$ ^{b}$P.N. Lebedev Physical Institute, Russian Academy of Science (LPI RAS), Moscow, Russia\\
$ ^{c}$Universit\`{a} di Bari, Bari, Italy\\
$ ^{d}$Universit\`{a} di Bologna, Bologna, Italy\\
$ ^{e}$Universit\`{a} di Cagliari, Cagliari, Italy\\
$ ^{f}$Universit\`{a} di Ferrara, Ferrara, Italy\\
$ ^{g}$Universit\`{a} di Firenze, Firenze, Italy\\
$ ^{h}$Universit\`{a} di Urbino, Urbino, Italy\\
$ ^{i}$Universit\`{a} di Modena e Reggio Emilia, Modena, Italy\\
$ ^{j}$Universit\`{a} di Genova, Genova, Italy\\
$ ^{k}$Universit\`{a} di Milano Bicocca, Milano, Italy\\
$ ^{l}$Universit\`{a} di Roma Tor Vergata, Roma, Italy\\
$ ^{m}$Universit\`{a} di Roma La Sapienza, Roma, Italy\\
$ ^{n}$Universit\`{a} della Basilicata, Potenza, Italy\\
$ ^{o}$AGH - University of Science and Technology, Faculty of Computer Science, Electronics and Telecommunications, Krak\'{o}w, Poland\\
$ ^{p}$LIFAELS, La Salle, Universitat Ramon Llull, Barcelona, Spain\\
$ ^{q}$Hanoi University of Science, Hanoi, Viet Nam\\
$ ^{r}$Universit\`{a} di Padova, Padova, Italy\\
$ ^{s}$Universit\`{a} di Pisa, Pisa, Italy\\
$ ^{t}$Scuola Normale Superiore, Pisa, Italy\\
$ ^{u}$Universit\`{a} degli Studi di Milano, Milano, Italy\\
$ ^{v}$Politecnico di Milano, Milano, Italy\\
\medskip
$ ^{\dagger}$Deceased
}
\end{flushleft}
%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%

LHCb_HD_comma_separated_author_2015-01-13.tex
LHCb collaboration:
R. Aaij, 
B. Adeva, 
M. Adinolfi, 
A. Affolder, 
Z. Ajaltouni, 
S. Akar, 
J. Albrecht, 
F. Alessio, 
M. Alexander, 
S. Ali, 
G. Alkhazov, 
P. Alvarez Cartelle, 
A.A. Alves Jr, 
S. Amato, 
S. Amerio, 
Y. Amhis, 
L. An, 
L. Anderlini, 
J. Anderson, 
M. Andreotti, 
J.E. Andrews, 
R.B. Appleby, 
O. Aquines Gutierrez, 
F. Archilli, 
P. d'Argent, 
A. Artamonov, 
M. Artuso, 
E. Aslanides, 
G. Auriemma, 
M. Baalouch, 
S. Bachmann, 
J.J. Back, 
A. Badalov, 
C. Baesso, 
W. Baldini, 
R.J. Barlow, 
C. Barschel, 
S. Barsuk, 
W. Barter, 
V. Batozskaya, 
V. Battista, 
A. Bay, 
L. Beaucourt, 
J. Beddow, 
F. Bedeschi, 
I. Bediaga, 
L.J. Bel, 
I. Belyaev, 
E. Ben-Haim, 
G. Bencivenni, 
S. Benson, 
J. Benton, 
A. Berezhnoy, 
R. Bernet, 
A. Bertolin, 
M.-O. Bettler, 
M. van Beuzekom, 
A. Bien, 
S. Bifani, 
T. Bird, 
A. Birnkraut, 
A. Bizzeti, 
T. Blake, 
F. Blanc, 
J. Blouw, 
S. Blusk, 
V. Bocci, 
A. Bondar, 
N. Bondar, 
W. Bonivento, 
S. Borghi, 
A. Borgia, 
M. Borsato, 
T.J.V. Bowcock, 
E. Bowen, 
C. Bozzi, 
D. Brett, 
M. Britsch, 
T. Britton, 
J. Brodzicka, 
N.H. Brook, 
A. Bursche, 
J. Buytaert, 
S. Cadeddu, 
R. Calabrese, 
M. Calvi, 
M. Calvo Gomez, 
P. Campana, 
D. Campora Perez, 
L. Capriotti, 
A. Carbone, 
G. Carboni, 
R. Cardinale, 
A. Cardini, 
P. Carniti, 
L. Carson, 
K. Carvalho Akiba, 
R. Casanova Mohr, 
G. Casse, 
L. Cassina, 
L. Castillo Garcia, 
M. Cattaneo, 
Ch. Cauet, 
G. Cavallero, 
R. Cenci, 
M. Charles, 
Ph. Charpentier, 
M. Chefdeville, 
S. Chen, 
S.-F. Cheung, 
N. Chiapolini, 
M. Chrzaszcz, 
X. Cid Vidal, 
G. Ciezarek, 
P.E.L. Clarke, 
M. Clemencic, 
H.V. Cliff, 
J. Closier, 
V. Coco, 
J. Cogan, 
E. Cogneras, 
V. Cogoni, 
L. Cojocariu, 
G. Collazuol, 
P. Collins, 
A. Comerma-Montells, 
A. Contu, 
A. Cook, 
M. Coombes, 
S. Coquereau, 
G. Corti, 
M. Corvo, 
I. Counts, 
B. Couturier, 
G.A. Cowan, 
D.C. Craik, 
A. Crocombe, 
M. Cruz Torres, 
S. Cunliffe, 
R. Currie, 
C. D'Ambrosio, 
J. Dalseno, 
P.N.Y. David, 
A. Davis, 
K. De Bruyn, 
S. De Capua, 
M. De Cian, 
J.M. De Miranda, 
L. De Paula, 
W. De Silva, 
P. De Simone, 
C.-T. Dean, 
D. Decamp, 
M. Deckenhoff, 
L. Del Buono, 
N. D\'{e}l\'{e}age, 
D. Derkach, 
O. Deschamps, 
F. Dettori, 
B. Dey, 
A. Di Canto, 
F. Di Ruscio, 
H. Dijkstra, 
S. Donleavy, 
F. Dordei, 
M. Dorigo, 
A. Dosil Su\'{a}rez, 
D. Dossett, 
A. Dovbnya, 
K. Dreimanis, 
G. Dujany, 
F. Dupertuis, 
P. Durante, 
R. Dzhelyadin, 
A. Dziurda, 
A. Dzyuba, 
S. Easo, 
U. Egede, 
V. Egorychev, 
S. Eidelman, 
S. Eisenhardt, 
U. Eitschberger, 
R. Ekelhof, 
L. Eklund, 
I. El Rifai, 
Ch. Elsasser, 
S. Ely, 
S. Esen, 
H.M. Evans, 
T. Evans, 
A. Falabella, 
C. F\"{a}rber, 
C. Farinelli, 
N. Farley, 
S. Farry, 
R. Fay, 
D. Ferguson, 
V. Fernandez Albor, 
F. Ferrari, 
F. Ferreira Rodrigues, 
M. Ferro-Luzzi, 
S. Filippov, 
M. Fiore, 
M. Fiorini, 
M. Firlej, 
C. Fitzpatrick, 
T. Fiutowski, 
P. Fol, 
M. Fontana, 
F. Fontanelli, 
R. Forty, 
O. Francisco, 
M. Frank, 
C. Frei, 
M. Frosini, 
J. Fu, 
E. Furfaro, 
A. Gallas Torreira, 
D. Galli, 
S. Gallorini, 
S. Gambetta, 
M. Gandelman, 
P. Gandini, 
Y. Gao, 
J. Garc\'{i}a Pardi\~{n}as, 
J. Garofoli, 
J. Garra Tico, 
L. Garrido, 
D. Gascon, 
C. Gaspar, 
U. Gastaldi, 
R. Gauld, 
L. Gavardi, 
G. Gazzoni, 
A. Geraci, 
D. Gerick, 
E. Gersabeck, 
M. Gersabeck, 
T. Gershon, 
Ph. Ghez, 
A. Gianelle, 
S. Gian\`{i}, 
V. Gibson, 
L. Giubega, 
V.V. Gligorov, 
C. G\"{o}bel, 
D. Golubkov, 
A. Golutvin, 
A. Gomes, 
C. Gotti, 
M. Grabalosa G\'{a}ndara, 
R. Graciani Diaz, 
L.A. Granado Cardoso, 
E. Graug\'{e}s, 
E. Graverini, 
G. Graziani, 
A. Grecu, 
E. Greening, 
S. Gregson, 
P. Griffith, 
L. Grillo, 
O. Gr\"{u}nberg, 
B. Gui, 
E. Gushchin, 
Yu. Guz, 
T. Gys, 
C. Hadjivasiliou, 
G. Haefeli, 
C. Haen, 
S.C. Haines, 
S. Hall, 
B. Hamilton, 
T. Hampson, 
X. Han, 
S. Hansmann-Menzemer, 
N. Harnew, 
S.T. Harnew, 
J. Harrison, 
J. He, 
T. Head, 
V. Heijne, 
K. Hennessy, 
P. Henrard, 
L. Henry, 
J.A. Hernando Morata, 
E. van Herwijnen, 
M. He\ss, 
A. Hicheur, 
D. Hill, 
M. Hoballah, 
C. Hombach, 
W. Hulsbergen, 
T. Humair, 
N. Hussain, 
D. Hutchcroft, 
D. Hynds, 
M. Idzik, 
P. Ilten, 
R. Jacobsson, 
A. Jaeger, 
J. Jalocha, 
E. Jans, 
A. Jawahery, 
F. Jing, 
M. John, 
D. Johnson, 
C.R. Jones, 
C. Joram, 
B. Jost, 
N. Jurik, 
S. Kandybei, 
W. Kanso, 
M. Karacson, 
T.M. Karbach, 
S. Karodia, 
M. Kelsey, 
I.R. Kenyon, 
M. Kenzie, 
T. Ketel, 
B. Khanji, 
C. Khurewathanakul, 
S. Klaver, 
K. Klimaszewski, 
O. Kochebina, 
M. Kolpin, 
I. Komarov, 
R.F. Koopman, 
P. Koppenburg, 
M. Korolev, 
L. Kravchuk, 
K. Kreplin, 
M. Kreps, 
G. Krocker, 
P. Krokovny, 
F. Kruse, 
W. Kucewicz, 
M. Kucharczyk, 
V. Kudryavtsev, 
K. Kurek, 
T. Kvaratskheliya, 
V.N. La Thi, 
D. Lacarrere, 
G. Lafferty, 
A. Lai, 
D. Lambert, 
R.W. Lambert, 
G. Lanfranchi, 
C. Langenbruch, 
B. Langhans, 
T. Latham, 
C. Lazzeroni, 
R. Le Gac, 
J. van Leerdam, 
J.-P. Lees, 
R. Lef\`{e}vre, 
A. Leflat, 
J. Lefran\c{c}ois, 
O. Leroy, 
T. Lesiak, 
B. Leverington, 
Y. Li, 
T. Likhomanenko, 
M. Liles, 
R. Lindner, 
C. Linn, 
F. Lionetto, 
B. Liu, 
S. Lohn, 
I. Longstaff, 
J.H. Lopes, 
P. Lowdon, 
D. Lucchesi, 
H. Luo, 
A. Lupato, 
E. Luppi, 
O. Lupton, 
F. Machefert, 
I.V. Machikhiliyan, 
F. Maciuc, 
O. Maev, 
S. Malde, 
A. Malinin, 
G. Manca, 
G. Mancinelli, 
P. Manning, 
A. Mapelli, 
J. Maratas, 
J.F. Marchand, 
U. Marconi, 
C. Marin Benito, 
P. Marino, 
R. M\"{a}rki, 
J. Marks, 
G. Martellotti, 
M. Martinelli, 
D. Martinez Santos, 
F. Martinez Vidal, 
D. Martins Tostes, 
A. Massafferri, 
R. Matev, 
Z. Mathe, 
C. Matteuzzi, 
A. Mauri, 
B. Maurin, 
A. Mazurov, 
M. McCann, 
J. McCarthy, 
A. McNab, 
R. McNulty, 
B. McSkelly, 
B. Meadows, 
F. Meier, 
M. Meissner, 
M. Merk, 
D.A. Milanes, 
M.-N. Minard, 
D.S. Mitzel, 
J. Molina Rodriguez, 
S. Monteil, 
M. Morandin, 
P. Morawski, 
A. Mord\`{a}, 
M.J. Morello, 
J. Moron, 
A.B. Morris, 
R. Mountain, 
F. Muheim, 
J. M\"{u}ller, 
K. M\"{u}ller, 
V. M\"{u}ller, 
M. Mussini, 
B. Muster, 
P. Naik, 
T. Nakada, 
R. Nandakumar, 
I. Nasteva, 
M. Needham, 
N. Neri, 
S. Neubert, 
N. Neufeld, 
M. Neuner, 
A.D. Nguyen, 
T.D. Nguyen, 
C. Nguyen-Mau, 
V. Niess, 
R. Niet, 
N. Nikitin, 
T. Nikodem, 
A. Novoselov, 
D.P. O'Hanlon, 
A. Oblakowska-Mucha, 
V. Obraztsov, 
S. Ogilvy, 
O. Okhrimenko, 
R. Oldeman, 
C.J.G. Onderwater, 
B. Osorio Rodrigues, 
J.M. Otalora Goicochea, 
A. Otto, 
P. Owen, 
A. Oyanguren, 
A. Palano, 
F. Palombo, 
M. Palutan, 
J. Panman, 
A. Papanestis, 
M. Pappagallo, 
L.L. Pappalardo, 
C. Parkes, 
G. Passaleva, 
G.D. Patel, 
M. Patel, 
C. Patrignani, 
A. Pearce, 
A. Pellegrino, 
G. Penso, 
M. Pepe Altarelli, 
S. Perazzini, 
P. Perret, 
L. Pescatore, 
K. Petridis, 
A. Petrolini, 
M. Petruzzo, 
E. Picatoste Olloqui, 
B. Pietrzyk, 
T. Pila\v{r}, 
D. Pinci, 
A. Pistone, 
S. Playfer, 
M. Plo Casasus, 
T. Poikela, 
F. Polci, 
A. Poluektov, 
I. Polyakov, 
E. Polycarpo, 
A. Popov, 
D. Popov, 
B. Popovici, 
C. Potterat, 
E. Price, 
J.D. Price, 
J. Prisciandaro, 
A. Pritchard, 
C. Prouve, 
V. Pugatch, 
A. Puig Navarro, 
G. Punzi, 
W. Qian, 
R. Quagliani, 
B. Rachwal, 
J.H. Rademacker, 
B. Rakotomiaramanana, 
M. Rama, 
M.S. Rangel, 
I. Raniuk, 
N. Rauschmayr, 
G. Raven, 
F. Redi, 
S. Reichert, 
M.M. Reid, 
A.C. dos Reis, 
S. Ricciardi, 
S. Richards, 
M. Rihl, 
K. Rinnert, 
V. Rives Molina, 
P. Robbe, 
A.B. Rodrigues, 
E. Rodrigues, 
P. Rodriguez Perez, 
S. Roiser, 
V. Romanovsky, 
A. Romero Vidal, 
M. Rotondo, 
J. Rouvinet, 
T. Ruf, 
H. Ruiz, 
P. Ruiz Valls, 
J.J. Saborido Silva, 
N. Sagidova, 
P. Sail, 
B. Saitta, 
V. Salustino Guimaraes, 
C. Sanchez Mayordomo, 
B. Sanmartin Sedes, 
R. Santacesaria, 
C. Santamarina Rios, 
E. Santovetti, 
A. Sarti, 
C. Satriano, 
A. Satta, 
D.M. Saunders, 
D. Savrina, 
M. Schiller, 
H. Schindler, 
M. Schlupp, 
M. Schmelling, 
T. Schmelzer, 
B. Schmidt, 
O. Schneider, 
A. Schopper, 
M.-H. Schune, 
R. Schwemmer, 
B. Sciascia, 
A. Sciubba, 
A. Semennikov, 
I. Sepp, 
N. Serra, 
J. Serrano, 
L. Sestini, 
P. Seyfert, 
M. Shapkin, 
I. Shapoval, 
Y. Shcheglov, 
T. Shears, 
L. Shekhtman, 
V. Shevchenko, 
A. Shires, 
R. Silva Coutinho, 
G. Simi, 
M. Sirendi, 
N. Skidmore, 
I. Skillicorn, 
T. Skwarnicki, 
E. Smith, 
E. Smith, 
J. Smith, 
M. Smith, 
H. Snoek, 
M.D. Sokoloff, 
F.J.P. Soler, 
F. Soomro, 
D. Souza, 
B. Souza De Paula, 
B. Spaan, 
P. Spradlin, 
S. Sridharan, 
F. Stagni, 
M. Stahl, 
S. Stahl, 
O. Steinkamp, 
O. Stenyakin, 
F. Sterpka, 
S. Stevenson, 
S. Stoica, 
S. Stone, 
B. Storaci, 
S. Stracka, 
M. Straticiuc, 
U. Straumann, 
R. Stroili, 
L. Sun, 
W. Sutcliffe, 
K. Swientek, 
S. Swientek, 
V. Syropoulos, 
M. Szczekowski, 
P. Szczypka, 
T. Szumlak, 
S. T'Jampens, 
T. Tekampe, 
M. Teklishyn, 
G. Tellarini, 
F. Teubert, 
C. Thomas, 
E. Thomas, 
J. van Tilburg, 
V. Tisserand, 
M. Tobin, 
J. Todd, 
S. Tolk, 
L. Tomassetti, 
D. Tonelli, 
S. Topp-Joergensen, 
N. Torr, 
E. Tournefier, 
S. Tourneur, 
K. Trabelsi, 
M.T. Tran, 
M. Tresch, 
A. Trisovic, 
A. Tsaregorodtsev, 
P. Tsopelas, 
N. Tuning, 
M. Ubeda Garcia, 
A. Ukleja, 
A. Ustyuzhanin, 
U. Uwer, 
C. Vacca, 
V. Vagnoni, 
G. Valenti, 
A. Vallier, 
R. Vazquez Gomez, 
P. Vazquez Regueiro, 
C. V\'{a}zquez Sierra, 
S. Vecchi, 
J.J. Velthuis, 
M. Veltri, 
G. Veneziano, 
M. Vesterinen, 
B. Viaud, 
D. Vieira, 
M. Vieites Diaz, 
X. Vilasis-Cardona, 
A. Vollhardt, 
D. Volyanskyy, 
D. Voong, 
A. Vorobyev, 
V. Vorobyev, 
C. Vo\ss, 
J.A. de Vries, 
R. Waldi, 
C. Wallace, 
R. Wallace, 
J. Walsh, 
S. Wandernoth, 
J. Wang, 
D.R. Ward, 
N.K. Watson, 
D. Websdale, 
A. Weiden, 
M. Whitehead, 
D. Wiedner, 
G. Wilkinson, 
M. Wilkinson, 
M. Williams, 
M.P. Williams, 
M. Williams, 
F.F. Wilson, 
J. Wimberley, 
J. Wishahi, 
W. Wislicki, 
M. Witek, 
G. Wormser, 
S.A. Wotton, 
S. Wright, 
K. Wyllie, 
Y. Xie, 
Z. Xu, 
Z. Yang, 
X. Yuan, 
O. Yushchenko, 
M. Zangoli, 
M. Zavertyaev, 
L. Zhang, 
Y. Zhang, 
A. Zhelezov, 
A. Zhokhov, 
L. Zhong

lhcb-symbols-def.tex
%%% $Id: lhcb-symbols-def.tex 71144 2015-04-16 15:53:48Z rwallace $
%%% ======================================================================
%%% Purpose: Standard LHCb aliases
%%% Author: Originally Ulrik Egede, adapted by Tomasz Skwarnicki for templates,
%%% rewritten by Chris Parkes
%%% Maintainer : Ulrik Egede (2010 - 2012)
%%% Maintainer : Rolf Oldeman (2012 - 2014)
%%% =======================================================================

%%% To use this file outside the normal LHCb document environment, the
%%% following should be added in a preamble (before \begin{document}
%%%
%%%\usepackage{ifthen} 
%%%\newboolean{uprightparticles}
%%%\setboolean{uprightparticles}{false} %Set true for upright particle symbols
%%% \usepackage{xspace} 
%%% \usepackage{upgreek}

%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
%%%
%%% The following is to ensure that the template automatically can process
%%% this file.
%%%
%%% Add comments with at least three %%% preceding.
%%% Add new sections with one % preceding
%%% Add new subsections with two %% preceding
%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%

%%%%%%%%%%%%%
% Experiments
%%%%%%%%%%%%%
\def\lhcb {\mbox{LHCb}\xspace}
\def\atlas  {\mbox{ATLAS}\xspace}
\def\cms    {\mbox{CMS}\xspace}
\def\alice  {\mbox{ALICE}\xspace}
\def\babar  {\mbox{BaBar}\xspace}
\def\belle  {\mbox{Belle}\xspace}
\def\cleo   {\mbox{CLEO}\xspace}
\def\cdf    {\mbox{CDF}\xspace}
\def\dzero  {\mbox{D0}\xspace}
\def\aleph  {\mbox{ALEPH}\xspace}
\def\delphi {\mbox{DELPHI}\xspace}
\def\opal   {\mbox{OPAL}\xspace}
\def\lthree {\mbox{L3}\xspace}
\def\sld    {\mbox{SLD}\xspace}
%%%\def\argus  {\mbox{ARGUS}\xspace}
%%%\def\uaone  {\mbox{UA1}\xspace}
%%%\def\uatwo  {\mbox{UA2}\xspace}
%%%\def\ux85 {\mbox{UX85}\xspace}
\def\cern {\mbox{CERN}\xspace}
\def\lhc    {\mbox{LHC}\xspace}
\def\lep    {\mbox{LEP}\xspace}
\def\tevatron {Tevatron\xspace}

%% LHCb sub-detectors and sub-systems

%%%\def\pu     {PU\xspace}
\def\velo   {VELO\xspace}
\def\rich   {RICH\xspace}
\def\richone {RICH1\xspace}
\def\richtwo {RICH2\xspace}
\def\ttracker {TT\xspace}
\def\intr   {IT\xspace}
\def\st     {ST\xspace}
\def\ot     {OT\xspace}
%%%\def\Tone   {T1\xspace}
%%%\def\Ttwo   {T2\xspace}
%%%\def\Tthree {T3\xspace}
%%%\def\Mone   {M1\xspace}
%%%\def\Mtwo   {M2\xspace}
%%%\def\Mthree {M3\xspace}
%%%\def\Mfour  {M4\xspace}
%%%\def\Mfive  {M5\xspace}
\def\spd    {SPD\xspace}
\def\presh  {PS\xspace}
\def\ecal   {ECAL\xspace}
\def\hcal   {HCAL\xspace}
%%%\def\bcm    {BCM\xspace}
\def\MagUp {\mbox{\em Mag\kern -0.05em Up}\xspace}
\def\MagDown {\mbox{\em MagDown}\xspace}

%%%\def\ode    {ODE\xspace}
%%%\def\daq    {DAQ\xspace}
%%%\def\tfc    {TFC\xspace}
%%%\def\ecs    {ECS\xspace}
%%%\def\lone   {L0\xspace}
%%%\def\hlt    {HLT\xspace}
%%%\def\hltone {HLT1\xspace}
%%%\def\hlttwo {HLT2\xspace}

%%% Upright (not slanted) Particles

\ifthenelse{\boolean{uprightparticles}}%
{\def\Palpha      {\ensuremath{\upalpha}\xspace}
 \def\Pbeta       {\ensuremath{\upbeta}\xspace}
 \def\Pgamma      {\ensuremath{\upgamma}\xspace}                 
 \def\Pdelta      {\ensuremath{\updelta}\xspace}                 
 \def\Pepsilon    {\ensuremath{\upepsilon}\xspace}                 
 \def\Pvarepsilon {\ensuremath{\upvarepsilon}\xspace}                 
 \def\Pzeta       {\ensuremath{\upzeta}\xspace}                 
 \def\Peta        {\ensuremath{\upeta}\xspace}                 
 \def\Ptheta      {\ensuremath{\uptheta}\xspace}                 
 \def\Pvartheta   {\ensuremath{\upvartheta}\xspace}                 
 \def\Piota       {\ensuremath{\upiota}\xspace}                 
 \def\Pkappa      {\ensuremath{\upkappa}\xspace}                 
 \def\Plambda     {\ensuremath{\uplambda}\xspace}                 
 \def\Pmu         {\ensuremath{\upmu}\xspace}                 
 \def\Pnu         {\ensuremath{\upnu}\xspace}                 
 \def\Pxi         {\ensuremath{\upxi}\xspace}                 
 \def\Ppi         {\ensuremath{\uppi}\xspace}                 
 \def\Pvarpi      {\ensuremath{\upvarpi}\xspace}                 
 \def\Prho        {\ensuremath{\uprho}\xspace}                 
 \def\Pvarrho     {\ensuremath{\upvarrho}\xspace}                 
 \def\Ptau        {\ensuremath{\uptau}\xspace}                 
 \def\Pupsilon    {\ensuremath{\upupsilon}\xspace}                 
 \def\Pphi        {\ensuremath{\upphi}\xspace}                 
 \def\Pvarphi     {\ensuremath{\upvarphi}\xspace}                 
 \def\Pchi        {\ensuremath{\upchi}\xspace}                 
 \def\Ppsi        {\ensuremath{\uppsi}\xspace}                 
 \def\Pomega      {\ensuremath{\upomega}\xspace}                 

 \def\PDelta      {\ensuremath{\Delta}\xspace}                 
 \def\PXi      {\ensuremath{\Xi}\xspace}                 
 \def\PLambda      {\ensuremath{\Lambda}\xspace}                 
 \def\PSigma      {\ensuremath{\Sigma}\xspace}                 
 \def\POmega      {\ensuremath{\Omega}\xspace}                 
 \def\PUpsilon      {\ensuremath{\Upsilon}\xspace}                 
 
 %\mathchardef\Deltares="7101
 %\mathchardef\Xi="7104
 %\mathchardef\Lambda="7103
 %\mathchardef\Sigma="7106
 %\mathchardef\Omega="710A


 \def\PA      {\ensuremath{\mathrm{A}}\xspace}                 
 \def\PB      {\ensuremath{\mathrm{B}}\xspace}                 
 \def\PC      {\ensuremath{\mathrm{C}}\xspace}                 
 \def\PD      {\ensuremath{\mathrm{D}}\xspace}                 
 \def\PE      {\ensuremath{\mathrm{E}}\xspace}                 
 \def\PF      {\ensuremath{\mathrm{F}}\xspace}                 
 \def\PG      {\ensuremath{\mathrm{G}}\xspace}                 
 \def\PH      {\ensuremath{\mathrm{H}}\xspace}                 
 \def\PI      {\ensuremath{\mathrm{I}}\xspace}                 
 \def\PJ      {\ensuremath{\mathrm{J}}\xspace}                 
 \def\PK      {\ensuremath{\mathrm{K}}\xspace}                 
 \def\PL      {\ensuremath{\mathrm{L}}\xspace}                 
 \def\PM      {\ensuremath{\mathrm{M}}\xspace}                 
 \def\PN      {\ensuremath{\mathrm{N}}\xspace}                 
 \def\PO      {\ensuremath{\mathrm{O}}\xspace}                 
 \def\PP      {\ensuremath{\mathrm{P}}\xspace}                 
 \def\PQ      {\ensuremath{\mathrm{Q}}\xspace}                 
 \def\PR      {\ensuremath{\mathrm{R}}\xspace}                 
 \def\PS      {\ensuremath{\mathrm{S}}\xspace}                 
 \def\PT      {\ensuremath{\mathrm{T}}\xspace}                 
 \def\PU      {\ensuremath{\mathrm{U}}\xspace}                 
 \def\PV      {\ensuremath{\mathrm{V}}\xspace}                 
 \def\PW      {\ensuremath{\mathrm{W}}\xspace}                 
 \def\PX      {\ensuremath{\mathrm{X}}\xspace}                 
 \def\PY      {\ensuremath{\mathrm{Y}}\xspace}                 
 \def\PZ      {\ensuremath{\mathrm{Z}}\xspace}                 
 \def\Pa      {\ensuremath{\mathrm{a}}\xspace}                 
 \def\Pb      {\ensuremath{\mathrm{b}}\xspace}                 
 \def\Pc      {\ensuremath{\mathrm{c}}\xspace}                 
 \def\Pd      {\ensuremath{\mathrm{d}}\xspace}                 
 \def\Pe      {\ensuremath{\mathrm{e}}\xspace}                 
 \def\Pf      {\ensuremath{\mathrm{f}}\xspace}                 
 \def\Pg      {\ensuremath{\mathrm{g}}\xspace}                 
 \def\Ph      {\ensuremath{\mathrm{h}}\xspace}                 
 \def\Pi      {\ensuremath{\mathrm{i}}\xspace}                 
 \def\Pj      {\ensuremath{\mathrm{j}}\xspace}                 
 \def\Pk      {\ensuremath{\mathrm{k}}\xspace}                 
 \def\Pl      {\ensuremath{\mathrm{l}}\xspace}                 
 \def\Pm      {\ensuremath{\mathrm{m}}\xspace}                 
 \def\Pn      {\ensuremath{\mathrm{n}}\xspace}                 
 \def\Po      {\ensuremath{\mathrm{o}}\xspace}                 
 \def\Pp      {\ensuremath{\mathrm{p}}\xspace}                 
 \def\Pq      {\ensuremath{\mathrm{q}}\xspace}                 
 \def\Pr      {\ensuremath{\mathrm{r}}\xspace}                 
 \def\Ps      {\ensuremath{\mathrm{s}}\xspace}                 
 \def\Pt      {\ensuremath{\mathrm{t}}\xspace}                 
 \def\Pu      {\ensuremath{\mathrm{u}}\xspace}                 
 \def\Pv      {\ensuremath{\mathrm{v}}\xspace}                 
 \def\Pw      {\ensuremath{\mathrm{w}}\xspace}                 
 \def\Px      {\ensuremath{\mathrm{x}}\xspace}                 
 \def\Py      {\ensuremath{\mathrm{y}}\xspace}                 
 \def\Pz      {\ensuremath{\mathrm{z}}\xspace}                 
}
{\def\Palpha      {\ensuremath{\alpha}\xspace}
 \def\Pbeta       {\ensuremath{\beta}\xspace}
 \def\Pgamma      {\ensuremath{\gamma}\xspace}                 
 \def\Pdelta      {\ensuremath{\delta}\xspace}                 
 \def\Pepsilon    {\ensuremath{\epsilon}\xspace}                 
 \def\Pvarepsilon {\ensuremath{\varepsilon}\xspace}                 
 \def\Pzeta       {\ensuremath{\zeta}\xspace}                 
 \def\Peta        {\ensuremath{\eta}\xspace}                 
 \def\Ptheta      {\ensuremath{\theta}\xspace}                 
 \def\Pvartheta   {\ensuremath{\vartheta}\xspace}                 
 \def\Piota       {\ensuremath{\iota}\xspace}                 
 \def\Pkappa      {\ensuremath{\kappa}\xspace}                 
 \def\Plambda     {\ensuremath{\lambda}\xspace}                 
 \def\Pmu         {\ensuremath{\mu}\xspace}                 
 \def\Pnu         {\ensuremath{\nu}\xspace}                 
 \def\Pxi         {\ensuremath{\xi}\xspace}                 
 \def\Ppi         {\ensuremath{\pi}\xspace}                 
 \def\Pvarpi      {\ensuremath{\varpi}\xspace}                 
 \def\Prho        {\ensuremath{\rho}\xspace}                 
 \def\Pvarrho     {\ensuremath{\varrho}\xspace}                 
 \def\Ptau        {\ensuremath{\tau}\xspace}                 
 \def\Pupsilon    {\ensuremath{\upsilon}\xspace}                 
 \def\Pphi        {\ensuremath{\phi}\xspace}                 
 \def\Pvarphi     {\ensuremath{\varphi}\xspace}                 
 \def\Pchi        {\ensuremath{\chi}\xspace}                 
 \def\Ppsi        {\ensuremath{\psi}\xspace}                 
 \def\Pomega      {\ensuremath{\omega}\xspace}                 
 \mathchardef\PDelta="7101
 \mathchardef\PXi="7104
 \mathchardef\PLambda="7103
 \mathchardef\PSigma="7106
 \mathchardef\POmega="710A
 \mathchardef\PUpsilon="7107
 \def\PA      {\ensuremath{A}\xspace}                 
 \def\PB      {\ensuremath{B}\xspace}                 
 \def\PC      {\ensuremath{C}\xspace}                 
 \def\PD      {\ensuremath{D}\xspace}                 
 \def\PE      {\ensuremath{E}\xspace}                 
 \def\PF      {\ensuremath{F}\xspace}                 
 \def\PG      {\ensuremath{G}\xspace}                 
 \def\PH      {\ensuremath{H}\xspace}                 
 \def\PI      {\ensuremath{I}\xspace}                 
 \def\PJ      {\ensuremath{J}\xspace}                 
 \def\PK      {\ensuremath{K}\xspace}                 
 \def\PL      {\ensuremath{L}\xspace}                 
 \def\PM      {\ensuremath{M}\xspace}                 
 \def\PN      {\ensuremath{N}\xspace}                 
 \def\PO      {\ensuremath{O}\xspace}                 
 \def\PP      {\ensuremath{P}\xspace}                 
 \def\PQ      {\ensuremath{Q}\xspace}                 
 \def\PR      {\ensuremath{R}\xspace}                 
 \def\PS      {\ensuremath{S}\xspace}                 
 \def\PT      {\ensuremath{T}\xspace}                 
 \def\PU      {\ensuremath{U}\xspace}                 
 \def\PV      {\ensuremath{V}\xspace}                 
 \def\PW      {\ensuremath{W}\xspace}                 
 \def\PX      {\ensuremath{X}\xspace}                 
 \def\PY      {\ensuremath{Y}\xspace}                 
 \def\PZ      {\ensuremath{Z}\xspace}                 
 \def\Pa      {\ensuremath{a}\xspace}                 
 \def\Pb      {\ensuremath{b}\xspace}                 
 \def\Pc      {\ensuremath{c}\xspace}                 
 \def\Pd      {\ensuremath{d}\xspace}                 
 \def\Pe      {\ensuremath{e}\xspace}                 
 \def\Pf      {\ensuremath{f}\xspace}                 
 \def\Pg      {\ensuremath{g}\xspace}                 
 \def\Ph      {\ensuremath{h}\xspace}                 
 \def\Pi      {\ensuremath{i}\xspace}                 
 \def\Pj      {\ensuremath{j}\xspace}                 
 \def\Pk      {\ensuremath{k}\xspace}                 
 \def\Pl      {\ensuremath{l}\xspace}                 
 \def\Pm      {\ensuremath{m}\xspace}                 
 \def\Pn      {\ensuremath{n}\xspace}                 
 \def\Po      {\ensuremath{o}\xspace}                 
 \def\Pp      {\ensuremath{p}\xspace}                 
 \def\Pq      {\ensuremath{q}\xspace}                 
 \def\Pr      {\ensuremath{r}\xspace}                 
 \def\Ps      {\ensuremath{s}\xspace}                 
 \def\Pt      {\ensuremath{t}\xspace}                 
 \def\Pu      {\ensuremath{u}\xspace}                 
 \def\Pv      {\ensuremath{v}\xspace}                 
 \def\Pw      {\ensuremath{w}\xspace}                 
 \def\Px      {\ensuremath{x}\xspace}                 
 \def\Py      {\ensuremath{y}\xspace}                 
 \def\Pz      {\ensuremath{z}\xspace}                 
}

%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
% Particles
\makeatletter
\ifcase \@ptsize \relax% 10pt
  \newcommand{\miniscule}{\@setfontsize\miniscule{4}{5}}% \tiny: 5/6
\or% 11pt
  \newcommand{\miniscule}{\@setfontsize\miniscule{5}{6}}% \tiny: 6/7
\or% 12pt
  \newcommand{\miniscule}{\@setfontsize\miniscule{5}{6}}% \tiny: 6/7
\fi
\makeatother


\DeclareRobustCommand{\optbar}[1]{\shortstack{{\miniscule (\rule[.5ex]{1.25em}{.18mm})}
  \\ [-.7ex] $#1$}}


%% Leptons

\let\emi\en
\def\electron   {{\ensuremath{\Pe}}\xspace}
\def\en         {{\ensuremath{\Pe^-}}\xspace}   % electron negative (\em is taken)
\def\ep         {{\ensuremath{\Pe^+}}\xspace}
\def\epm        {{\ensuremath{\Pe^\pm}}\xspace} 
\def\epem       {{\ensuremath{\Pe^+\Pe^-}}\xspace}
%%%\def\ee         {\ensuremath{\Pe^-\Pe^-}\xspace}

\def\muon       {{\ensuremath{\Pmu}}\xspace}
\def\mup        {{\ensuremath{\Pmu^+}}\xspace}
\def\mun        {{\ensuremath{\Pmu^-}}\xspace} % muon negative (\mum is taken)
\def\mumu       {{\ensuremath{\Pmu^+\Pmu^-}}\xspace}

\def\tauon      {{\ensuremath{\Ptau}}\xspace}
\def\taup       {{\ensuremath{\Ptau^+}}\xspace}
\def\taum       {{\ensuremath{\Ptau^-}}\xspace}
\def\tautau     {{\ensuremath{\Ptau^+\Ptau^-}}\xspace}

\def\lepton     {{\ensuremath{\ell}}\xspace}
\def\ellm       {{\ensuremath{\ell^-}}\xspace}
\def\ellp       {{\ensuremath{\ell^+}}\xspace}
%%%\def\ellell     {\ensuremath{\ell^+ \ell^-}\xspace}

\def\neu        {{\ensuremath{\Pnu}}\xspace}
\def\neub       {{\ensuremath{\overline{\Pnu}}}\xspace}
%%%\def\nuenueb    {\ensuremath{\neu\neub}\xspace}
\def\neue       {{\ensuremath{\neu_e}}\xspace}
\def\neueb      {{\ensuremath{\neub_e}}\xspace}
%%%\def\neueneueb  {\ensuremath{\neue\neueb}\xspace}
\def\neum       {{\ensuremath{\neu_\mu}}\xspace}
\def\neumb      {{\ensuremath{\neub_\mu}}\xspace}
%%%\def\neumneumb  {\ensuremath{\neum\neumb}\xspace}
\def\neut       {{\ensuremath{\neu_\tau}}\xspace}
\def\neutb      {{\ensuremath{\neub_\tau}}\xspace}
%%%\def\neutneutb  {\ensuremath{\neut\neutb}\xspace}
\def\neul       {{\ensuremath{\neu_\ell}}\xspace}
\def\neulb      {{\ensuremath{\neub_\ell}}\xspace}
%%%\def\neulneulb  {\ensuremath{\neul\neulb}\xspace}

%% Gauge bosons and scalars

\def\g      {{\ensuremath{\Pgamma}}\xspace}
\def\H      {{\ensuremath{\PH^0}}\xspace}
\def\Hp     {{\ensuremath{\PH^+}}\xspace}
\def\Hm     {{\ensuremath{\PH^-}}\xspace}
\def\Hpm    {{\ensuremath{\PH^\pm}}\xspace}
\def\W      {{\ensuremath{\PW}}\xspace}
\def\Wp     {{\ensuremath{\PW^+}}\xspace}
\def\Wm     {{\ensuremath{\PW^-}}\xspace}
\def\Wpm    {{\ensuremath{\PW^\pm}}\xspace}
\def\Z      {{\ensuremath{\PZ}}\xspace}

%% Quarks

\def\quark     {{\ensuremath{\Pq}}\xspace}
\def\quarkbar  {{\ensuremath{\overline \quark}}\xspace}
\def\qqbar     {{\ensuremath{\quark\quarkbar}}\xspace}
\def\uquark    {{\ensuremath{\Pu}}\xspace}
\def\uquarkbar {{\ensuremath{\overline \uquark}}\xspace}
\def\uubar     {{\ensuremath{\uquark\uquarkbar}}\xspace}
\def\dquark    {{\ensuremath{\Pd}}\xspace}
\def\dquarkbar {{\ensuremath{\overline \dquark}}\xspace}
\def\ddbar     {{\ensuremath{\dquark\dquarkbar}}\xspace}
\def\squark    {{\ensuremath{\Ps}}\xspace}
\def\squarkbar {{\ensuremath{\overline \squark}}\xspace}
\def\ssbar     {{\ensuremath{\squark\squarkbar}}\xspace}
\def\cquark    {{\ensuremath{\Pc}}\xspace}
\def\cquarkbar {{\ensuremath{\overline \cquark}}\xspace}
\def\ccbar     {{\ensuremath{\cquark\cquarkbar}}\xspace}
\def\bquark    {{\ensuremath{\Pb}}\xspace}
\def\bquarkbar {{\ensuremath{\overline \bquark}}\xspace}
\def\bbbar     {{\ensuremath{\bquark\bquarkbar}}\xspace}
\def\tquark    {{\ensuremath{\Pt}}\xspace}
\def\tquarkbar {{\ensuremath{\overline \tquark}}\xspace}
\def\ttbar     {{\ensuremath{\tquark\tquarkbar}}\xspace}

%% Light mesons

\def\hadron {{\ensuremath{\Ph}}\xspace}
\def\pion   {{\ensuremath{\Ppi}}\xspace}
\def\piz    {{\ensuremath{\pion^0}}\xspace}
\def\pizs   {{\ensuremath{\pion^0\mbox\,\rm{s}}}\xspace}
\def\pip    {{\ensuremath{\pion^+}}\xspace}
\def\pim    {{\ensuremath{\pion^-}}\xspace}
\def\pipm   {{\ensuremath{\pion^\pm}}\xspace}
\def\pimp   {{\ensuremath{\pion^\mp}}\xspace}

\def\rhomeson {{\ensuremath{\Prho}}\xspace}
\def\rhoz     {{\ensuremath{\rhomeson^0}}\xspace}
\def\rhop     {{\ensuremath{\rhomeson^+}}\xspace}
\def\rhom     {{\ensuremath{\rhomeson^-}}\xspace}
\def\rhopm    {{\ensuremath{\rhomeson^\pm}}\xspace}
\def\rhomp    {{\ensuremath{\rhomeson^\mp}}\xspace}

\def\kaon    {{\ensuremath{\PK}}\xspace}
%%% do NOT use ensuremath here
  \def\Kbar    {{\kern 0.2em\overline{\kern -0.2em \PK}{}}\xspace}
\def\Kb      {{\ensuremath{\Kbar}}\xspace}
\def\KorKbar    {\kern 0.18em\optbar{\kern -0.18em K}{}\xspace}
\def\Kz      {{\ensuremath{\kaon^0}}\xspace}
\def\Kzb     {{\ensuremath{\Kbar{}^0}}\xspace}
\def\Kp      {{\ensuremath{\kaon^+}}\xspace}
\def\Km      {{\ensuremath{\kaon^-}}\xspace}
\def\Kpm     {{\ensuremath{\kaon^\pm}}\xspace}
\def\Kmp     {{\ensuremath{\kaon^\mp}}\xspace}
\def\KS      {{\ensuremath{\kaon^0_{\rm\scriptscriptstyle S}}}\xspace}
\def\KL      {{\ensuremath{\kaon^0_{\rm\scriptscriptstyle L}}}\xspace}
\def\Kstarz  {{\ensuremath{\kaon^{*0}}}\xspace}
\def\Kstarzb {{\ensuremath{\Kbar{}^{*0}}}\xspace}
\def\Kstar   {{\ensuremath{\kaon^*}}\xspace}
\def\Kstarb  {{\ensuremath{\Kbar{}^*}}\xspace}
\def\Kstarp  {{\ensuremath{\kaon^{*+}}}\xspace}
\def\Kstarm  {{\ensuremath{\kaon^{*-}}}\xspace}
\def\Kstarpm {{\ensuremath{\kaon^{*\pm}}}\xspace}
\def\Kstarmp {{\ensuremath{\kaon^{*\mp}}}\xspace}

\newcommand{\etaz}{\ensuremath{\Peta}\xspace}
\newcommand{\etapr}{\ensuremath{\Peta^{\prime}}\xspace}
\newcommand{\phiz}{\ensuremath{\Pphi}\xspace}
\newcommand{\omegaz}{\ensuremath{\Pomega}\xspace}

%% Heavy mesons

%%% do NOT use ensuremath here
  \def\Dbar    {{\kern 0.2em\overline{\kern -0.2em \PD}{}}\xspace}
\def\D       {{\ensuremath{\PD}}\xspace}
\def\Db      {{\ensuremath{\Dbar}}\xspace}
\def\DorDbar    {\kern 0.18em\optbar{\kern -0.18em D}{}\xspace}
\def\Dz      {{\ensuremath{\D^0}}\xspace}
\def\Dzb     {{\ensuremath{\Dbar{}^0}}\xspace}
\def\Dp      {{\ensuremath{\D^+}}\xspace}
\def\Dm      {{\ensuremath{\D^-}}\xspace}
\def\Dpm     {{\ensuremath{\D^\pm}}\xspace}
\def\Dmp     {{\ensuremath{\D^\mp}}\xspace}
\def\Dstar   {{\ensuremath{\D^*}}\xspace}
\def\Dstarb  {{\ensuremath{\Dbar{}^*}}\xspace}
\def\Dstarz  {{\ensuremath{\D^{*0}}}\xspace}
\def\Dstarzb {{\ensuremath{\Dbar{}^{*0}}}\xspace}
\def\Dstarp  {{\ensuremath{\D^{*+}}}\xspace}
\def\Dstarm  {{\ensuremath{\D^{*-}}}\xspace}
\def\Dstarpm {{\ensuremath{\D^{*\pm}}}\xspace}
\def\Dstarmp {{\ensuremath{\D^{*\mp}}}\xspace}
\def\Ds      {{\ensuremath{\D^+_\squark}}\xspace}
\def\Dsp     {{\ensuremath{\D^+_\squark}}\xspace}
\def\Dsm     {{\ensuremath{\D^-_\squark}}\xspace}
\def\Dspm    {{\ensuremath{\D^{\pm}_\squark}}\xspace}
\def\Dsmp    {{\ensuremath{\D^{\mp}_\squark}}\xspace}
\def\Dss     {{\ensuremath{\D^{*+}_\squark}}\xspace}
\def\Dssp    {{\ensuremath{\D^{*+}_\squark}}\xspace}
\def\Dssm    {{\ensuremath{\D^{*-}_\squark}}\xspace}
\def\Dsspm   {{\ensuremath{\D^{*\pm}_\squark}}\xspace}
\def\Dssmp   {{\ensuremath{\D^{*\mp}_\squark}}\xspace}

\def\B       {{\ensuremath{\PB}}\xspace}
%%% do NOT use ensuremath here
\def\Bbar    {{\ensuremath{\kern 0.18em\overline{\kern -0.18em \PB}{}}}\xspace}
\def\Bb      {{\ensuremath{\Bbar}}\xspace}
\def\BorBbar    {\kern 0.18em\optbar{\kern -0.18em B}{}\xspace}
\def\Bz      {{\ensuremath{\B^0}}\xspace}
\def\Bzb     {{\ensuremath{\Bbar{}^0}}\xspace}
\def\Bu      {{\ensuremath{\B^+}}\xspace}
\def\Bub     {{\ensuremath{\B^-}}\xspace}
\def\Bp      {{\ensuremath{\Bu}}\xspace}
\def\Bm      {{\ensuremath{\Bub}}\xspace}
\def\Bpm     {{\ensuremath{\B^\pm}}\xspace}
\def\Bmp     {{\ensuremath{\B^\mp}}\xspace}
\def\Bd      {{\ensuremath{\B^0}}\xspace}
\def\Bs      {{\ensuremath{\B^0_\squark}}\xspace}
\def\Bsb     {{\ensuremath{\Bbar{}^0_\squark}}\xspace}
\def\Bdb     {{\ensuremath{\Bbar{}^0}}\xspace}
\def\Bc      {{\ensuremath{\B_\cquark^+}}\xspace}
\def\Bcp     {{\ensuremath{\B_\cquark^+}}\xspace}
\def\Bcm     {{\ensuremath{\B_\cquark^-}}\xspace}
\def\Bcpm    {{\ensuremath{\B_\cquark^\pm}}\xspace}

%% Onia

\def\jpsi     {{\ensuremath{{\PJ\mskip -3mu/\mskip -2mu\Ppsi\mskip 2mu}}}\xspace}
\def\psitwos  {{\ensuremath{\Ppsi{(2S)}}}\xspace}
\def\psiprpr  {{\ensuremath{\Ppsi(3770)}}\xspace}
\def\etac     {{\ensuremath{\Peta_\cquark}}\xspace}
\def\chiczero {{\ensuremath{\Pchi_{\cquark 0}}}\xspace}
\def\chicone  {{\ensuremath{\Pchi_{\cquark 1}}}\xspace}
\def\chictwo  {{\ensuremath{\Pchi_{\cquark 2}}}\xspace}
  %\mathchardef\Upsilon="7107
  \def\Y#1S{\ensuremath{\PUpsilon{(#1S)}}\xspace}% no space before {...}!
\def\OneS  {{\Y1S}}
\def\TwoS  {{\Y2S}}
\def\ThreeS{{\Y3S}}
\def\FourS {{\Y4S}}
\def\FiveS {{\Y5S}}

\def\chic  {{\ensuremath{\Pchi_{c}}}\xspace}

%% Baryons

\def\proton      {{\ensuremath{\Pp}}\xspace}
\def\antiproton  {{\ensuremath{\overline \proton}}\xspace}
\def\neutron     {{\ensuremath{\Pn}}\xspace}
\def\antineutron {{\ensuremath{\overline \neutron}}\xspace}
\def\Deltares    {{\ensuremath{\PDelta}}\xspace}
\def\Deltaresbar {{\ensuremath{\overline \Deltares}}\xspace}
\def\Xires       {{\ensuremath{\PXi}}\xspace}
\def\Xiresbar    {{\ensuremath{\overline \Xires}}\xspace}
\def\Lz          {{\ensuremath{\PLambda}}\xspace}
\def\Lbar        {{\ensuremath{\kern 0.1em\overline{\kern -0.1em\PLambda}}}\xspace}
\def\LorLbar    {\kern 0.18em\optbar{\kern -0.18em \PLambda}{}\xspace}
\def\Lambdares   {{\ensuremath{\PLambda}}\xspace}
\def\Lambdaresbar{{\ensuremath{\Lbar}}\xspace}
\def\Sigmares    {{\ensuremath{\PSigma}}\xspace}
\def\Sigmaresbar {{\ensuremath{\overline \Sigmares}}\xspace}
\def\Omegares    {{\ensuremath{\POmega}}\xspace}
\def\Omegaresbar {{\ensuremath{\overline \POmega}}\xspace}

%%% do NOT use ensuremath here
 % \def\Deltabar{\kern 0.25em\overline{\kern -0.25em \Deltares}{}\xspace}
 % \def\Sigbar{\kern 0.2em\overline{\kern -0.2em \Sigma}{}\xspace}
 % \def\Xibar{\kern 0.2em\overline{\kern -0.2em \Xi}{}\xspace}
 % \def\Obar{\kern 0.2em\overline{\kern -0.2em \Omega}{}\xspace}
 % \def\Nbar{\kern 0.2em\overline{\kern -0.2em N}{}\xspace}
 % \def\Xb{\kern 0.2em\overline{\kern -0.2em X}{}\xspace}

\def\Lb      {{\ensuremath{\Lz^0_\bquark}}\xspace}
\def\Lbbar   {{\ensuremath{\Lbar{}^0_\bquark}}\xspace}
\def\Lc      {{\ensuremath{\Lz^+_\cquark}}\xspace}
\def\Lcbar   {{\ensuremath{\Lbar{}^-_\cquark}}\xspace}
\def\Xibz    {{\ensuremath{\Xires^0_\bquark}}\xspace}
\def\Xibm    {{\ensuremath{\Xires^-_\bquark}}\xspace}
\def\Xibbarz {{\ensuremath{\Xiresbar{}_\bquark^0}}\xspace}
\def\Xibbarp {{\ensuremath{\Xiresbar{}_\bquark^+}}\xspace}
\def\Xicz    {{\ensuremath{\Xires^0_\cquark}}\xspace}
\def\Xicp    {{\ensuremath{\Xires^+_\cquark}}\xspace}
\def\Xicbarz {{\ensuremath{\Xiresbar{}_\cquark^0}}\xspace}
\def\Xicbarm {{\ensuremath{\Xiresbar{}_\cquark^-}}\xspace}
\def\Omegac    {{\ensuremath{\Omegares^0_\cquark}}\xspace}
\def\Omegacbar {{\ensuremath{\Omegaresbar{}_\cquark^0}}\xspace}
\def\Omegab    {{\ensuremath{\Omegares^-_\bquark}}\xspace}
\def\Omegabbar {{\ensuremath{\Omegaresbar{}_\bquark^+}}\xspace}

%%%%%%%%%%%%%%%%%%
% Physics symbols
%%%%%%%%%%%%%%%%%

%% Decays
\def\BF         {{\ensuremath{\cal B}}\xspace}
\def\BRvis      {{\ensuremath{\BR_{\rm{vis}}}}}
\def\BR         {\BF}
\newcommand{\decay}[2]{\ensuremath{#1\!\to #2}\xspace}         % {\Pa}{\Pb \Pc}
\def\ra                 {\ensuremath{\rightarrow}\xspace}
\def\to                 {\ensuremath{\rightarrow}\xspace}

%% Lifetimes
\newcommand{\tauBs}{{\ensuremath{\tau_{\Bs}}}\xspace}
\newcommand{\tauBd}{{\ensuremath{\tau_{\Bd}}}\xspace}
\newcommand{\tauBz}{{\ensuremath{\tau_{\Bz}}}\xspace}
\newcommand{\tauBu}{{\ensuremath{\tau_{\Bp}}}\xspace}
\newcommand{\tauDp}{{\ensuremath{\tau_{\Dp}}}\xspace}
\newcommand{\tauDz}{{\ensuremath{\tau_{\Dz}}}\xspace}
\newcommand{\tauL}{{\ensuremath{\tau_{\rm L}}}\xspace}
\newcommand{\tauH}{{\ensuremath{\tau_{\rm H}}}\xspace}

%% Masses
\newcommand{\mBd}{{\ensuremath{m_{\Bd}}}\xspace}
\newcommand{\mBp}{{\ensuremath{m_{\Bp}}}\xspace}
\newcommand{\mBs}{{\ensuremath{m_{\Bs}}}\xspace}
\newcommand{\mBc}{{\ensuremath{m_{\Bc}}}\xspace}
\newcommand{\mLb}{{\ensuremath{m_{\Lb}}}\xspace}

%% EW theory, groups
\def\grpsuthree {{\ensuremath{\mathrm{SU}(3)}}\xspace}
\def\grpsutw    {{\ensuremath{\mathrm{SU}(2)}}\xspace}
\def\grpuone    {{\ensuremath{\mathrm{U}(1)}}\xspace}

\def\ssqtw   {{\ensuremath{\sin^{2}\!\theta_{\mathrm{W}}}}\xspace}
\def\csqtw   {{\ensuremath{\cos^{2}\!\theta_{\mathrm{W}}}}\xspace}
\def\stw     {{\ensuremath{\sin\theta_{\mathrm{W}}}}\xspace}
\def\ctw     {{\ensuremath{\cos\theta_{\mathrm{W}}}}\xspace}
\def\ssqtwef {{\ensuremath{{\sin}^{2}\theta_{\mathrm{W}}^{\mathrm{eff}}}}\xspace}
\def\csqtwef {{\ensuremath{{\cos}^{2}\theta_{\mathrm{W}}^{\mathrm{eff}}}}\xspace}
\def\stwef   {{\ensuremath{\sin\theta_{\mathrm{W}}^{\mathrm{eff}}}}\xspace}
\def\ctwef   {{\ensuremath{\cos\theta_{\mathrm{W}}^{\mathrm{eff}}}}\xspace}
\def\gv      {{\ensuremath{g_{\mbox{\tiny V}}}}\xspace}
\def\ga      {{\ensuremath{g_{\mbox{\tiny A}}}}\xspace}

\def\order   {{\ensuremath{\mathcal{O}}}\xspace}
\def\ordalph {{\ensuremath{\mathcal{O}(\alpha)}}\xspace}
\def\ordalsq {{\ensuremath{\mathcal{O}(\alpha^{2})}}\xspace}
\def\ordalcb {{\ensuremath{\mathcal{O}(\alpha^{3})}}\xspace}

%% QCD parameters
\newcommand{\as}{{\ensuremath{\alpha_s}}\xspace}
\newcommand{\MSb}{{\ensuremath{\overline{\mathrm{MS}}}}\xspace}
\newcommand{\lqcd}{{\ensuremath{\Lambda_{\mathrm{QCD}}}}\xspace}
\def\qsq       {{\ensuremath{q^2}}\xspace}

%% CKM, CP violation

\def\eps   {{\ensuremath{\varepsilon}}\xspace}
\def\epsK  {{\ensuremath{\varepsilon_K}}\xspace}
\def\epsB  {{\ensuremath{\varepsilon_B}}\xspace}
\def\epsp  {{\ensuremath{\varepsilon^\prime_K}}\xspace}

\def\CP                {{\ensuremath{C\!P}}\xspace}
\def\CPT               {{\ensuremath{C\!PT}}\xspace}

\def\rhobar {{\ensuremath{\overline \rho}}\xspace}
\def\etabar {{\ensuremath{\overline \eta}}\xspace}

\def\Vud  {{\ensuremath{V_{\uquark\dquark}}}\xspace}
\def\Vcd  {{\ensuremath{V_{\cquark\dquark}}}\xspace}
\def\Vtd  {{\ensuremath{V_{\tquark\dquark}}}\xspace}
\def\Vus  {{\ensuremath{V_{\uquark\squark}}}\xspace}
\def\Vcs  {{\ensuremath{V_{\cquark\squark}}}\xspace}
\def\Vts  {{\ensuremath{V_{\tquark\squark}}}\xspace}
\def\Vub  {{\ensuremath{V_{\uquark\bquark}}}\xspace}
\def\Vcb  {{\ensuremath{V_{\cquark\bquark}}}\xspace}
\def\Vtb  {{\ensuremath{V_{\tquark\bquark}}}\xspace}
\def\Vuds  {{\ensuremath{V_{\uquark\dquark}^\ast}}\xspace}
\def\Vcds  {{\ensuremath{V_{\cquark\dquark}^\ast}}\xspace}
\def\Vtds  {{\ensuremath{V_{\tquark\dquark}^\ast}}\xspace}
\def\Vuss  {{\ensuremath{V_{\uquark\squark}^\ast}}\xspace}
\def\Vcss  {{\ensuremath{V_{\cquark\squark}^\ast}}\xspace}
\def\Vtss  {{\ensuremath{V_{\tquark\squark}^\ast}}\xspace}
\def\Vubs  {{\ensuremath{V_{\uquark\bquark}^\ast}}\xspace}
\def\Vcbs  {{\ensuremath{V_{\cquark\bquark}^\ast}}\xspace}
\def\Vtbs  {{\ensuremath{V_{\tquark\bquark}^\ast}}\xspace}

%% Oscillations

\newcommand{\dm}{{\ensuremath{\Delta m}}\xspace}
\newcommand{\dms}{{\ensuremath{\Delta m_{\squark}}}\xspace}
\newcommand{\dmd}{{\ensuremath{\Delta m_{\dquark}}}\xspace}
\newcommand{\DG}{{\ensuremath{\Delta\Gamma}}\xspace}
\newcommand{\DGs}{{\ensuremath{\Delta\Gamma_{\squark}}}\xspace}
\newcommand{\DGd}{{\ensuremath{\Delta\Gamma_{\dquark}}}\xspace}
\newcommand{\Gs}{{\ensuremath{\Gamma_{\squark}}}\xspace}
\newcommand{\Gd}{{\ensuremath{\Gamma_{\dquark}}}\xspace}
\newcommand{\MBq}{{\ensuremath{M_{\B_\quark}}}\xspace}
\newcommand{\DGq}{{\ensuremath{\Delta\Gamma_{\quark}}}\xspace}
\newcommand{\Gq}{{\ensuremath{\Gamma_{\quark}}}\xspace}
\newcommand{\dmq}{{\ensuremath{\Delta m_{\quark}}}\xspace}
\newcommand{\GL}{{\ensuremath{\Gamma_{\rm L}}}\xspace}
\newcommand{\GH}{{\ensuremath{\Gamma_{\rm H}}}\xspace}
\newcommand{\DGsGs}{{\ensuremath{\Delta\Gamma_{\squark}/\Gamma_{\squark}}}\xspace}
\newcommand{\Delm}{{\mbox{$\Delta m $}}\xspace}
\newcommand{\ACP}{{\ensuremath{{\cal A}^{\CP}}}\xspace}
\newcommand{\Adir}{{\ensuremath{{\cal A}^{\rm dir}}}\xspace}
\newcommand{\Amix}{{\ensuremath{{\cal A}^{\rm mix}}}\xspace}
\newcommand{\ADelta}{{\ensuremath{{\cal A}^\Delta}}\xspace}
\newcommand{\phid}{{\ensuremath{\phi_{\dquark}}}\xspace}
\newcommand{\sinphid}{{\ensuremath{\sin\!\phid}}\xspace}
\newcommand{\phis}{{\ensuremath{\phi_{\squark}}}\xspace}
\newcommand{\betas}{{\ensuremath{\beta_{\squark}}}\xspace}
\newcommand{\sbetas}{{\ensuremath{\sigma(\beta_{\squark})}}\xspace}
\newcommand{\stbetas}{{\ensuremath{\sigma(2\beta_{\squark})}}\xspace}
\newcommand{\stphis}{{\ensuremath{\sigma(\phi_{\squark})}}\xspace}
\newcommand{\sinphis}{{\ensuremath{\sin\!\phis}}\xspace}

%% Tagging
\newcommand{\edet}{{\ensuremath{\varepsilon_{\rm det}}}\xspace}
\newcommand{\erec}{{\ensuremath{\varepsilon_{\rm rec/det}}}\xspace}
\newcommand{\esel}{{\ensuremath{\varepsilon_{\rm sel/rec}}}\xspace}
\newcommand{\etrg}{{\ensuremath{\varepsilon_{\rm trg/sel}}}\xspace}
\newcommand{\etot}{{\ensuremath{\varepsilon_{\rm tot}}}\xspace}

\newcommand{\mistag}{\ensuremath{\omega}\xspace}
\newcommand{\wcomb}{\ensuremath{\omega^{\rm comb}}\xspace}
\newcommand{\etag}{{\ensuremath{\varepsilon_{\rm tag}}}\xspace}
\newcommand{\etagcomb}{{\ensuremath{\varepsilon_{\rm tag}^{\rm comb}}}\xspace}
\newcommand{\effeff}{\ensuremath{\varepsilon_{\rm eff}}\xspace}
\newcommand{\effeffcomb}{\ensuremath{\varepsilon_{\rm eff}^{\rm comb}}\xspace}
\newcommand{\efftag}{{\ensuremath{\etag(1-2\omega)^2}}\xspace}
\newcommand{\effD}{{\ensuremath{\etag D^2}}\xspace}

\newcommand{\etagprompt}{{\ensuremath{\varepsilon_{\rm tag}^{\rm Pr}}}\xspace}
\newcommand{\etagLL}{{\ensuremath{\varepsilon_{\rm tag}^{\rm LL}}}\xspace}

%% Key decay channels

\def\BdToKstmm    {\decay{\Bd}{\Kstarz\mup\mun}}
\def\BdbToKstmm   {\decay{\Bdb}{\Kstarzb\mup\mun}}

\def\BsToJPsiPhi  {\decay{\Bs}{\jpsi\phi}}
\def\BdToJPsiKst  {\decay{\Bd}{\jpsi\Kstarz}}
\def\BdbToJPsiKst {\decay{\Bdb}{\jpsi\Kstarzb}}

\def\BsPhiGam     {\decay{\Bs}{\phi \g}}
\def\BdKstGam     {\decay{\Bd}{\Kstarz \g}}

\def\BTohh        {\decay{\B}{\Ph^+ \Ph'^-}}
\def\BdTopipi     {\decay{\Bd}{\pip\pim}}
\def\BdToKpi      {\decay{\Bd}{\Kp\pim}}
\def\BsToKK       {\decay{\Bs}{\Kp\Km}}
\def\BsTopiK      {\decay{\Bs}{\pip\Km}}

%% Rare decays
\def\BdKstee  {\decay{\Bd}{\Kstarz\epem}}
\def\BdbKstee {\decay{\Bdb}{\Kstarzb\epem}}
\def\bsll     {\decay{\bquark}{\squark \ell^+ \ell^-}}
\def\AFB      {\ensuremath{A_{\mathrm{FB}}}\xspace}
\def\FL       {\ensuremath{F_{\mathrm{L}}}\xspace}
\def\AT#1     {\ensuremath{A_{\mathrm{T}}^{#1}}\xspace}           % 2
\def\btosgam  {\decay{\bquark}{\squark \g}}
\def\btodgam  {\decay{\bquark}{\dquark \g}}
\def\Bsmm     {\decay{\Bs}{\mup\mun}}
\def\Bdmm     {\decay{\Bd}{\mup\mun}}
\def\ctl       {\ensuremath{\cos{\theta_\ell}}\xspace}
\def\ctk       {\ensuremath{\cos{\theta_K}}\xspace}

%% Wilson coefficients and operators
\def\C#1      {\ensuremath{\mathcal{C}_{#1}}\xspace}                       % 9
\def\Cp#1     {\ensuremath{\mathcal{C}_{#1}^{'}}\xspace}                    % 7
\def\Ceff#1   {\ensuremath{\mathcal{C}_{#1}^{\mathrm{(eff)}}}\xspace}        % 9  
\def\Cpeff#1  {\ensuremath{\mathcal{C}_{#1}^{'\mathrm{(eff)}}}\xspace}       % 7
\def\Ope#1    {\ensuremath{\mathcal{O}_{#1}}\xspace}                       % 2
\def\Opep#1   {\ensuremath{\mathcal{O}_{#1}^{'}}\xspace}                    % 7

%% Charm

\def\xprime     {\ensuremath{x^{\prime}}\xspace}
\def\yprime     {\ensuremath{y^{\prime}}\xspace}
\def\ycp        {\ensuremath{y_{\CP}}\xspace}
\def\agamma     {\ensuremath{A_{\Gamma}}\xspace}
%%%\def\kpi        {\ensuremath{\PK\Ppi}\xspace}
%%%\def\kk         {\ensuremath{\PK\PK}\xspace}
%%%\def\dkpi       {\decay{\PD}{\PK\Ppi}}
%%%\def\dkk        {\decay{\PD}{\PK\PK}}
\def\dkpicf     {\decay{\Dz}{\Km\pip}}

%% QM
\newcommand{\bra}[1]{\ensuremath{\langle #1|}}             % {a}
\newcommand{\ket}[1]{\ensuremath{|#1\rangle}}              % {b}
\newcommand{\braket}[2]{\ensuremath{\langle #1|#2\rangle}} % {a}{b}

%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
% Units
%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
\newcommand{\unit}[1]{\ensuremath{\rm\,#1}\xspace}          % {kg}

%% Energy and momentum
\newcommand{\tev}{\ifthenelse{\boolean{inbibliography}}{\ensuremath{~T\kern -0.05em eV}\xspace}{\ensuremath{\mathrm{\,Te\kern -0.1em V}}}\xspace}
\newcommand{\gev}{\ensuremath{\mathrm{\,Ge\kern -0.1em V}}\xspace}
\newcommand{\mev}{\ensuremath{\mathrm{\,Me\kern -0.1em V}}\xspace}
\newcommand{\kev}{\ensuremath{\mathrm{\,ke\kern -0.1em V}}\xspace}
\newcommand{\ev}{\ensuremath{\mathrm{\,e\kern -0.1em V}}\xspace}
\newcommand{\gevc}{\ensuremath{{\mathrm{\,Ge\kern -0.1em V\!/}c}}\xspace}
\newcommand{\mevc}{\ensuremath{{\mathrm{\,Me\kern -0.1em V\!/}c}}\xspace}
\newcommand{\gevcc}{\ensuremath{{\mathrm{\,Ge\kern -0.1em V\!/}c^2}}\xspace}
\newcommand{\gevgevcccc}{\ensuremath{{\mathrm{\,Ge\kern -0.1em V^2\!/}c^4}}\xspace}
\newcommand{\mevcc}{\ensuremath{{\mathrm{\,Me\kern -0.1em V\!/}c^2}}\xspace}

%% Distance and area
\def\km   {\ensuremath{\rm \,km}\xspace}
\def\m    {\ensuremath{\rm \,m}\xspace}
\def\ma   {\ensuremath{{\rm \,m}^2}\xspace}
\def\cm   {\ensuremath{\rm \,cm}\xspace}
\def\cma  {\ensuremath{{\rm \,cm}^2}\xspace}
\def\mm   {\ensuremath{\rm \,mm}\xspace}
\def\mma  {\ensuremath{{\rm \,mm}^2}\xspace}
\def\mum  {\ensuremath{{\,\upmu\rm m}}\xspace}
\def\muma {\ensuremath{{\,\upmu\rm m^2}}\xspace}
\def\nm   {\ensuremath{\rm \,nm}\xspace}
\def\fm   {\ensuremath{\rm \,fm}\xspace}
\def\barn{\ensuremath{\rm \,b}\xspace}
%%%\def\barnhyph{\ensuremath{\rm -b}\xspace}
\def\mbarn{\ensuremath{\rm \,mb}\xspace}
\def\mub{\ensuremath{{\rm \,\upmu b}}\xspace}
%%%\def\mbarnhyph{\ensuremath{\rm -mb}\xspace}
\def\nb {\ensuremath{\rm \,nb}\xspace}
\def\invnb {\ensuremath{\mbox{\,nb}^{-1}}\xspace}
\def\pb {\ensuremath{\rm \,pb}\xspace}
\def\invpb {\ensuremath{\mbox{\,pb}^{-1}}\xspace}
\def\fb   {\ensuremath{\mbox{\,fb}}\xspace}
\def\invfb   {\ensuremath{\mbox{\,fb}^{-1}}\xspace}

%% Time 
\def\sec  {\ensuremath{\rm {\,s}}\xspace}
\def\ms   {\ensuremath{{\rm \,ms}}\xspace}
\def\mus  {\ensuremath{{\,\upmu{\rm s}}}\xspace}
\def\ns   {\ensuremath{{\rm \,ns}}\xspace}
\def\ps   {\ensuremath{{\rm \,ps}}\xspace}
\def\fs   {\ensuremath{\rm \,fs}\xspace}

\def\mhz  {\ensuremath{{\rm \,MHz}}\xspace}
\def\khz  {\ensuremath{{\rm \,kHz}}\xspace}
\def\hz   {\ensuremath{{\rm \,Hz}}\xspace}

\def\invps{\ensuremath{{\rm \,ps^{-1}}}\xspace}

\def\yr   {\ensuremath{\rm \,yr}\xspace}
\def\hr   {\ensuremath{\rm \,hr}\xspace}

%% Temperature
\def\degc {\ensuremath{^\circ}{C}\xspace}
\def\degk {\ensuremath {\rm K}\xspace}

%% Material lengths, radiation
\def\Xrad {\ensuremath{X_0}\xspace}
\def\NIL{\ensuremath{\lambda_{int}}\xspace}
\def\mip {MIP\xspace}
\def\neutroneq {\ensuremath{\rm \,n_{eq}}\xspace}
\def\neqcmcm {\ensuremath{\rm \,n_{eq} / cm^2}\xspace}
\def\kRad {\ensuremath{\rm \,kRad}\xspace}
\def\MRad {\ensuremath{\rm \,MRad}\xspace}
\def\ci {\ensuremath{\rm \,Ci}\xspace}
\def\mci {\ensuremath{\rm \,mCi}\xspace}

%% Uncertainties
\def\sx    {\ensuremath{\sigma_x}\xspace}    
\def\sy    {\ensuremath{\sigma_y}\xspace}   
\def\sz    {\ensuremath{\sigma_z}\xspace}    

\newcommand{\stat}{\ensuremath{\mathrm{\,(stat)}}\xspace}
\newcommand{\syst}{\ensuremath{\mathrm{\,(syst)}}\xspace}

%% Maths

\def\order{{\ensuremath{\cal O}}\xspace}
\newcommand{\chisq}{\ensuremath{\chi^2}\xspace}
\newcommand{\chisqndf}{\ensuremath{\chi^2/\mathrm{ndf}}\xspace}
\newcommand{\chisqip}{\ensuremath{\chi^2_{\rm IP}}\xspace}
\newcommand{\chisqvs}{\ensuremath{\chi^2_{\rm VS}}\xspace}
\newcommand{\chisqvtx}{\ensuremath{\chi^2_{\rm vtx}}\xspace}

\def\deriv {\ensuremath{\mathrm{d}}}

\def\gsim{{~\raise.15em\hbox{$>$}\kern-.85em
          \lower.35em\hbox{$\sim$}~}\xspace}
\def\lsim{{~\raise.15em\hbox{$<$}\kern-.85em
          \lower.35em\hbox{$\sim$}~}\xspace}

\newcommand{\mean}[1]{\ensuremath{\left\langle #1 \right\rangle}} % {x}
\newcommand{\abs}[1]{\ensuremath{\left\|#1\right\|}} % {x}
\newcommand{\Real}{\ensuremath{\mathcal{R}e}\xspace}
\newcommand{\Imag}{\ensuremath{\mathcal{I}m}\xspace}

\def\PDF {PDF\xspace}

\def\sPlot{\mbox{\em sPlot}\xspace}
%%%\def\sWeight{\mbox{\em sWeight}\xspace}

%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
% Kinematics
%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%

%% Energy, Momenta
\def\Ebeam {\ensuremath{E_{\mbox{\tiny BEAM}}}\xspace}
\def\sqs   {\ensuremath{\protect\sqrt{s}}\xspace}

\def\ptot       {\mbox{$p$}\xspace}
\def\pt         {\mbox{$p_{\rm T}$}\xspace}
\def\et         {\mbox{$E_{\rm T}$}\xspace}
\def\mt         {\mbox{$M_{\rm T}$}\xspace}
\def\dpp        {\ensuremath{\Delta p/p}\xspace}
\def\msq        {\ensuremath{m^2}\xspace}
\newcommand{\dedx}{\ensuremath{\mathrm{d}\hspace{-0.1em}E/\mathrm{d}x}\xspace}

%% PID

\def\dllkpi     {\ensuremath{\mathrm{DLL}_{\kaon\pion}}\xspace}
\def\dllppi     {\ensuremath{\mathrm{DLL}_{\proton\pion}}\xspace}
\def\dllepi     {\ensuremath{\mathrm{DLL}_{\electron\pion}}\xspace}
\def\dllmupi    {\ensuremath{\mathrm{DLL}_{\muon\pi}}\xspace}

%% Geometry
%%%\def\mphi       {\mbox{$\phi$}\xspace}
%%%\def\mtheta     {\mbox{$\theta$}\xspace}
%%%\def\ctheta     {\mbox{$\cos\theta$}\xspace}
%%%\def\stheta     {\mbox{$\sin\theta$}\xspace}
%%%\def\ttheta     {\mbox{$\tan\theta$}\xspace}

\def\degrees{\ensuremath{^{\circ}}\xspace}
\def\krad {\ensuremath{\rm \,krad}\xspace}
\def\mrad{\ensuremath{\rm \,mrad}\xspace}
\def\rad{\ensuremath{\rm \,rad}\xspace}

%% Accelerator
\def\betastar {\ensuremath{\beta^*}}
\newcommand{\lum} {\ensuremath{\mathcal{L}}\xspace}
\newcommand{\intlum}[1]{\ensuremath{\int\lum=#1}\xspace}  % {2 \,\invfb}

%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
% Software
%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%

%% Programs
%%%\def\ansys      {\mbox{\textsc{Ansys}}\xspace}
\def\bcvegpy    {\mbox{\textsc{Bcvegpy}}\xspace}
\def\boole      {\mbox{\textsc{Boole}}\xspace}
\def\brunel     {\mbox{\textsc{Brunel}}\xspace}
\def\davinci    {\mbox{\textsc{DaVinci}}\xspace}
\def\dirac      {\mbox{\textsc{Dirac}}\xspace}
%%%\def\erasmus    {\mbox{\textsc{Erasmus}}\xspace}
\def\evtgen     {\mbox{\textsc{EvtGen}}\xspace}
\def\fewz       {\mbox{\textsc{Fewz}}\xspace}
\def\dynnlo       {\mbox{\textsc{DYNNLO}}\xspace}
\def\fluka      {\mbox{\textsc{Fluka}}\xspace}
\def\ganga      {\mbox{\textsc{Ganga}}\xspace}
%%%\def\garfield   {\mbox{\textsc{Garfield}}\xspace}
\def\gaudi      {\mbox{\textsc{Gaudi}}\xspace}
\def\gauss      {\mbox{\textsc{Gauss}}\xspace}
\def\geant      {\mbox{\textsc{Geant4}}\xspace}
\def\hepmc      {\mbox{\textsc{HepMC}}\xspace}
\def\herwig     {\mbox{\textsc{Herwig}}\xspace}
\def\herwiri     {\mbox{\textsc{Herwiri}}\xspace}
\def\mc@nlo     {\mbox{\textsc{MC@NLO}}\xspace}
\def\moore      {\mbox{\textsc{Moore}}\xspace}
\def\neurobayes {\mbox{\textsc{NeuroBayes}}\xspace}
\def\photos     {\mbox{\textsc{Photos}}\xspace}
\def\powheg     {\mbox{\textsc{Powheg}}\xspace}
%%%\def\pyroot     {\mbox{\textsc{PyRoot}}\xspace}
\def\pythia     {\mbox{\textsc{Pythia}}\xspace}
\def\resbos     {\mbox{\textsc{ResBos}}\xspace}
\def\roofit     {\mbox{\textsc{RooFit}}\xspace}
\def\root       {\mbox{\textsc{Root}}\xspace}
\def\spice      {\mbox{\textsc{Spice}}\xspace}
%%%\def\tosca      {\mbox{\textsc{Tosca}}\xspace}
\def\urania     {\mbox{\textsc{Urania}}\xspace}

%% Languages
\def\cpp        {\mbox{\textsc{C\raisebox{0.1em}{{\footnotesize{++}}}}}\xspace}
%%%\def\python     {\mbox{\textsc{Python}}\xspace}
\def\ruby       {\mbox{\textsc{Ruby}}\xspace}
\def\fortran    {\mbox{\textsc{Fortran}}\xspace}
\def\svn        {\mbox{\textsc{SVN}}\xspace}

%% Data processing
\def\kbytes     {\ensuremath{{\rm \,kbytes}}\xspace}
\def\kbsps      {\ensuremath{{\rm \,kbytes/s}}\xspace}
\def\kbits      {\ensuremath{{\rm \,kbits}}\xspace}
\def\kbsps      {\ensuremath{{\rm \,kbits/s}}\xspace}
\def\mbsps      {\ensuremath{{\rm \,Mbits/s}}\xspace}
\def\mbytes     {\ensuremath{{\rm \,Mbytes}}\xspace}
\def\mbps       {\ensuremath{{\rm \,Mbyte/s}}\xspace}
\def\mbsps      {\ensuremath{{\rm \,Mbytes/s}}\xspace}
\def\gbsps      {\ensuremath{{\rm \,Gbits/s}}\xspace}
\def\gbytes     {\ensuremath{{\rm \,Gbytes}}\xspace}
\def\gbsps      {\ensuremath{{\rm \,Gbytes/s}}\xspace}
\def\tbytes     {\ensuremath{{\rm \,Tbytes}}\xspace}
\def\tbpy       {\ensuremath{{\rm \,Tbytes/yr}}\xspace}

\def\dst        {DST\xspace}

%%%%%%%%%%%%%%%%%%%%%%%%%%%
% Detector related
%%%%%%%%%%%%%%%%%%%%%%%%%%%

%% Detector technologies
\def\nonn {\ensuremath{\rm {\it{n^+}}\mbox{-}on\mbox{-}{\it{n}}}\xspace}
\def\ponn {\ensuremath{\rm {\it{p^+}}\mbox{-}on\mbox{-}{\it{n}}}\xspace}
\def\nonp {\ensuremath{\rm {\it{n^+}}\mbox{-}on\mbox{-}{\it{p}}}\xspace}
\def\cvd  {CVD\xspace}
\def\mwpc {MWPC\xspace}
\def\gem  {GEM\xspace}

%% Detector components, electronics
\def\tell1  {TELL1\xspace}
\def\ukl1   {UKL1\xspace}
\def\beetle {Beetle\xspace}
\def\otis   {OTIS\xspace}
\def\croc   {CROC\xspace}
\def\carioca {CARIOCA\xspace}
\def\dialog {DIALOG\xspace}
\def\sync   {SYNC\xspace}
\def\cardiac {CARDIAC\xspace}
\def\gol    {GOL\xspace}
\def\vcsel  {VCSEL\xspace}
\def\ttc    {TTC\xspace}
\def\ttcrx  {TTCrx\xspace}
\def\hpd    {HPD\xspace}
\def\pmt    {PMT\xspace}
\def\specs  {SPECS\xspace}
\def\elmb   {ELMB\xspace}
\def\fpga   {FPGA\xspace}
\def\plc    {PLC\xspace}
\def\rasnik {RASNIK\xspace}
\def\elmb   {ELMB\xspace}
\def\can    {CAN\xspace}
\def\lvds   {LVDS\xspace}
\def\ntc    {NTC\xspace}
\def\adc    {ADC\xspace}
\def\led    {LED\xspace}
\def\ccd    {CCD\xspace}
\def\hv     {HV\xspace}
\def\lv     {LV\xspace}
\def\pvss   {PVSS\xspace}
\def\cmos   {CMOS\xspace}
\def\fifo   {FIFO\xspace}
\def\ccpc   {CCPC\xspace}

%% Chemical symbols
\def\cfourften     {\ensuremath{\rm C_4 F_{10}}\xspace}
\def\cffour        {\ensuremath{\rm CF_4}\xspace}
\def\cotwo         {\ensuremath{\rm CO_2}\xspace} 
\def\csixffouteen  {\ensuremath{\rm C_6 F_{14}}\xspace} 
\def\mgftwo     {\ensuremath{\rm Mg F_2}\xspace} 
\def\siotwo     {\ensuremath{\rm SiO_2}\xspace} 

%%%%%%%%%%%%%%%
% Special Text 
%%%%%%%%%%%%%%%
\newcommand{\eg}{\mbox{\itshape e.g.}\xspace}
\newcommand{\ie}{\mbox{\itshape i.e.}\xspace}
\newcommand{\etal}{\mbox{\itshape et al.}\xspace}
\newcommand{\etc}{\mbox{\itshape etc.}\xspace}
\newcommand{\cf}{\mbox{\itshape cf.}\xspace}
\newcommand{\ffp}{\mbox{\itshape ff.}\xspace}
\newcommand{\vs}{\mbox{\itshape vs.}\xspace}

lhcb-symbols-list.tex
% This is an automatically generated appendix to template.tex. 
% When included it will show all the symbols defined in lhcb-symbols-def.tex.
%
% To regenerate with the latest definitions run the script ./listsymbols

\section{List of all symbols}
\label{sec:listofsymbols}
\subsection{Experiments}
\begin{tabular*}{\linewidth}{@{\extracolsep{\fill}}l@{\extracolsep{0.5cm}}l@{\extracolsep{\fill}}l@{\extracolsep{0.5cm}}l@{\extracolsep{\fill}}l@{\extracolsep{0.5cm}}l}
\texttt{\textbackslash lhcb} & \lhcb & \texttt{\textbackslash atlas} & \atlas & \texttt{\textbackslash cms} & \cms \\
\texttt{\textbackslash alice} & \alice & \texttt{\textbackslash babar} & \babar & \texttt{\textbackslash belle} & \belle \\
\texttt{\textbackslash cleo} & \cleo & \texttt{\textbackslash cdf} & \cdf & \texttt{\textbackslash dzero} & \dzero \\
\texttt{\textbackslash aleph} & \aleph & \texttt{\textbackslash delphi} & \delphi & \texttt{\textbackslash opal} & \opal \\
\texttt{\textbackslash lthree} & \lthree & \texttt{\textbackslash sld} & \sld & \texttt{\textbackslash cern} & \cern \\
\texttt{\textbackslash lhc} & \lhc & \texttt{\textbackslash lep} & \lep & \texttt{\textbackslash tevatron} & \tevatron \\
\end{tabular*}

\subsubsection{LHCb sub-detectors and sub-systems}
\begin{tabular*}{\linewidth}{@{\extracolsep{\fill}}l@{\extracolsep{0.5cm}}l@{\extracolsep{\fill}}l@{\extracolsep{0.5cm}}l@{\extracolsep{\fill}}l@{\extracolsep{0.5cm}}l}
\texttt{\textbackslash velo} & \velo & \texttt{\textbackslash rich} & \rich & \texttt{\textbackslash richone} & \richone \\
\texttt{\textbackslash richtwo} & \richtwo & \texttt{\textbackslash ttracker} & \ttracker & \texttt{\textbackslash intr} & \intr \\
\texttt{\textbackslash st} & \st & \texttt{\textbackslash ot} & \ot & \texttt{\textbackslash spd} & \spd \\
\texttt{\textbackslash presh} & \presh & \texttt{\textbackslash ecal} & \ecal & \texttt{\textbackslash hcal} & \hcal \\
\texttt{\textbackslash MagUp} & \MagUp & \texttt{\textbackslash MagDown} & \MagDown &  \\
\end{tabular*}

\subsection{Particles}
\subsubsection{Leptons}
\begin{tabular*}{\linewidth}{@{\extracolsep{\fill}}l@{\extracolsep{0.5cm}}l@{\extracolsep{\fill}}l@{\extracolsep{0.5cm}}l@{\extracolsep{\fill}}l@{\extracolsep{0.5cm}}l}
\texttt{\textbackslash electron} & \electron & \texttt{\textbackslash en} & \en & \texttt{\textbackslash ep} & \ep \\
\texttt{\textbackslash epm} & \epm & \texttt{\textbackslash epem} & \epem & \texttt{\textbackslash muon} & \muon \\
\texttt{\textbackslash mup} & \mup & \texttt{\textbackslash mun} & \mun & \texttt{\textbackslash mumu} & \mumu \\
\texttt{\textbackslash tauon} & \tauon & \texttt{\textbackslash taup} & \taup & \texttt{\textbackslash taum} & \taum \\
\texttt{\textbackslash tautau} & \tautau & \texttt{\textbackslash lepton} & \lepton & \texttt{\textbackslash ellm} & \ellm \\
\texttt{\textbackslash ellp} & \ellp & \texttt{\textbackslash neu} & \neu & \texttt{\textbackslash neub} & \neub \\
\texttt{\textbackslash neue} & \neue & \texttt{\textbackslash neueb} & \neueb & \texttt{\textbackslash neum} & \neum \\
\texttt{\textbackslash neumb} & \neumb & \texttt{\textbackslash neut} & \neut & \texttt{\textbackslash neutb} & \neutb \\
\texttt{\textbackslash neul} & \neul & \texttt{\textbackslash neulb} & \neulb &  \\
\end{tabular*}

\subsubsection{Gauge bosons and scalars}
\begin{tabular*}{\linewidth}{@{\extracolsep{\fill}}l@{\extracolsep{0.5cm}}l@{\extracolsep{\fill}}l@{\extracolsep{0.5cm}}l@{\extracolsep{\fill}}l@{\extracolsep{0.5cm}}l}
\texttt{\textbackslash g} & \g & \texttt{\textbackslash H} & \H & \texttt{\textbackslash Hp} & \Hp \\
\texttt{\textbackslash Hm} & \Hm & \texttt{\textbackslash Hpm} & \Hpm & \texttt{\textbackslash W} & \W \\
\texttt{\textbackslash Wp} & \Wp & \texttt{\textbackslash Wm} & \Wm & \texttt{\textbackslash Wpm} & \Wpm \\
\texttt{\textbackslash Z} & \Z &  \\
\end{tabular*}

\subsubsection{Quarks}
\begin{tabular*}{\linewidth}{@{\extracolsep{\fill}}l@{\extracolsep{0.5cm}}l@{\extracolsep{\fill}}l@{\extracolsep{0.5cm}}l@{\extracolsep{\fill}}l@{\extracolsep{0.5cm}}l}
\texttt{\textbackslash quark} & \quark & \texttt{\textbackslash quarkbar} & \quarkbar & \texttt{\textbackslash qqbar} & \qqbar \\
\texttt{\textbackslash uquark} & \uquark & \texttt{\textbackslash uquarkbar} & \uquarkbar & \texttt{\textbackslash uubar} & \uubar \\
\texttt{\textbackslash dquark} & \dquark & \texttt{\textbackslash dquarkbar} & \dquarkbar & \texttt{\textbackslash ddbar} & \ddbar \\
\texttt{\textbackslash squark} & \squark & \texttt{\textbackslash squarkbar} & \squarkbar & \texttt{\textbackslash ssbar} & \ssbar \\
\texttt{\textbackslash cquark} & \cquark & \texttt{\textbackslash cquarkbar} & \cquarkbar & \texttt{\textbackslash ccbar} & \ccbar \\
\texttt{\textbackslash bquark} & \bquark & \texttt{\textbackslash bquarkbar} & \bquarkbar & \texttt{\textbackslash bbbar} & \bbbar \\
\texttt{\textbackslash tquark} & \tquark & \texttt{\textbackslash tquarkbar} & \tquarkbar & \texttt{\textbackslash ttbar} & \ttbar \\
\end{tabular*}

\subsubsection{Light mesons}
\begin{tabular*}{\linewidth}{@{\extracolsep{\fill}}l@{\extracolsep{0.5cm}}l@{\extracolsep{\fill}}l@{\extracolsep{0.5cm}}l@{\extracolsep{\fill}}l@{\extracolsep{0.5cm}}l}
\texttt{\textbackslash hadron} & \hadron & \texttt{\textbackslash pion} & \pion & \texttt{\textbackslash piz} & \piz \\
\texttt{\textbackslash pizs} & \pizs & \texttt{\textbackslash pip} & \pip & \texttt{\textbackslash pim} & \pim \\
\texttt{\textbackslash pipm} & \pipm & \texttt{\textbackslash pimp} & \pimp & \texttt{\textbackslash rhomeson} & \rhomeson \\
\texttt{\textbackslash rhoz} & \rhoz & \texttt{\textbackslash rhop} & \rhop & \texttt{\textbackslash rhom} & \rhom \\
\texttt{\textbackslash rhopm} & \rhopm & \texttt{\textbackslash rhomp} & \rhomp & \texttt{\textbackslash kaon} & \kaon \\
\texttt{\textbackslash Kb} & \Kb & \texttt{\textbackslash KorKbar} & \KorKbar & \texttt{\textbackslash Kz} & \Kz \\
\texttt{\textbackslash Kzb} & \Kzb & \texttt{\textbackslash Kp} & \Kp & \texttt{\textbackslash Km} & \Km \\
\texttt{\textbackslash Kpm} & \Kpm & \texttt{\textbackslash Kmp} & \Kmp & \texttt{\textbackslash KS} & \KS \\
\texttt{\textbackslash KL} & \KL & \texttt{\textbackslash Kstarz} & \Kstarz & \texttt{\textbackslash Kstarzb} & \Kstarzb \\
\texttt{\textbackslash Kstar} & \Kstar & \texttt{\textbackslash Kstarb} & \Kstarb & \texttt{\textbackslash Kstarp} & \Kstarp \\
\texttt{\textbackslash Kstarm} & \Kstarm & \texttt{\textbackslash Kstarpm} & \Kstarpm & \texttt{\textbackslash Kstarmp} & \Kstarmp \\
\texttt{\textbackslash etaz} & \etaz & \texttt{\textbackslash etapr} & \etapr & \texttt{\textbackslash phiz} & \phiz \\
\texttt{\textbackslash omegaz} & \omegaz &  \\
\end{tabular*}

\subsubsection{Heavy mesons}
\begin{tabular*}{\linewidth}{@{\extracolsep{\fill}}l@{\extracolsep{0.5cm}}l@{\extracolsep{\fill}}l@{\extracolsep{0.5cm}}l@{\extracolsep{\fill}}l@{\extracolsep{0.5cm}}l}
\texttt{\textbackslash D} & \D & \texttt{\textbackslash Db} & \Db & \texttt{\textbackslash DorDbar} & \DorDbar \\
\texttt{\textbackslash Dz} & \Dz & \texttt{\textbackslash Dzb} & \Dzb & \texttt{\textbackslash Dp} & \Dp \\
\texttt{\textbackslash Dm} & \Dm & \texttt{\textbackslash Dpm} & \Dpm & \texttt{\textbackslash Dmp} & \Dmp \\
\texttt{\textbackslash Dstar} & \Dstar & \texttt{\textbackslash Dstarb} & \Dstarb & \texttt{\textbackslash Dstarz} & \Dstarz \\
\texttt{\textbackslash Dstarzb} & \Dstarzb & \texttt{\textbackslash Dstarp} & \Dstarp & \texttt{\textbackslash Dstarm} & \Dstarm \\
\texttt{\textbackslash Dstarpm} & \Dstarpm & \texttt{\textbackslash Dstarmp} & \Dstarmp & \texttt{\textbackslash Ds} & \Ds \\
\texttt{\textbackslash Dsp} & \Dsp & \texttt{\textbackslash Dsm} & \Dsm & \texttt{\textbackslash Dspm} & \Dspm \\
\texttt{\textbackslash Dsmp} & \Dsmp & \texttt{\textbackslash Dss} & \Dss & \texttt{\textbackslash Dssp} & \Dssp \\
\texttt{\textbackslash Dssm} & \Dssm & \texttt{\textbackslash Dsspm} & \Dsspm & \texttt{\textbackslash Dssmp} & \Dssmp \\
\texttt{\textbackslash B} & \B & \texttt{\textbackslash Bbar} & \Bbar & \texttt{\textbackslash Bb} & \Bb \\
\texttt{\textbackslash BorBbar} & \BorBbar & \texttt{\textbackslash Bz} & \Bz & \texttt{\textbackslash Bzb} & \Bzb \\
\texttt{\textbackslash Bu} & \Bu & \texttt{\textbackslash Bub} & \Bub & \texttt{\textbackslash Bp} & \Bp \\
\texttt{\textbackslash Bm} & \Bm & \texttt{\textbackslash Bpm} & \Bpm & \texttt{\textbackslash Bmp} & \Bmp \\
\texttt{\textbackslash Bd} & \Bd & \texttt{\textbackslash Bs} & \Bs & \texttt{\textbackslash Bsb} & \Bsb \\
\texttt{\textbackslash Bdb} & \Bdb & \texttt{\textbackslash Bc} & \Bc & \texttt{\textbackslash Bcp} & \Bcp \\
\texttt{\textbackslash Bcm} & \Bcm & \texttt{\textbackslash Bcpm} & \Bcpm &  \\
\end{tabular*}

\subsubsection{Onia}
\begin{tabular*}{\linewidth}{@{\extracolsep{\fill}}l@{\extracolsep{0.5cm}}l@{\extracolsep{\fill}}l@{\extracolsep{0.5cm}}l@{\extracolsep{\fill}}l@{\extracolsep{0.5cm}}l}
\texttt{\textbackslash jpsi} & \jpsi & \texttt{\textbackslash psitwos} & \psitwos & \texttt{\textbackslash psiprpr} & \psiprpr \\
\texttt{\textbackslash etac} & \etac & \texttt{\textbackslash chiczero} & \chiczero & \texttt{\textbackslash chicone} & \chicone \\
\texttt{\textbackslash chictwo} & \chictwo & \texttt{\textbackslash OneS} & \OneS & \texttt{\textbackslash TwoS} & \TwoS \\
\texttt{\textbackslash ThreeS} & \ThreeS & \texttt{\textbackslash FourS} & \FourS & \texttt{\textbackslash FiveS} & \FiveS \\
\texttt{\textbackslash chic} & \chic &  \\
\end{tabular*}

\subsubsection{Baryons}
\begin{tabular*}{\linewidth}{@{\extracolsep{\fill}}l@{\extracolsep{0.5cm}}l@{\extracolsep{\fill}}l@{\extracolsep{0.5cm}}l@{\extracolsep{\fill}}l@{\extracolsep{0.5cm}}l}
\texttt{\textbackslash proton} & \proton & \texttt{\textbackslash antiproton} & \antiproton & \texttt{\textbackslash neutron} & \neutron \\
\texttt{\textbackslash antineutron} & \antineutron & \texttt{\textbackslash Deltares} & \Deltares & \texttt{\textbackslash Deltaresbar} & \Deltaresbar \\
\texttt{\textbackslash Xires} & \Xires & \texttt{\textbackslash Xiresbar} & \Xiresbar & \texttt{\textbackslash Lz} & \Lz \\
\texttt{\textbackslash Lbar} & \Lbar & \texttt{\textbackslash LorLbar} & \LorLbar & \texttt{\textbackslash Lambdares} & \Lambdares \\
\texttt{\textbackslash Lambdaresbar} & \Lambdaresbar & \texttt{\textbackslash Sigmares} & \Sigmares & \texttt{\textbackslash Sigmaresbar} & \Sigmaresbar \\
\texttt{\textbackslash Omegares} & \Omegares & \texttt{\textbackslash Omegaresbar} & \Omegaresbar & \texttt{\textbackslash Lb} & \Lb \\
\texttt{\textbackslash Lbbar} & \Lbbar & \texttt{\textbackslash Lc} & \Lc & \texttt{\textbackslash Lcbar} & \Lcbar \\
\texttt{\textbackslash Xibz} & \Xibz & \texttt{\textbackslash Xibm} & \Xibm & \texttt{\textbackslash Xibbarz} & \Xibbarz \\
\texttt{\textbackslash Xibbarp} & \Xibbarp & \texttt{\textbackslash Xicz} & \Xicz & \texttt{\textbackslash Xicp} & \Xicp \\
\texttt{\textbackslash Xicbarz} & \Xicbarz & \texttt{\textbackslash Xicbarm} & \Xicbarm & \texttt{\textbackslash Omegac} & \Omegac \\
\texttt{\textbackslash Omegacbar} & \Omegacbar & \texttt{\textbackslash Omegab} & \Omegab & \texttt{\textbackslash Omegabbar} & \Omegabbar \\
\end{tabular*}

\subsection{Physics symbols}
\subsubsection{Decays}
\begin{tabular*}{\linewidth}{@{\extracolsep{\fill}}l@{\extracolsep{0.5cm}}l@{\extracolsep{\fill}}l@{\extracolsep{0.5cm}}l@{\extracolsep{\fill}}l@{\extracolsep{0.5cm}}l}
\texttt{\textbackslash BF} & \BF & \texttt{\textbackslash BRvis} & \BRvis & \texttt{\textbackslash BR} & \BR \\
\texttt{\textbackslash decay[2] \textbackslash decay\{\Pa\}\{\Pb \Pc\}} & \decay{\Pa}{\Pb \Pc} & \texttt{\textbackslash ra} & \ra & \texttt{\textbackslash to} & \to \\
\end{tabular*}

\subsubsection{Lifetimes}
\begin{tabular*}{\linewidth}{@{\extracolsep{\fill}}l@{\extracolsep{0.5cm}}l@{\extracolsep{\fill}}l@{\extracolsep{0.5cm}}l@{\extracolsep{\fill}}l@{\extracolsep{0.5cm}}l}
\texttt{\textbackslash tauBs} & \tauBs & \texttt{\textbackslash tauBd} & \tauBd & \texttt{\textbackslash tauBz} & \tauBz \\
\texttt{\textbackslash tauBu} & \tauBu & \texttt{\textbackslash tauDp} & \tauDp & \texttt{\textbackslash tauDz} & \tauDz \\
\texttt{\textbackslash tauL} & \tauL & \texttt{\textbackslash tauH} & \tauH &  \\
\end{tabular*}

\subsubsection{Masses}
\begin{tabular*}{\linewidth}{@{\extracolsep{\fill}}l@{\extracolsep{0.5cm}}l@{\extracolsep{\fill}}l@{\extracolsep{0.5cm}}l@{\extracolsep{\fill}}l@{\extracolsep{0.5cm}}l}
\texttt{\textbackslash mBd} & \mBd & \texttt{\textbackslash mBp} & \mBp & \texttt{\textbackslash mBs} & \mBs \\
\texttt{\textbackslash mBc} & \mBc & \texttt{\textbackslash mLb} & \mLb &  \\
\end{tabular*}

\subsubsection{EW theory, groups}
\begin{tabular*}{\linewidth}{@{\extracolsep{\fill}}l@{\extracolsep{0.5cm}}l@{\extracolsep{\fill}}l@{\extracolsep{0.5cm}}l@{\extracolsep{\fill}}l@{\extracolsep{0.5cm}}l}
\texttt{\textbackslash grpsuthree} & \grpsuthree & \texttt{\textbackslash grpsutw} & \grpsutw & \texttt{\textbackslash grpuone} & \grpuone \\
\texttt{\textbackslash ssqtw} & \ssqtw & \texttt{\textbackslash csqtw} & \csqtw & \texttt{\textbackslash stw} & \stw \\
\texttt{\textbackslash ctw} & \ctw & \texttt{\textbackslash ssqtwef} & \ssqtwef & \texttt{\textbackslash csqtwef} & \csqtwef \\
\texttt{\textbackslash stwef} & \stwef & \texttt{\textbackslash ctwef} & \ctwef & \texttt{\textbackslash gv} & \gv \\
\texttt{\textbackslash ga} & \ga & \texttt{\textbackslash order} & \order & \texttt{\textbackslash ordalph} & \ordalph \\
\texttt{\textbackslash ordalsq} & \ordalsq & \texttt{\textbackslash ordalcb} & \ordalcb &  \\
\end{tabular*}

\subsubsection{QCD parameters}
\begin{tabular*}{\linewidth}{@{\extracolsep{\fill}}l@{\extracolsep{0.5cm}}l@{\extracolsep{\fill}}l@{\extracolsep{0.5cm}}l@{\extracolsep{\fill}}l@{\extracolsep{0.5cm}}l}
\texttt{\textbackslash as} & \as & \texttt{\textbackslash MSb} & \MSb & \texttt{\textbackslash lqcd} & \lqcd \\
\texttt{\textbackslash qsq} & \qsq &  \\
\end{tabular*}

\subsubsection{CKM, CP violation}
\begin{tabular*}{\linewidth}{@{\extracolsep{\fill}}l@{\extracolsep{0.5cm}}l@{\extracolsep{\fill}}l@{\extracolsep{0.5cm}}l@{\extracolsep{\fill}}l@{\extracolsep{0.5cm}}l}
\texttt{\textbackslash eps} & \eps & \texttt{\textbackslash epsK} & \epsK & \texttt{\textbackslash epsB} & \epsB \\
\texttt{\textbackslash epsp} & \epsp & \texttt{\textbackslash CP} & \CP & \texttt{\textbackslash CPT} & \CPT \\
\texttt{\textbackslash rhobar} & \rhobar & \texttt{\textbackslash etabar} & \etabar & \texttt{\textbackslash Vud} & \Vud \\
\texttt{\textbackslash Vcd} & \Vcd & \texttt{\textbackslash Vtd} & \Vtd & \texttt{\textbackslash Vus} & \Vus \\
\texttt{\textbackslash Vcs} & \Vcs & \texttt{\textbackslash Vts} & \Vts & \texttt{\textbackslash Vub} & \Vub \\
\texttt{\textbackslash Vcb} & \Vcb & \texttt{\textbackslash Vtb} & \Vtb & \texttt{\textbackslash Vuds} & \Vuds \\
\texttt{\textbackslash Vcds} & \Vcds & \texttt{\textbackslash Vtds} & \Vtds & \texttt{\textbackslash Vuss} & \Vuss \\
\texttt{\textbackslash Vcss} & \Vcss & \texttt{\textbackslash Vtss} & \Vtss & \texttt{\textbackslash Vubs} & \Vubs \\
\texttt{\textbackslash Vcbs} & \Vcbs & \texttt{\textbackslash Vtbs} & \Vtbs &  \\
\end{tabular*}

\subsubsection{Oscillations}
\begin{tabular*}{\linewidth}{@{\extracolsep{\fill}}l@{\extracolsep{0.5cm}}l@{\extracolsep{\fill}}l@{\extracolsep{0.5cm}}l@{\extracolsep{\fill}}l@{\extracolsep{0.5cm}}l}
\texttt{\textbackslash dm} & \dm & \texttt{\textbackslash dms} & \dms & \texttt{\textbackslash dmd} & \dmd \\
\texttt{\textbackslash DG} & \DG & \texttt{\textbackslash DGs} & \DGs & \texttt{\textbackslash DGd} & \DGd \\
\texttt{\textbackslash Gs} & \Gs & \texttt{\textbackslash Gd} & \Gd & \texttt{\textbackslash MBq} & \MBq \\
\texttt{\textbackslash DGq} & \DGq & \texttt{\textbackslash Gq} & \Gq & \texttt{\textbackslash dmq} & \dmq \\
\texttt{\textbackslash GL} & \GL & \texttt{\textbackslash GH} & \GH & \texttt{\textbackslash DGsGs} & \DGsGs \\
\texttt{\textbackslash Delm} & \Delm & \texttt{\textbackslash ACP} & \ACP & \texttt{\textbackslash Adir} & \Adir \\
\texttt{\textbackslash Amix} & \Amix & \texttt{\textbackslash ADelta} & \ADelta & \texttt{\textbackslash phid} & \phid \\
\texttt{\textbackslash sinphid} & \sinphid & \texttt{\textbackslash phis} & \phis & \texttt{\textbackslash betas} & \betas \\
\texttt{\textbackslash sbetas} & \sbetas & \texttt{\textbackslash stbetas} & \stbetas & \texttt{\textbackslash stphis} & \stphis \\
\texttt{\textbackslash sinphis} & \sinphis &  \\
\end{tabular*}

\subsubsection{Tagging}
\begin{tabular*}{\linewidth}{@{\extracolsep{\fill}}l@{\extracolsep{0.5cm}}l@{\extracolsep{\fill}}l@{\extracolsep{0.5cm}}l@{\extracolsep{\fill}}l@{\extracolsep{0.5cm}}l}
\texttt{\textbackslash edet} & \edet & \texttt{\textbackslash erec} & \erec & \texttt{\textbackslash esel} & \esel \\
\texttt{\textbackslash etrg} & \etrg & \texttt{\textbackslash etot} & \etot & \texttt{\textbackslash mistag} & \mistag \\
\texttt{\textbackslash wcomb} & \wcomb & \texttt{\textbackslash etag} & \etag & \texttt{\textbackslash etagcomb} & \etagcomb \\
\texttt{\textbackslash effeff} & \effeff & \texttt{\textbackslash effeffcomb} & \effeffcomb & \texttt{\textbackslash efftag} & \efftag \\
\texttt{\textbackslash effD} & \effD & \texttt{\textbackslash etagprompt} & \etagprompt & \texttt{\textbackslash etagLL} & \etagLL \\
\end{tabular*}

\subsubsection{Key decay channels}
\begin{tabular*}{\linewidth}{@{\extracolsep{\fill}}l@{\extracolsep{0.5cm}}l@{\extracolsep{\fill}}l@{\extracolsep{0.5cm}}l@{\extracolsep{\fill}}l@{\extracolsep{0.5cm}}l}
\texttt{\textbackslash BdToKstmm} & \BdToKstmm & \texttt{\textbackslash BdbToKstmm} & \BdbToKstmm & \texttt{\textbackslash BsToJPsiPhi} & \BsToJPsiPhi \\
\texttt{\textbackslash BdToJPsiKst} & \BdToJPsiKst & \texttt{\textbackslash BdbToJPsiKst} & \BdbToJPsiKst & \texttt{\textbackslash BsPhiGam} & \BsPhiGam \\
\texttt{\textbackslash BdKstGam} & \BdKstGam & \texttt{\textbackslash BTohh} & \BTohh & \texttt{\textbackslash BdTopipi} & \BdTopipi \\
\texttt{\textbackslash BdToKpi} & \BdToKpi & \texttt{\textbackslash BsToKK} & \BsToKK & \texttt{\textbackslash BsTopiK} & \BsTopiK \\
\end{tabular*}

\subsubsection{Rare decays}
\begin{tabular*}{\linewidth}{@{\extracolsep{\fill}}l@{\extracolsep{0.5cm}}l@{\extracolsep{\fill}}l@{\extracolsep{0.5cm}}l@{\extracolsep{\fill}}l@{\extracolsep{0.5cm}}l}
\texttt{\textbackslash BdKstee} & \BdKstee & \texttt{\textbackslash BdbKstee} & \BdbKstee & \texttt{\textbackslash bsll} & \bsll \\
\texttt{\textbackslash AFB} & \AFB & \texttt{\textbackslash FL} & \FL & \texttt{\textbackslash AT\#1 \textbackslash AT2} & \AT2 \\
\texttt{\textbackslash btosgam} & \btosgam & \texttt{\textbackslash btodgam} & \btodgam & \texttt{\textbackslash Bsmm} & \Bsmm \\
\texttt{\textbackslash Bdmm} & \Bdmm & \texttt{\textbackslash ctl} & \ctl & \texttt{\textbackslash ctk} & \ctk \\
\end{tabular*}

\subsubsection{Wilson coefficients and operators}
\begin{tabular*}{\linewidth}{@{\extracolsep{\fill}}l@{\extracolsep{0.5cm}}l@{\extracolsep{\fill}}l@{\extracolsep{0.5cm}}l@{\extracolsep{\fill}}l@{\extracolsep{0.5cm}}l}
\texttt{\textbackslash C\#1 \textbackslash C9} & \C9 & \texttt{\textbackslash Cp\#1 \textbackslash Cp7} & \Cp7 & \texttt{\textbackslash Ceff\#1 \textbackslash Ceff9  } & \Ceff9   \\
\texttt{\textbackslash Cpeff\#1 \textbackslash Cpeff7} & \Cpeff7 & \texttt{\textbackslash Ope\#1 \textbackslash Ope2} & \Ope2 & \texttt{\textbackslash Opep\#1 \textbackslash Opep7} & \Opep7 \\
\end{tabular*}

\subsubsection{Charm}
\begin{tabular*}{\linewidth}{@{\extracolsep{\fill}}l@{\extracolsep{0.5cm}}l@{\extracolsep{\fill}}l@{\extracolsep{0.5cm}}l@{\extracolsep{\fill}}l@{\extracolsep{0.5cm}}l}
\texttt{\textbackslash xprime} & \xprime & \texttt{\textbackslash yprime} & \yprime & \texttt{\textbackslash ycp} & \ycp \\
\texttt{\textbackslash agamma} & \agamma & \texttt{\textbackslash dkpicf} & \dkpicf &  \\
\end{tabular*}

\subsubsection{QM}
\begin{tabular*}{\linewidth}{@{\extracolsep{\fill}}l@{\extracolsep{0.5cm}}l@{\extracolsep{\fill}}l@{\extracolsep{0.5cm}}l@{\extracolsep{\fill}}l@{\extracolsep{0.5cm}}l}
\texttt{\textbackslash bra[1] \textbackslash bra\{a\}} & \bra{a} & \texttt{\textbackslash ket[1] \textbackslash ket\{b\}} & \ket{b} & \texttt{\textbackslash braket[2] \textbackslash braket\{a\}\{b\}} & \braket{a}{b} \\
\end{tabular*}

\subsection{Units}
\begin{tabular*}{\linewidth}{@{\extracolsep{\fill}}l@{\extracolsep{0.5cm}}l@{\extracolsep{\fill}}l@{\extracolsep{0.5cm}}l@{\extracolsep{\fill}}l@{\extracolsep{0.5cm}}l}
\texttt{\textbackslash unit[1] \textbackslash unit\{kg\}} & \unit{kg} &  \\
\end{tabular*}

\subsubsection{Energy and momentum}
\begin{tabular*}{\linewidth}{@{\extracolsep{\fill}}l@{\extracolsep{0.5cm}}l@{\extracolsep{\fill}}l@{\extracolsep{0.5cm}}l@{\extracolsep{\fill}}l@{\extracolsep{0.5cm}}l}
\texttt{\textbackslash tev} & \tev & \texttt{\textbackslash gev} & \gev & \texttt{\textbackslash mev} & \mev \\
\texttt{\textbackslash kev} & \kev & \texttt{\textbackslash ev} & \ev & \texttt{\textbackslash gevc} & \gevc \\
\texttt{\textbackslash mevc} & \mevc & \texttt{\textbackslash gevcc} & \gevcc & \texttt{\textbackslash gevgevcccc} & \gevgevcccc \\
\texttt{\textbackslash mevcc} & \mevcc &  \\
\end{tabular*}

\subsubsection{Distance and area}
\begin{tabular*}{\linewidth}{@{\extracolsep{\fill}}l@{\extracolsep{0.5cm}}l@{\extracolsep{\fill}}l@{\extracolsep{0.5cm}}l@{\extracolsep{\fill}}l@{\extracolsep{0.5cm}}l}
\texttt{\textbackslash km} & \km & \texttt{\textbackslash m} & \m & \texttt{\textbackslash ma} & \ma \\
\texttt{\textbackslash cm} & \cm & \texttt{\textbackslash cma} & \cma & \texttt{\textbackslash mm} & \mm \\
\texttt{\textbackslash mma} & \mma & \texttt{\textbackslash mum} & \mum & \texttt{\textbackslash muma} & \muma \\
\texttt{\textbackslash nm} & \nm & \texttt{\textbackslash fm} & \fm & \texttt{\textbackslash barn} & \barn \\
\texttt{\textbackslash mbarn} & \mbarn & \texttt{\textbackslash mub} & \mub & \texttt{\textbackslash nb} & \nb \\
\texttt{\textbackslash invnb} & \invnb & \texttt{\textbackslash pb} & \pb & \texttt{\textbackslash invpb} & \invpb \\
\texttt{\textbackslash fb} & \fb & \texttt{\textbackslash invfb} & \invfb &  \\
\end{tabular*}

\subsubsection{Time }
\begin{tabular*}{\linewidth}{@{\extracolsep{\fill}}l@{\extracolsep{0.5cm}}l@{\extracolsep{\fill}}l@{\extracolsep{0.5cm}}l@{\extracolsep{\fill}}l@{\extracolsep{0.5cm}}l}
\texttt{\textbackslash sec} & \sec & \texttt{\textbackslash ms} & \ms & \texttt{\textbackslash mus} & \mus \\
\texttt{\textbackslash ns} & \ns & \texttt{\textbackslash ps} & \ps & \texttt{\textbackslash fs} & \fs \\
\texttt{\textbackslash mhz} & \mhz & \texttt{\textbackslash khz} & \khz & \texttt{\textbackslash hz} & \hz \\
\texttt{\textbackslash invps} & \invps & \texttt{\textbackslash yr} & \yr & \texttt{\textbackslash hr} & \hr \\
\end{tabular*}

\subsubsection{Temperature}
\begin{tabular*}{\linewidth}{@{\extracolsep{\fill}}l@{\extracolsep{0.5cm}}l@{\extracolsep{\fill}}l@{\extracolsep{0.5cm}}l@{\extracolsep{\fill}}l@{\extracolsep{0.5cm}}l}
\texttt{\textbackslash degc} & \degc & \texttt{\textbackslash degk} & \degk &  \\
\end{tabular*}

\subsubsection{Material lengths, radiation}
\begin{tabular*}{\linewidth}{@{\extracolsep{\fill}}l@{\extracolsep{0.5cm}}l@{\extracolsep{\fill}}l@{\extracolsep{0.5cm}}l@{\extracolsep{\fill}}l@{\extracolsep{0.5cm}}l}
\texttt{\textbackslash Xrad} & \Xrad & \texttt{\textbackslash NIL} & \NIL & \texttt{\textbackslash mip} & \mip \\
\texttt{\textbackslash neutroneq} & \neutroneq & \texttt{\textbackslash neqcmcm} & \neqcmcm & \texttt{\textbackslash kRad} & \kRad \\
\texttt{\textbackslash MRad} & \MRad & \texttt{\textbackslash ci} & \ci & \texttt{\textbackslash mci} & \mci \\
\end{tabular*}

\subsubsection{Uncertainties}
\begin{tabular*}{\linewidth}{@{\extracolsep{\fill}}l@{\extracolsep{0.5cm}}l@{\extracolsep{\fill}}l@{\extracolsep{0.5cm}}l@{\extracolsep{\fill}}l@{\extracolsep{0.5cm}}l}
\texttt{\textbackslash sx} & \sx & \texttt{\textbackslash sy} & \sy & \texttt{\textbackslash sz} & \sz \\
\texttt{\textbackslash stat} & \stat & \texttt{\textbackslash syst} & \syst &  \\
\end{tabular*}

\subsubsection{Maths}
\begin{tabular*}{\linewidth}{@{\extracolsep{\fill}}l@{\extracolsep{0.5cm}}l@{\extracolsep{\fill}}l@{\extracolsep{0.5cm}}l@{\extracolsep{\fill}}l@{\extracolsep{0.5cm}}l}
\texttt{\textbackslash order} & \order & \texttt{\textbackslash chisq} & \chisq & \texttt{\textbackslash chisqndf} & \chisqndf \\
\texttt{\textbackslash chisqip} & \chisqip & \texttt{\textbackslash chisqvs} & \chisqvs & \texttt{\textbackslash chisqvtx} & \chisqvtx \\
\texttt{\textbackslash deriv} & \deriv & \texttt{\textbackslash gsim} & \gsim & \texttt{\textbackslash lsim} & \lsim \\
\texttt{\textbackslash mean[1] \textbackslash mean\{x\}} & \mean{x} & \texttt{\textbackslash abs[1] \textbackslash abs\{x\}} & \abs{x} & \texttt{\textbackslash Real} & \Real \\
\texttt{\textbackslash Imag} & \Imag & \texttt{\textbackslash PDF} & \PDF & \texttt{\textbackslash sPlot} & \sPlot \\
\end{tabular*}

\subsection{Kinematics}
\subsubsection{Energy, Momenta}
\begin{tabular*}{\linewidth}{@{\extracolsep{\fill}}l@{\extracolsep{0.5cm}}l@{\extracolsep{\fill}}l@{\extracolsep{0.5cm}}l@{\extracolsep{\fill}}l@{\extracolsep{0.5cm}}l}
\texttt{\textbackslash Ebeam} & \Ebeam & \texttt{\textbackslash sqs} & \sqs & \texttt{\textbackslash ptot} & \ptot \\
\texttt{\textbackslash pt} & \pt & \texttt{\textbackslash et} & \et & \texttt{\textbackslash mt} & \mt \\
\texttt{\textbackslash dpp} & \dpp & \texttt{\textbackslash msq} & \msq & \texttt{\textbackslash dedx} & \dedx \\
\end{tabular*}

\subsubsection{PID}
\begin{tabular*}{\linewidth}{@{\extracolsep{\fill}}l@{\extracolsep{0.5cm}}l@{\extracolsep{\fill}}l@{\extracolsep{0.5cm}}l@{\extracolsep{\fill}}l@{\extracolsep{0.5cm}}l}
\texttt{\textbackslash dllkpi} & \dllkpi & \texttt{\textbackslash dllppi} & \dllppi & \texttt{\textbackslash dllepi} & \dllepi \\
\texttt{\textbackslash dllmupi} & \dllmupi &  \\
\end{tabular*}

\subsubsection{Geometry}
\begin{tabular*}{\linewidth}{@{\extracolsep{\fill}}l@{\extracolsep{0.5cm}}l@{\extracolsep{\fill}}l@{\extracolsep{0.5cm}}l@{\extracolsep{\fill}}l@{\extracolsep{0.5cm}}l}
\texttt{\textbackslash degrees} & \degrees & \texttt{\textbackslash krad} & \krad & \texttt{\textbackslash mrad} & \mrad \\
\texttt{\textbackslash rad} & \rad &  \\
\end{tabular*}

\subsubsection{Accelerator}
\begin{tabular*}{\linewidth}{@{\extracolsep{\fill}}l@{\extracolsep{0.5cm}}l@{\extracolsep{\fill}}l@{\extracolsep{0.5cm}}l@{\extracolsep{\fill}}l@{\extracolsep{0.5cm}}l}
\texttt{\textbackslash betastar} & \betastar & \texttt{\textbackslash lum} & \lum & \texttt{\textbackslash intlum[1] \textbackslash intlum\{2 \,\invfb\}} & \intlum{2 \,\invfb} \\
\end{tabular*}

\subsection{Software}
\subsubsection{Programs}
\begin{tabular*}{\linewidth}{@{\extracolsep{\fill}}l@{\extracolsep{0.5cm}}l@{\extracolsep{\fill}}l@{\extracolsep{0.5cm}}l@{\extracolsep{\fill}}l@{\extracolsep{0.5cm}}l}
\texttt{\textbackslash bcvegpy} & \bcvegpy & \texttt{\textbackslash boole} & \boole & \texttt{\textbackslash brunel} & \brunel \\
\texttt{\textbackslash davinci} & \davinci & \texttt{\textbackslash dirac} & \dirac & \texttt{\textbackslash evtgen} & \evtgen \\
\texttt{\textbackslash fewz} & \fewz & \texttt{\textbackslash fluka} & \fluka & \texttt{\textbackslash ganga} & \ganga \\
\texttt{\textbackslash dynnlo} & \dynnlo \\
\texttt{\textbackslash gaudi} & \gaudi & \texttt{\textbackslash gauss} & \gauss & \texttt{\textbackslash geant} & \geant \\
\texttt{\textbackslash hepmc} & \hepmc & \texttt{\textbackslash herwig} & \herwig & \texttt{\textbackslash moore} & \moore \\
\texttt{\textbackslash neurobayes} & \neurobayes & \texttt{\textbackslash photos} & \photos & \texttt{\textbackslash powheg} & \powheg \\
\texttt{\textbackslash pythia} & \pythia & \texttt{\textbackslash resbos} & \resbos & \texttt{\textbackslash roofit} & \roofit \\
\texttt{\textbackslash root} & \root & \texttt{\textbackslash spice} & \spice & \texttt{\textbackslash urania} & \urania & \\
\texttt{\textbackslash herwiri} & \herwiri & \texttt{\textbackslash mc@nlo} & \mc@nlo \\
\end{tabular*}

\subsubsection{Languages}
\begin{tabular*}{\linewidth}{@{\extracolsep{\fill}}l@{\extracolsep{0.5cm}}l@{\extracolsep{\fill}}l@{\extracolsep{0.5cm}}l@{\extracolsep{\fill}}l@{\extracolsep{0.5cm}}l}
\texttt{\textbackslash cpp} & \cpp & \texttt{\textbackslash ruby} & \ruby & \texttt{\textbackslash fortran} & \fortran \\
\texttt{\textbackslash svn} & \svn &  \\
\end{tabular*}

\subsubsection{Data processing}
\begin{tabular*}{\linewidth}{@{\extracolsep{\fill}}l@{\extracolsep{0.5cm}}l@{\extracolsep{\fill}}l@{\extracolsep{0.5cm}}l@{\extracolsep{\fill}}l@{\extracolsep{0.5cm}}l}
\texttt{\textbackslash kbytes} & \kbytes & \texttt{\textbackslash kbsps} & \kbsps & \texttt{\textbackslash kbits} & \kbits \\
\texttt{\textbackslash kbsps} & \kbsps & \texttt{\textbackslash mbsps} & \mbsps & \texttt{\textbackslash mbytes} & \mbytes \\
\texttt{\textbackslash mbps} & \mbps & \texttt{\textbackslash mbsps} & \mbsps & \texttt{\textbackslash gbsps} & \gbsps \\
\texttt{\textbackslash gbytes} & \gbytes & \texttt{\textbackslash gbsps} & \gbsps & \texttt{\textbackslash tbytes} & \tbytes \\
\texttt{\textbackslash tbpy} & \tbpy & \texttt{\textbackslash dst} & \dst &  \\
\end{tabular*}

\subsection{Detector related}
\subsubsection{Detector technologies}
\begin{tabular*}{\linewidth}{@{\extracolsep{\fill}}l@{\extracolsep{0.5cm}}l@{\extracolsep{\fill}}l@{\extracolsep{0.5cm}}l@{\extracolsep{\fill}}l@{\extracolsep{0.5cm}}l}
\texttt{\textbackslash nonn} & \nonn & \texttt{\textbackslash ponn} & \ponn & \texttt{\textbackslash nonp} & \nonp \\
\texttt{\textbackslash cvd} & \cvd & \texttt{\textbackslash mwpc} & \mwpc & \texttt{\textbackslash gem} & \gem \\
\end{tabular*}

\subsubsection{Detector components, electronics}
\begin{tabular*}{\linewidth}{@{\extracolsep{\fill}}l@{\extracolsep{0.5cm}}l@{\extracolsep{\fill}}l@{\extracolsep{0.5cm}}l@{\extracolsep{\fill}}l@{\extracolsep{0.5cm}}l}
\texttt{\textbackslash tell1} & \tell1 & \texttt{\textbackslash ukl1} & \ukl1 & \texttt{\textbackslash beetle} & \beetle \\
\texttt{\textbackslash otis} & \otis & \texttt{\textbackslash croc} & \croc & \texttt{\textbackslash carioca} & \carioca \\
\texttt{\textbackslash dialog} & \dialog & \texttt{\textbackslash sync} & \sync & \texttt{\textbackslash cardiac} & \cardiac \\
\texttt{\textbackslash gol} & \gol & \texttt{\textbackslash vcsel} & \vcsel & \texttt{\textbackslash ttc} & \ttc \\
\texttt{\textbackslash ttcrx} & \ttcrx & \texttt{\textbackslash hpd} & \hpd & \texttt{\textbackslash pmt} & \pmt \\
\texttt{\textbackslash specs} & \specs & \texttt{\textbackslash elmb} & \elmb & \texttt{\textbackslash fpga} & \fpga \\
\texttt{\textbackslash plc} & \plc & \texttt{\textbackslash rasnik} & \rasnik & \texttt{\textbackslash elmb} & \elmb \\
\texttt{\textbackslash can} & \can & \texttt{\textbackslash lvds} & \lvds & \texttt{\textbackslash ntc} & \ntc \\
\texttt{\textbackslash adc} & \adc & \texttt{\textbackslash led} & \led & \texttt{\textbackslash ccd} & \ccd \\
\texttt{\textbackslash hv} & \hv & \texttt{\textbackslash lv} & \lv & \texttt{\textbackslash pvss} & \pvss \\
\texttt{\textbackslash cmos} & \cmos & \texttt{\textbackslash fifo} & \fifo & \texttt{\textbackslash ccpc} & \ccpc \\
\end{tabular*}

\subsubsection{Chemical symbols}
\begin{tabular*}{\linewidth}{@{\extracolsep{\fill}}l@{\extracolsep{0.5cm}}l@{\extracolsep{\fill}}l@{\extracolsep{0.5cm}}l@{\extracolsep{\fill}}l@{\extracolsep{0.5cm}}l}
\texttt{\textbackslash cfourften} & \cfourften & \texttt{\textbackslash cffour} & \cffour & \texttt{\textbackslash cotwo} & \cotwo \\
\texttt{\textbackslash csixffouteen} & \csixffouteen & \texttt{\textbackslash mgftwo} & \mgftwo & \texttt{\textbackslash siotwo} & \siotwo \\
\end{tabular*}

\subsection{Special Text }
\begin{tabular*}{\linewidth}{@{\extracolsep{\fill}}l@{\extracolsep{0.5cm}}l@{\extracolsep{\fill}}l@{\extracolsep{0.5cm}}l@{\extracolsep{\fill}}l@{\extracolsep{0.5cm}}l}
\texttt{\textbackslash eg} & \eg & \texttt{\textbackslash ie} & \ie & \texttt{\textbackslash etal} & \etal \\
\texttt{\textbackslash etc} & \etc & \texttt{\textbackslash cf} & \cf & \texttt{\textbackslash ffp} & \ffp \\
\texttt{\textbackslash vs} & \vs &  \\
\end{tabular*}


main.tex
\pdfoutput=1
% Uncomment line above if submitting to arXiv and using pdflatex

% $Id: main.tex 72989 2015-05-26 14:49:11Z rwallace $
% ============================================================================
% Purpose: Template for LHCb documents
% Authors: Tomasz Skwarnicki, Roger Forty, Ulrik Egede
% Created on: 2010-09-24
% ============================================================================
\documentclass[12pt,a4paper]{article}
% For two column text, add "twocolumn" as an option to the document
% class. Also uncomment the two "onecolumn" and "twocolumn" lines
% around the title page below.

% Variables that controls behaviour
\usepackage{ifthen} % for conditional statements
\newboolean{pdflatex}
\setboolean{pdflatex}{true} % False for eps figures 

\newboolean{articletitles}
\setboolean{articletitles}{true} % False removes titles in references

\newboolean{uprightparticles}
\setboolean{uprightparticles}{false} %True for upright particle symbols

\newboolean{inbibliography}
\setboolean{inbibliography}{false} %True once you enter the bibliography

\input{preamble}
%\usepackage{longtable} % only for template; not usually to be used in PAPERs

\begin{document}

%%%%%%%%%%%%%%%%%%%%%%%%%
%%%%% Title     %%%%%%%%%
%%%%%%%%%%%%%%%%%%%%%%%%%
\renewcommand{\thefootnote}{\fnsymbol{footnote}}
\setcounter{footnote}{1}

% %%%%%%% CHOOSE TITLE PAGE--------
%\onecolumn
% \input{title-LHCb-ANA}
%\input{title-LHCb-CONF}
\input{title-LHCb-PAPER}
%\twocolumn
% %%%%%%%%%%%%% ---------

\renewcommand{\thefootnote}{\arabic{footnote}}
\setcounter{footnote}{0}

%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
%%%%%  Table of Content   %%%%%%
%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
%%%% Uncomment next 2 lines if desired
%\tableofcontents
%\cleardoublepage


%%%%%%%%%%%%%%%%%%%%%%%%%
%%%%% Main text %%%%%%%%%
%%%%%%%%%%%%%%%%%%%%%%%%%

\pagestyle{plain} % restore page numbers for the main text
\setcounter{page}{1}
\pagenumbering{arabic}

%% Uncomment during review phase. 
%% Comment before a final submission.
%%\linenumbers

% You can include short sections directly in the main tex file.
% However, for larger papers it is desirable to split the text into
% several semiautonomous files, which can be revised independently.
% This is especially useful when developing a document in
% collaboration with several people, since then different parts can be
% edited independently.  This type of file organization is shown here.
% 

\input{introduction}

\input{detector}

%\input{layout}

%\input{typography}

\input{principles}

%\input{figures}

%\input{reference}

%\input{supplementary}

% Do not include this in analysis note and conference reports
\input{acknowledgements}

\input{appendix}

% This should be taken out in the final paper
%\input{supplementary-app}

\addcontentsline{toc}{section}{References}
\setboolean{inbibliography}{true}
\bibliographystyle{LHCb}
\bibliography{main,LHCb-PAPER,LHCb-CONF,LHCb-DP,LHCb-TDR}

\newpage

% Author List ----------------------------                                                                                                                                                                                                                                                                                                
%  You need to get a new author list!                                                                                                                                                                                                                                                                                                    

\input{LHCb_HD_authorlist_2015-01-13}
 
\newpage

\iffalse
\input{LHCb_authorlist.tex}

The author list for journal publications is provided by the Membership Committee shortly after 'approval to go to paper' has been given.
It will be sent to you by email shortly after a paper number has beens assigned.
The author list should be included already at first circulation,
to allow new members of the collaboration to verify whether they have been included correctly.
Occasionally a misspelled name is corrected or associated institutions become full members.
In that case, a new author list will be sent to you.
In case line numbering doesn't work well after including the authorlist, try moving the \verb!\bigskip! after the last author to a separate line.


The authorship for Conference Reports should be ``The LHCb                                                                                                                                                                                                                                                                                
  collaboration'', with a footnote giving the name(s) of the contact
  author(s), but without the full list of collaboration names.
\fi


\end{document}

preamble.tex
% THis file contains all the default packages and modifications for
% LHCb formatting

%% %%%%%%%%%%%%%%%%%%
%%  Page formatting
%% %%%%%%%%%%%%%%%%%%
\textheight=230mm
\textwidth=160mm
\oddsidemargin=7mm
\evensidemargin=-10mm
\topmargin=-10mm
\headsep=20mm
\columnsep=5mm
\addtolength{\belowcaptionskip}{0.5em}

\renewcommand{\textfraction}{0.01}
\renewcommand{\floatpagefraction}{0.99}
\renewcommand{\topfraction}{0.9}
\renewcommand{\bottomfraction}{0.9}


\setlength{\hoffset}{-2cm}
\setlength{\voffset}{-2cm}
% Page defaults ...
\topmargin=0.5cm
\oddsidemargin=2.5cm
\textwidth=16cm
\textheight=22cm
% Allow the page size to vary a bit ...
\raggedbottom
% To avoid Latex to be too fussy with line breaking ...
\sloppy

%% %%%%%%%%%%%%%%%%%%%%%%%
%% Packages to be used
%% %%%%%%%%%%%%%%%%%%%%%%% 
\usepackage{rotating} %allows use iof sidewaystable
\usepackage{microtype}
\usepackage{lineno}  % for line numbering during review
\usepackage{xspace} % To avoid problems with missing or double spaces after
                    % predefined symbold
\usepackage{caption} %these three command get the figure and table captions automatically small
\renewcommand{\captionfont}{\small}
\renewcommand{\captionlabelfont}{\small}

%% Graphics
\usepackage{graphicx}  % to include figures (can also use other packages)
\usepackage{color}
\usepackage{colortbl}
\graphicspath{{./figs/}} % Make Latex search fig subdir for figures

%% Math
\usepackage{amsmath} % Adds a large collection of math symbols
\usepackage{amssymb}
\usepackage{amsfonts}
\usepackage{upgreek} % Adds in support for greek letters in roman typeset

%% fix to allow peaceful coexistence of line numbering and
%% mathematical objects
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\expandafter\let\csname old#1\expandafter\endcsname\csname #1\endcsname
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end#1\endcsname
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% Get hyperlinks to captions and in references.
% These do not work with revtex. Use "hypertext" as class option instead.
\usepackage{hyperref}    % Hyperlinks in references
\usepackage[all]{hypcap} % Internal hyperlinks to floats.

\input{lhcb-symbols-def} % Add in the predefined LHCb symbols

% Ronan added packages
\usepackage{multirow}
\usepackage{bm}
% Make this the last packages you include before the \begin{document}
\usepackage{cite} % Allows for ranges in citations
\usepackage{mciteplus}

principles.tex
\section{Event selection}
\label{sec:selection}
Events considered in this analysis are selected by the muon trigger.
At the hardware stage, this trigger requires a muon with $\pt > 1.5\gevc$ and imposes an upper limit of 600 hits in the 
SPD sub-detector.
At the software stage, a muon with $\pt > 10\gevc$ is required. The muon track must also satisfy additional track quality 
criteria.
Candidate events are selected by requiring a pair of well-reconstructed particles of opposite
charge, identified as muons, that also pass the fiducial requirements~\cite{lhcbwz}.
In total, 58\,466 \PZ boson candidates are selected and their invariant mass distribution 
is shown in Fig.~\ref{fig:zmass}. 

\begin{figure}[h]
  \begin{center}
    \includegraphics[width=0.75\linewidth]{reco_mass_hist_2011}
  \end{center}
  \caption{Invariant mass of dimuon candidates.}
  \label{fig:zmass}
\end{figure}


The background contamination in the candidate sample is low. Five background sources are investigated: 
decays of heavy flavour hadrons, hadron misidentification, $\PZ\nolinebreak\rightarrow\nolinebreak\tau^{+}\tau^{-} $ decays, $t\bar{t}$ and 
$W^{+}W^{-}$ production.
Unlike muons from signal, muons arising from decays of heavy flavour hadrons are neither
directly produced at the primary interaction vertex, nor
are they isolated particles. Using the techniques
from Ref.~\cite{lhcbwz}, the contribution from this background is estimated 
from the data to be $227\pm32$ events, which amounts to 0.4$\%$ of the candidate sample.
The contribution from hadrons that decay in flight or have sufficient energy to traverse the calorimeters 
and be detected in the muon stations is studied 
in randomly triggered data, as described in Ref.~\cite{lhcbwz}, and determined to be $116\pm45$ events, which is 0.2$\%$ of the candidate sample.
Other electroweak and QCD backgrounds are estimated using \pythia 
simulation~\cite{pythia8} and normalised to the measured total 
cross-sections
for $\PZ\rightarrow\tau^{+}\tau^{-}$ decays~\cite{ATLAStautaumeas,CMStautaumeas}, $t\bar{t}$~\cite{ttbarATLAS,ttbarCMS} and 
$W^{+}W^{-}$~\cite{ATLASWWmeas,CMSWWmeas} production. The estimate for these sources is 
$66\pm6$ events, or 0.1$\%$ of the candidate sample. In total, the background is estimated to be $409\pm56$ events, or 0.7$\%$ 
of the candidate sample.

The purity, defined to be the ratio of signal to total candidate events, is 
$\rho$=0.993$\pm$0.002. 
It is assumed to be constant as a function of $y_{Z}$, $p_{T,Z}$ and $\phi^{*}_{Z}$.
A systematic uncertainty, discussed later, is assigned to allow for possible inaccuracies in this assumption.

\section{Cross-section measurement}
\label{sec:cs}

Cross-sections are quoted in the kinematic range defined by the measurement and are corrected 
for quantum electrodynamic (QED) final-state radiation (FSR) in order to 
provide a consistent 
comparison with NLO and NNLO QCD predictions.
No corrections are
applied for initial-state radiation, electroweak effects, nor their 
interplay
with QED effects.
The cross-section in a given bin $i$ of
$y_{Z}$, $p_{T,Z}$ or $\phi^{*}_{Z}$, with both final-state muons
inside the fiducial region, is measured as
\begin{equation}
 \label{eq:cs1}
 \sigma_{\PZ\rightarrow\mu^{+}\mu^{-}}(i) = \frac{\rho}{\mathcal{L}} \ \frac{f_{\rm FSR}(i)}{\varepsilon_{\rm GEC}(i)} 
 \sum_j U_{ij} \left( \sum_k \frac{1}{\varepsilon(\eta_{k}^{\mu^{+}},\eta_{k}^{\mu^{-}})}\right)_{j}.
\end{equation}
The indices $i$ and $j$ run over the bins of the variable under study.  
The index $k$ runs over the candidates contributing to bin $j$.
The total muon reconstruction efficiency for an event is given by
$\varepsilon(\eta_{k}^{\mu^{+}},\eta_{k}^{\mu^{-}})$, which is dependent on the pseudorapidity of the two muons. 
The matrix $U$ corrects the data for bin migrations due to detector resolution effects.
It is determined using an unfolding procedure, which is described in Section~\ref{sec:unfld}.
The efficiency of the
requirement on the number of SPD hits in the hardware trigger is denoted by $\varepsilon_{\rm GEC}$.
The correction factors for QED final-state radiation are denoted 
by $f_{\rm FSR}(i)$ and are
determined for each bin. The integrated luminosity is denoted by $\mathcal{L}$.
Though not entering the expression for the cross-section, an uncertainty due to the beam energy
is assigned to all cross-sections.
More detail on these individual components is given below.
Once the binned cross-sections are determined, they are summed to give the total cross-section
\begin{equation}
 \sigma_{\PZ\rightarrow\mu^{+}\mu^{-}}=\sum_i \sigma_{\PZ\rightarrow\mu^{+}\mu^{-}}(i).
\end{equation}
The most precise estimate of the total cross-section is obtained by summing 
the cross-sections as a function
of rapidity, where uncertainties due to data unfolding are negligible.

\subsection{Muon reconstruction efficiencies}

The data are corrected for efficiency losses due to track reconstruction, muon identification,
and trigger requirements. All efficiencies are determined from data using the techniques detailed in Refs.~\cite{lhcbwz,ze}, 
where the track reconstruction, muon identification, and muon trigger efficiencies
are obtained using tag-and-probe methods on the $\PZ$ resonance. 
The tag and probe tracks are required to satisfy the fiducial requirements.
The tag must be identified as a muon and be consistent with triggering the event, while the
probe is defined so that it is unbiased by the requirement for which the 
efficiency is being measured.
The efficiency is studied as a function of several variables, which 
describe both the muon kinematics
and the detector occupancy. In this analysis the efficiency as a function of muon $\eta$ is used. 
The efficiency in each bin of $\eta$ is defined as the fraction of tag-and-probe
candidate events where the probe satisfies a track reconstruction, identification or trigger requirement. 

The tracking efficiency is determined using probe tracks that are 
reconstructed by combining hits from the muon
stations and the large-area silicon-strip detector. 
%Hits from these sub-detectors are not used to find standard \lhcb tracks. 
The efficiency depends on $\eta$ and varies between 89.5$\%$ and 98.5$\%$ with uncertainties between 
0.4$\%$ and 1.9$\%$.

The muon identification efficiency is determined using probe tracks that are reconstructed without using the muon system.
The efficiency depends on $\eta$ and varies between 91.3$\%$ and 99.2$\%$ with
uncertainties between 0.1$\%$ and 0.9$\%$.        

The single-muon trigger efficiency is determined using reconstructed muons 
as probes. 
The efficiency depends on $\eta$ and varies between 71.6$\%$ and 82.0$\%$ with
uncertainties between 0.5$\%$ and 1.2$\%$.
Since only one muon candidate is required for the event to pass the trigger requirements, 
the overall trigger efficiency for the analysis is about 95$\%$. 

The efficiency to reconstruct any given event is taken to be the product of the three individual
efficiencies and determined on an event-by-event basis as a function of muon $\eta$,
\begin{equation}
 \varepsilon(\mu^{+},\mu^{-}) = \varepsilon_{\rm trk}^{\mu^{+}} \cdot \varepsilon_{\rm trk}^{\mu^{-}} \cdot \varepsilon_{\rm id}^{\mu^{+}} \cdot \varepsilon_{\rm id}^{\mu^{-}} \cdot \left( \varepsilon_{\rm trg}^{\mu^{+}} + \varepsilon_{\rm trg}^{\mu^{-}} - \varepsilon_{\rm trg}^{\mu^{+}} \cdot \varepsilon_{\rm trg}^{\mu^{-}} \right). 
\label{eq:effeqn}
\end{equation}
In Equation~\ref{eq:effeqn}, the efficiency $\varepsilon$ is written explicitly in terms of the muon tracking ($\varepsilon_{\rm trk}$), identification ($\varepsilon_{\rm id}$) and
trigger ($\varepsilon_{\rm trg}$) efficiencies. 
The average reconstruction efficiency for the analysis is about 85$\%$.
Effects that correlate the efficiency of the two muons are considered, but these are negligible at the current level of 
precision. 

\subsection{GEC efficiency}
\label{sec:gec}
The GEC efficiency is the efficiency of the SPD multiplicity limit at 600 hits in the muon trigger.
This efficiency is evaluated from data using two independent methods. The first
exploits the fact that the SPD multiplicities of single $pp$ interactions are always below the 600 hit threshold.
The expected SPD multiplicity distribution of signal events is constructed by adding the multiplicities
of signal events in single $pp$ interactions to the multiplicities of randomly triggered events, as in Ref.~\cite{lhcbwz}.
The convolution of the distributions extends to values above 600 hits, 
and the fraction of events that the trigger rejects can be determined.
The second method consists of fitting
the SPD multiplicity distribution and extrapolating the fit function to determine the fraction of events that are rejected,
as in Ref.~\cite{ze}. Both methods give consistent results and 
$\varepsilon_{\rm GEC} \nolinebreak=\nolinebreak (94.0 \pm 0.2)\%$ is used in this analysis. 
The central value is the estimate from the first method, while 
the difference between the two estimates contributes to the uncertainty. 
This efficiency depends linearly on
$y_{Z}$ with about 2$\%$ variation across the full range. A weaker dependence on both the $p_{T,Z}$ and $\phi^{*}_{Z}$ 
is also observed. Corrections for these effects are made. 

\subsection{Final-state radiation}

The FSR correction is taken to be the mean of the corrections calculated with \text{\sc Herwig++}~\cite{herwig} and \text{\sc Pythia8}~\cite{pythia8}. 
The corrections are tabulated in Appendix~\ref{sec:difftab} and are on average about 2.5$\%$. 

\subsection{Unfolding detector response}
\label{sec:unfld}
To correct for detector resolution effects, an unfolding is performed (matrix $U$ of Equation~\ref{eq:cs1}) using \lhcb 
simulation and the 
\text{\sc RooUnfold}~\cite{roounfold} software package.
%The simulated momentum is calibrated to the data since the momentum resolution is underestimated in the simulation.
The momentum resolution in the simulation is calibrated to the data.
The data are then unfolded using the iterative Bayesian approach proposed in Ref.~\cite{dagostini}.
Other unfolding techniques~\cite{svd,cowan} 
give similar results.
Additionally, all unfolding methods are tested for model
dependence using underlying distributions from leading order \pythia~\cite{pythia,pythia8}, leading order \text{\sc Herwig++}~\cite{herwig}, as well as 
NLO \powheg~\cite{powheg, powheg1, powheg2} showered with both \pythia and \herwig using the
\powheg matching scheme. 
The correction is on average about 2$\%$ as a function of $p_{T,Z}$, while 
it is significantly less as a function of $\phi^{*}_{Z}$.
Only the $p_{T,Z}$ and $\phi^{*}_{Z}$ distributions are unfolded. Since $y_{Z}$ is well measured, no 
unfolding is performed and $U$ is the identity matrix in this case. 

\subsection{Systematic uncertainties}
\label{sec:syst}

Sources of systematic uncertainty
and their effect on the total cross-section measurement are summarised in Table~\ref{tab:syst}.\footnote{Many of 
the systematic uncertainties quoted
here have a statistical component. The statistical uncertainty quoted on the measurement
is due to the number of observed \PZ candidates. In the case of unfolded measurements, the
statistical uncertainty is provided by the covariance matrix returned by \text{\sc RooUnfold}.}
The measured cross-sections as a function of $p_{T,Z}$ and $\phi^{*}_{Z}$ 
have additional systematic uncertainties
due to unfolding.
\begin{table}[h]
\caption{Contributions to the relative uncertainty on the total $\PZ$ boson cross-section.}
\label{tab:syst}
\begin{center}\begin{tabular}{lr}
    Source                           & Uncertainty ($\%$)  \\ \hline
    Statistical               & $0.39$ \\ \hline
    Trigger efficiency        & $  0.07 $          \\
    Identification efficiency & $  0.23 $         \\
    Tracking efficiency       & $  0.53 $           \\
    FSR                 & $  0.11 $                \\
    Purity              & $  0.22 $                 \\
    GEC efficiency            & $  0.26 $                  \\ \hline
    Systematic               & $0.68$                         \\ \hline
    Beam energy          & $1.25$    \\
    Luminosity          & $1.72$    \\ \hline
    Total                & $2.27$
  \end{tabular}\end{center}
\end{table}

The systematic uncertainty associated with the trigger, identification and tracking efficiencies is
determined by
re-evaluating all cross-sections
with the values of the individual efficiencies increased or decreased by one standard deviation. 
The full covariance matrix of the differential cross-section measurements is evaluated in this way
for each source of uncertainty separately. 
The covariance matrices for each source are added and the diagonal elements of the result determine
the total systematic uncertainty due to reconstruction efficiencies. These 
vary between
0.5 and 2.0$\%$ on the differential cross-section measurements.

The systematic uncertainty on the FSR correction is the quadratic sum of two components. The first is due
to the statistical precision of the \pythia and \text{\sc Herwig++} estimates and the second is half 
of the difference between their central values. The latter dominates, with the uncertainties on the differential
cross-sections varying between 0.3 and 3$\%$.

The systematic uncertainty on the purity is determined from the number of candidate and background events.   
In addition, an uncertainty based on the assumption that the purity
is the same for all variables and bins of the analysis is 
evaluated by comparing to cross-section measurements using
a binned purity, rather than a global one. The total uncertainties on the differential cross-section 
measurements due to variations in purity are typically less than 1$\%$.

The GEC efficiency is determined in each bin of $y_{Z}$, $p_{T,Z}$ and $\phi^{*}_{Z}$. The systematic uncertainty is the sum in quadrature of a 
component due to the available sample size in each bin and a component due to the 0.2$\%$ uncertainty on the integrated number, as determined in 
Section~\ref{sec:gec}. 
This varies between 0.4 and 4$\%$ across the differential measurements.

The systematic uncertainty due to unfolding is estimated by the differences between the differential cross-sections using Bayesian and matrix 
inversion unfolding techniques. The typical size is $1.5\%$.

The measurement is specified at centre-of-mass energy $\sqrt{s}$ = 7 \tev.
The beam energy, and consequently the centre-of-mass energy, is known to 0.65$\%$~\cite{BEAM}. 
The sensitivity of the cross-section 
to the centre-of-mass energy is studied using \dynnlo~\cite{dynnlo} and a systematic uncertainty of 1.25$\%$ is assigned.  

\section{Results} 
\label{sec:results}
\subsection{\emph{\textbf{Z}} boson production cross-section}
\label{sec:zresults}
The measured rapidity distribution as shown in Fig.~\ref{fig:diffxsecY} is 
compared to the prediction from \fewz~\cite{fewz,fewzold} with six different PDF sets.   
To compare the shapes of the differential cross-sections, measurements and
predictions are normalised to the total fiducial cross-section.
The normalised differential cross-sections are shown in 
Figs.~\ref{fig:diffxsecY},~\ref{fig:diffxsecPT} and~\ref{fig:diffxsecPHI}.
The measurements are compared to the predictions from \resbos~\cite{resbos1,resbos2,resbos3} and \powheg~\cite{powheg} where events
are interfaced with a parton shower that is simulated using \herwig~\cite{GEN-HERWIG1,GEN-HERWIG2}.
The $p_{T,Z}$ and $\phi^{*}_{Z}$ distributions are well described by \resbos and \powheg,
with the central values overestimating the data slightly at low $\phi^{*}_{Z}$ and underestimating slightly at high $\phi^{*}_{Z}$.
Comparisons to \mc@nlo + \herwiri and \mc@nlo + \herwig are shown in 
Figs.~\ref{fig:diffxsecHERWIRI_PT} and~\ref{fig:diffxsecHERWIRI_PHI}.
Here \herwig is configured with the root mean-square-deviation of the 
intrinsic $k_{T}$ distribution set to 0\gevc in
one instance and 2.2\gevc in another. The predictions straddle the measurement at low $p_{T,Z}$ and $\phi^{*}_{Z}$.
The high $p_{T,Z}$ and $\phi^{*}_{Z}$ tails are underestimated.

The total inclusive cross-section for $\PZ\rightarrow\mu^{+}\mu^{-}$ production for muons with $\pt \nolinebreak>\nolinebreak 20\nolinebreak\gevc$ in the
pseudorapidity region $2.0 < \eta < 4.5$ and the dimuon invariant mass range 
$60<M_{\mu^{+}\mu^{-}}<120\gevcc$ is measured to be
\begin{equation*}
 \sigma_{\PZ\rightarrow\mu^{+}\mu^{-}} = (76.0 \pm 0.3 \pm 0.5 \pm 1.0 \pm 1.3) \, \text{pb},
\end{equation*}
where the first uncertainty is statistical, the second systematic, the third is due to the beam energy
and the fourth is due to the luminosity.
The upper plot of Fig.~\ref{fig:totcs} shows agreement between this measurement and NNLO predictions given by \fewz
configured with various PDF sets.
The measurement also agrees with the measurements of the \PZ boson production cross-section performed in the
electron~\cite{ze} and tau lepton~\cite{ztau} channels but with a significantly smaller uncertainty.
All binned cross-sections are detailed in Tables~\ref{tab:csZY},~\ref{tab:csZPT} and~\ref{tab:csZPHI} of Appendix~\ref{sec:difftab}.

\subsection{Ratios of electroweak boson production cross-sections }
\label{sec:wzcomb}

The cross-section ratios   
are defined for muons with $\pt>20\gevc$, $2.0<\eta<4.5$ and, in the case of the \PZ boson cross-section, a dimuon
invariant mass between 60 and 120$\nolinebreak\gevcc$. 
The ratio of \PW boson to \PZ boson production
is defined as
\begin{equation}
R_{\it \PW\PZ} =
\frac{\sigma_{W^{+}\rightarrow\mu^{+}\nu_{\mu}}+\sigma_{W^{-}\rightarrow\mu^{-}\bar{\nu}_{\mu}}}{\sigma_{Z\rightarrow\mu^{+}\mu^{-}}}.
\end{equation}
The separate ratios of $W^{+}$ and $W^{-}$ to \PZ boson production cross-sections are defined as
\begin{equation}
R_{\it \PW^{\pm}\PZ} =
\frac{\sigma_{W^{\pm}\rightarrow\mu^{\pm}\nu_{\mu}}}{\sigma_{Z\rightarrow\mu^{+}\mu^{-}}},
\end{equation}
while the  \PW boson cross-section ratio is defined as
\begin{equation}
R_{\it \PW} = \frac{ \sigma_{W^{+}\rightarrow\mu^{+}\nu_{\mu}} } { \sigma_{W^{-}\rightarrow\mu^{-}\bar{\nu}_{\mu}}}.
\end{equation}

Many sources of systematic uncertainty cancel or are reduced in the ratios. As the data sets are identical, the largest 
single source of uncertainty 
on the individual cross-sections, due to the luminosity determination, is removed. The trigger used to select both samples
is identical and most of the uncertainty on the determination of the trigger efficiency cancels. In particular, the GEC
is common to both the \PW and \PZ boson 
analyses and it is 
expected that the size of the efficiency correction is similar for \PW and \PZ events. 
Cross-checks in data
and simulation support this assumption with a precision of approximately 0.3$\%$, which is included as a systematic 
uncertainty. The GEC efficiency was determined for the previous \PW boson 
measurement~\cite{wmu} to be 
$(95.9\pm1.1)\%$, whereas an improved precision of $(94.0\pm0.2)\%$ is obtained in the current analysis. Consequently, the \PW boson cross-section
results are updated to benefit from the more precise value. These results are listed in 
Tables~\ref{tab:csWETA},~\ref{tab:csrw} and~\ref{tab:csaw} 
of Appendix~\ref{sec:difftab}, along with the muon charge ratios
and asymmetries, and supersede those in Ref.~\cite{wmu}. 
The uncertainties on the tracking and muon identification partially cancel in the ratios of \PW 
and \PZ bosons. The uncertainty on the $W^{+}(W^{-})$ cross-section due to beam energy is 1.06(0.91)$\%$ and most of this uncertainty also cancels in the ratios. 
The uncertainties on the purities of the \PW and \PZ boson selections are uncorrelated.
The FSR uncertainties are taken to be uncorrelated.
The sources of uncertainty contributing to the determination of the ratios are summarised in Table~\ref{tab:wzsyst}.

\begin{table}[h]
\caption{Contributions to the relative uncertainty on the electroweak boson cross-section ratios.}

\label{tab:wzsyst}

\begin{center}\begin{tabular}{l c c c c}
    Source                           & \multicolumn{4}{c}{Uncertainty ($\%$)}  \\ \hline
                                        & $R_{\it \PW\PZ}$ & $R_{\it W^{+}\PZ}$ & $R_{\it W^{-}\PZ}$ & $R_{\it \PW}$ \\ \hline
    Statistical                         & $  0.45 $ & $  0.48 $ & $  0.50 $ & $  0.38 $           \\ \hline
    Trigger efficiency                        & $  0.15 $ & $  0.16 $ & $  0.13 $ & $  0.07 $           \\
    Identification efficiency                 & $  0.12 $ & $  0.12 $ & $  0.12 $ & $  0.03 $           \\
    Tracking efficiency                       & $  0.24 $ & $  0.23 $ & $  0.26 $ & $  0.08 $           \\
    FSR                                 & $  0.16 $ & $  0.21 $ & $  0.17 $ & $  0.21 $           \\
    Purity                              & $  0.41 $ & $  0.49 $ & $  0.55 $ & $  0.62 $           \\
    GEC efficiency                            & $  0.27 $ & $  0.28 $ & $  0.29 $ & $  0.18 $           \\ \hline
    Systematic                         & $  0.60 $ & $  0.67 $ & $  0.72 $ & $  0.69 $           \\ \hline           
    Beam energy                        & $  0.26 $ & $  0.19 $ & $  0.34 $ & $  0.15 $           \\ \hline
    Total                               & $  0.79 $ & $  0.85 $ & $  0.94 $ & $  0.80 $           \\

  \end{tabular}\end{center}
\end{table}

The dominant uncertainties on the ratios are due to the purity and the size of the sample. 
The correlation coefficients used in the 
uncertainty calculations are tabulated in Appendix~\ref{sec:correlation}.

The updated $W^{+}$ boson cross-section is 
$$\sigma_{W^{+}\rightarrow\mu^{+}\nu_{\mu}} = (878.0 \pm 2.1 \pm 6.7 \pm 9.3 \pm 15.0) \hspace{0.2cm} \text{pb},$$
where the uncertainties are due to the sample size, systematic effects, the beam energy and the luminosity determination.
The updated $W^{-}$ boson cross-section is
$$\sigma_{W^{-}\rightarrow\mu^{-}\bar{\nu}_{\mu}} = (689.5 \pm 2.0 \pm 5.3 \pm 6.3 \pm 11.8) \hspace{0.2cm} \text{pb}.$$
These measurements are in good agreement with the predictions of NNLO pQCD, as shown in Fig.~\ref{fig:totcs}.
Using the \PZ boson cross-section from Section~\ref{sec:zresults}, electroweak boson cross-section measurements
and theoretical predictions, with different parameterisations of the PDFs, are compared in Fig.~\ref{fig:ellipses}, with  
contours corresponding to the 68.3$\%$ confidence level.

The \PW to \PZ boson cross-section ratio is measured as $$R_{\it \PW\PZ} = 20.63\pm0.09\pm0.12\pm0.05,$$
where the first uncertainty is statistical, the second is systematic and the third is due to the beam energy.
The charged \PW to \PZ boson cross-section ratios are measured as 
\begin{align*}
R_{\it W^{+}\PZ} &= 11.56\pm0.06\pm0.08\pm0.02, \\
R_{\it W^{-}\PZ} &= \phantom{0}9.07\pm0.05\pm0.07\pm0.03,  
\end{align*}
while the \PW boson cross-section ratio is measured as $$R_{\it \PW} = 1.274\pm0.005\pm0.009\pm0.002.$$
These measurements, as well as their predictions, are displayed in Fig.~\ref{fig:ratiosummary}.
For $R_{\it \PW\PZ}$ and $R_{\it W^{+}\PZ}$, the data are well described by HERA1.5 and JR09, while
the values from CT10, MSTW08, NNPDF3.0 and ABM12 are larger than those measured. 
All PDF sets show good agreement for $R_{\it W^{-}\PZ}$.
As previously reported~\cite{wmu}, all PDF sets except ABM12 show good agreement for $R_{\it \PW}$. 
The $R_{\it \PW\PZ}$ and $R_{\it \PW}$ ratios are measured with a 
fractional uncertainty of $0.8\%$, which is similar both to 
the precision due to the PDFs
on the individual theoretical predictions and to the spread between the predictions. 
Considering the spread in the different predictions, the experimental measurements are in good agreement with SM predictions and can be used 
to improve the determination of the PDFs.

\begin{figure}[tbh]
  \begin{center}
    
\includegraphics[width=0.75\linewidth]{diff_xsection_y_fewz}\put(-40,215){(a)} \\
    \includegraphics[width=0.75\linewidth]{diff_xsection_y_norm}\put(-40,215){(b)}
  \end{center}
  \vspace{-1cm}\caption{
    %\small %captions should be a little bit smaller than main text
   (a) Differential cross-section as a function of $y_{Z}$ 
   compared with the prediction of \fewz configured with various PDF sets. 
   Different predictions are displaced horizontally for visibility.
   (b) Normalised differential cross-section as a function of $y_{Z}$ 
compared to the predictions of \resbos and \powheg + \herwig.
   The shaded (yellow) bands indicate the statistical and total 
uncertainties on the measurements, which are symmetric about the central value.
  }
  \label{fig:diffxsecY}
\end{figure}

\begin{figure}[tbh]
  \begin{center}
    \includegraphics[width=0.75\linewidth]{diff_xsection_pt_norm_high}\put(-40,215){(a)} \\
    \includegraphics[width=0.75\linewidth]{diff_xsection_pt_norm_low}\put(-40,215){(b)}
  \end{center}
  \vspace{-1cm}\caption{
    %\small %captions should be a little bit smaller than main text
   Normalised differential cross-section as a function of $p_{T,Z}$ on (a) logarithmic 
   and (b) linear scales.
   The shaded (yellow) bands indicate the statistical and total 
uncertainties on the measurements, which are symmetric about the central
value. The measurements are compared to the predictions of \resbos and \powheg + \herwig.
  }
  \label{fig:diffxsecPT}
\end{figure}

\begin{figure}[tbh]
  \begin{center}
    \includegraphics[width=0.75\linewidth]{diff_xsection_phi_norm_high}\put(-40,215){(a)} \\
    \includegraphics[width=0.75\linewidth]{diff_xsection_phi_norm_low}\put(-40,215){(b)}
  \end{center}
  \vspace{-1cm}\caption{
    %\small %captions should be a little bit smaller than main text
   Normalised differential cross-section as a function of $\phi^{*}_{Z}$ on (a) logarithmic
   and (b) linear scales.
   The shaded (yellow) bands indicate the statistical and total 
uncertainties on the measurements, which are symmetric about the central 
value. The measurements are compared to the predictions of \resbos and \powheg + \herwig. 
  }
  \label{fig:diffxsecPHI}
\end{figure}

\begin{figure}[tbh]
  \begin{center}
    \includegraphics[width=0.75\linewidth]{herwiri_pt_high}\put(-40,215){(a)} \\
    \includegraphics[width=0.75\linewidth]{herwiri_pt_low}\put(-40,215){(b)}
  \end{center}
  \vspace{-1cm}\caption{
    %\small %captions should be a little bit smaller than main text
   Normalised differential cross-section as a function of $p_{T,Z}$ on (a) logarithmic
   and (b) linear scales.
The shaded (yellow) bands indicate the statistical 
and total uncertainties on the measurements, which are symmetric about the 
central value. The measurements are compared to \mc@nlo + \herwig (HW) and 
\mc@nlo + \herwiri (HERWIRI). \herwig is configured with two choices of the 
root mean-square-deviation of the intrinsic $k_{T}$ distribution, 0 and 2.2 
\gevc.
  }
  \label{fig:diffxsecHERWIRI_PT}
\end{figure}

\begin{figure}[tbh]
  \begin{center}
    \includegraphics[width=0.75\linewidth]{herwiri_phi_high}\put(-40,215){(a)} \\
    \includegraphics[width=0.75\linewidth]{herwiri_phi_low}\put(-40,215){(b)}
  \end{center}
  \vspace{-1cm}\caption{
    %\small %captions should be a little bit smaller than main text
   Normalised differential cross-section as a function of $\phi^{*}_{Z}$ on (a) logarithmic
   and (b) linear scales.
The shaded (yellow) bands indicate the statistical        
and total uncertainties on the measurements, which are symmetric about the
central value. The measurements are compared to \mc@nlo + \herwig (HW) and 
\mc@nlo + \herwiri (HERWIRI). \herwig is configured with two choices of the 
root mean-square-deviation of the intrinsic $k_{T}$ distribution, 0 and 2.2 
\gevc.
  }
  \label{fig:diffxsecHERWIRI_PHI}
\end{figure}

\begin{figure}[tbh]
  \begin{center}
    \includegraphics[width=\linewidth]{CSS}
  \end{center}
  \caption{
    %\small %captions should be a little bit smaller than main text
   \lhcb measurements of electroweak boson production cross-sections compared to NNLO pQCD as implemented by the \fewz
   generator using various PDF sets.
   The shaded (yellow) bands indicate the statistical and total 
uncertainties on the measurements, which are symmetric about the central 
value.
  }
  \label{fig:totcs}
\end{figure}

\begin{figure}[tbh]
  \begin{center}
    \includegraphics[width=\linewidth]{CSE}
  \end{center}
  \caption{
   Two dimensional plots of electroweak boson cross-sections compared to NNLO predictions for various
   parameterisations of the PDFs. The outer, shaded (yellow) ellipse 
corresponds to the 
total uncertainty on the measurements. The inner, shaded (purple) ellipse 
excludes the beam energy and luminosity uncertainties. The uncertainty on the theoretical predictions corresponds to the PDF uncertainty only.
   All ellipses correspond to uncertainties at 68.3$\%$ confidence level.
 }
\label{fig:ellipses}
\end{figure}

\begin{figure}[tbh]
  \begin{center}   
    \includegraphics[width=\linewidth]{CSSR}
  \end{center}
  \caption{Ratios of electroweak boson production $R_{\it W^{+}Z}$, $R_{\it W^{-}Z}$, $R_{\it WZ}$, $R_{\it W}$, compared to 
various theoretical predictions.
    The shaded (yellow) bands indicate the statistical and total 
uncertainties 
on the measurements, which are symmetric about the central value.  
  }
  \label{fig:ratiosummary}
\end{figure}

\section{Conclusions} 
\label{sec:conclusions}

A measurement of the forward \PZ boson production cross-section at $\sqrt{s}$ = 7 \tev is presented, where
the \PZ bosons are reconstructed in the decay $Z\rightarrow\mu^{+}\mu^{-}$. The total cross-section 
in the fiducial range of the selection is in agreement with NNLO pQCD calculations. 
Normalised differential cross-sections as a function of $y_{Z}$, 
$\phi^{*}_{Z}$ and $p_{T,Z}$ are compared
to the predictions of various generators.
The increased precision on the determination of the event trigger efficiency motivates a re-evaluation of the
recently measured \PW boson production cross-section. These are presented here and supersede the values given in Ref.~\cite{wmu}.
Combining the \PZ boson cross-section with updated \PW boson cross-sections measured in a similar fiducial volume allows for
precision measurements of electroweak boson cross-section ratios. In particular, the \PW to \PZ boson
ratio is determined with a relative precision of $0.8\%$. The measured ratios are consistent with SM predictions
but are sensitive to the particular choice of PDF. Consequently, these results are expected to provide 
significant constraints on PDFs.

reference.tex
\section{References}
\label{sec:References}

References should be made using Bib\TeX~\cite{BibTeX}. A special style
\texttt{LHCb.bst} has been created to achieve a uniform
style. Independent of the journal the paper is submitted to, the
preprint should be created using this style. Where arXiv numbers
exist, these should be added even for published articles. In the PDF
file, hyperlinks will be created to both the arXiv and the published
version.

\begin{enumerate}

\item Citations are marked using square brackets, and the
  corresponding references should be typeset using Bib\TeX\ and the
  official \lhcb Bib\TeX\ style. An example is in
  Ref.~\cite{Sjostrand:2006za}.

\item For references with four or less authors all of the authors'
  names are listed~\cite{Majorana:1937vz}, otherwise the first author
  is given, followed by \etal. The \lhcb Bib\TeX\ style will
  take care of this.

\item The order of references should be sequential when reading the
  document. This is automatic when using Bib\TeX.

\item The titles of papers should in general be included. To remove
  them, change \texttt{\textbackslash
    setboolean\{articletitles\}\{false\}} to \texttt{true} at the top
  of this template.
  Note that the titles in \verb!LHCb-PAPER.bib! are in plain LaTex,
  in order to correspond to the actual title on the arXiv record.
  Some differences in style can thus be noticed with respect to the
  main text, for example particle names that use capital Greek letters
  are not slanted in the reference titles ($\Lambda$ vs \Lz)  

\item Whenever possible, use references from the supplied files
\verb!main.bib!, \verb!LHCb-PAPER.bib!, \verb!LHCb-CONF.bib!, and \verb!LHCB-DP.bib!.
These are kept up-to-date by the EB. If you see a mistake, do not edit these files,
but let the EB know. This way, for every update of the paper, you save
yourself the work of updating the references. Instead, you can just copy or
check in the latest versions of the \verb!.bib! files from the repository.   

\item For those references not provided by the EB, the best
  is to copy the Bib\TeX\ entry directly from
  \texttt{Inspire}. Often these need to be edited to get the 
  correct title, author names and formatting.
  For authors with multiple initials, add a space between them (change \texttt{R.G.C.} to \texttt{R. G. C.}),
  otherwise only the first initial will be taken. 
  Also, make sure to eliminate unnecessary capitalisation.
  Apart from that, the title should be respected as much as possible
  (\eg do not change particle names to PDG convention nor introduce/remove factors of $c$).
  Check that both the arXiv and the journal index are clickable
  and point to the right article.

%\item Even if the basic formatting of the Bib\TeX\ entry is taken from
%  \texttt{Inspire}, all the data should be cross checked against the
%  journal. Often there are minor changes to author initials or
%  titles. In case of a difference between the preprint and the
%  journal, the bibliographic information from the journal should be
%  used.

\item The \texttt{mciteplus}~\cite{mciteplus} package is used
  to enable multiple references to show up as a single item in the
  reference list. As an example \texttt{\textbackslash
    cite\{Mohapatra:1979ia,*Pascoli:2007qh\}} where the \texttt{*}
  indicates that the reference should be merged with the previous
  one. The result of this can be seen in
  Ref.~\cite{Mohapatra:1979ia,*Pascoli:2007qh}. Be aware that the
  \texttt{mciteplus} package should be included as the very last item
  before the \texttt{\textbackslash begin\{document\}} to work
  correctly.

\item It should be avoided to make references to public notes and
  conference reports in public documents. Exceptions can be discussed
  on a case-by-case basis with the review committee for the
  analysis. In internal reports they are of course welcome and can be
  referenced as seen in Ref.~\cite{LHCb-CONF-2011-003} using the
  \texttt{lhcbreport} category. For conference reports, omit the
  author field completely in the Bib\TeX\ record.

\item To get the typesetting and hyperlinks correct for \lhcb reports,
  the category \texttt{lhcbreport} should be used in the Bib\TeX\
  file. See Refs.~\cite{LHCb-INT-2011-047, *LHCb-ANA-2011-078,
    *CERN-THESIS-2014-057, *LHCb-PROC-2014-017, *LHCB-TALK-2014-257}
  for some examples. It can be used for \lhcb documents in the series
  \texttt{CONF}, \texttt{PAPER}, \texttt{PROC}, \texttt{THESIS},
  \texttt{LHCC}, \texttt{TDR} and internal \lhcb reports. Papers sent
  for publication, but not published yet, should be referred with
  their \texttt{arXiv} number, so the \texttt{PAPER} category should
  only be used in the rare case of a forward reference to a paper.

\item Proceedings can be used for references to items such as the
  \lhcb simulation~\cite{LHCb-PROC-2011-006}, where we do not yet have
  a published paper.

\end{enumerate}

There is a set of standard references to be used in \lhcb that are
listed in Appendix~\ref{sec:StandardReferences}.

supplementary-app.tex
\clearpage

\section{Supplementary material for LHCb-PAPER-2015-001}
\label{sec:Supplementary-App}

This appendix contains supplementary material that will posted
on the public cds record but will not appear in the paper.

\begin{figure}[tbh]
  \begin{center}
    \includegraphics[width=\linewidth]{universality}
  \end{center}
  \caption{Comparison of \lhcb \PZ cross-section measurements to theoretical prediction. The uncertainty due to the beam 
           energy is not displayed.}
  \label{fig:univ}
\end{figure}

\clearpage

\begin{figure}[tbh]
  \begin{center}
    \includegraphics[width=\linewidth]{diff_xsection_y_fewz_norm}
  \end{center}
  \caption{
    %\small %captions should be a little bit smaller than main text
   Normalised differential cross-section as a function of $y_{Z}$. The 
shaded (yellow) bands indicate
   the measurements. These are compared to \fewz with various PDF sets.
  }
  \label{fig:diffxsecYfewznorm}
\end{figure}

\clearpage

\begin{figure}[tbh]
  \begin{center}
    \includegraphics[width=\linewidth]{Results_CS_Z_ATLAS.pdf}
  \end{center}
  \caption{Extrapolation of \lhcb \PZ boson cross-section measurements to the ATLAS fiducial volume (muons with $\pt > 20$ \gevc and invariant mass $66<M_{\mu\mu}<116$ \gevcc)~\cite{atlaswz}.}
  \label{fig:extrap}
\end{figure}

\clearpage

\begin{figure}[tbh]
  \begin{center}
    \includegraphics[width=\linewidth]{herwiri_y}
  \end{center}
  \caption{
    %\small %captions should be a little bit smaller than main text
   Normalised differential cross-section as a function of \PZ boson $y$. 
The shaded (yellow) bands indicate
   the measurements, which are compared to \mc@nlo + \herwiri (HERWIRI) and 
\mc@nlo + \herwig (HW).
\herwig is configured with two choices of the root mean-square-deviation of 
the intrinsic $k_{T}$ distribution, 0 and 2.2 \gevc.
  }
  \label{fig:diffxsecYHERWIRI}
\end{figure}

\clearpage

\begin{figure}[tbh]
  \begin{center}
    \includegraphics[width=\linewidth]{CSW}
  \end{center}
  \caption{
          Differential $W^{+}$ and $W^{-}$ cross-sections as a function of 
muon $\eta$. Measurements, represented
          as bands corresponding to the statistical (orange (blue) for $W^{+}$ ($W^{-}$)) and total
          (yellow (light blue) for $W^{+}$ ($W^{-}$)) uncertainty, are compared to NNLO predictions with
          different parameterisations of the PDFs (black (blue) markers for $W^{+}$ ($W^{-}$)), displaced
          horizontally for presentation.
  }
  \label{fig:csw}
\end{figure}  

\clearpage

\begin{figure}[tbh]
  \begin{center}
    \includegraphics[width=\linewidth]{Results_CS_W_ATLAS.pdf}
  \end{center}
  \caption{
   Extrapolation of \lhcb \PW boson cross-section measurements to the ATLAS fiducial volume (muons with $\pt > 20$ \gevc
and invariant mass $66<M_{\mu\mu}<116$ \gevcc)~\cite{atlaswz}.
  }
  \label{fig:cswc}
\end{figure}

\clearpage

\begin{figure}[!t]
\begin{center}
\includegraphics[width=\textwidth]{./figs/Results_CSR_W.pdf}
\caption{\Wp to \Wm cross-section ratios as a function of muon $\eta$. 
Measurements, represented as bands corresponding 
to 
the (orange) statistical and (yellow) total uncertainty, are compared to (black markers, displaced horizontally for presentation) NNLO predictions with different parameterisations of the PDFs.}
\end{center}
\end{figure}

\clearpage
\begin{figure}[!t]
\begin{center}
\includegraphics[width=\textwidth]{./figs/Results_CSA_W.pdf}
\caption{Lepton charge asymmetries in \PW decays as a function of muon $\eta$. 
Measurements, represented as bands corresponding to 
the 
(orange) statistical and (yellow) total uncertainty, are compared to (open 
black markers, displaced horizontally for presentation) NNLO predictions with different parameterisations of the PDFs.}
\end{center}
\end{figure}

\clearpage
\begin{figure}[!t]
\begin{center}
\includegraphics[width=\textwidth]{./figs/Results_CSA_W_ATLAS.pdf}
\caption{Lepton charge asymmetries in \PW decays as a function of muon $\eta$. 
Measurements, represented as bands corresponding to 
the (yellow) total uncertainty, are extrapolated to the ATLAS fiducial 
volume ($M_{\textrm{T}} > 40\gevcc$ and $E_{\textrm{miss}} > 25\gev$) and 
compared to the (open black markers) ATLAS determinations~\cite{atlaswz}.}
\end{center}
\end{figure}

\clearpage
\begin{figure}[!t]
\begin{center}
\includegraphics[width=\textwidth]{./figs/Results_CSA_W_CMS.pdf}
\caption{Lepton charge asymmetries in \PW decays as a function of muon $\eta$. 
Measurements, represented as bands corresponding to 
the (yellow) total uncertainty, are extrapolated to the CMS fiducial volume 
($\pt > 25\gevc$) and compared to the (open black markers) CMS 
determinations~\cite{CMSAsymm}.} \end{center}
\end{figure}


\clearpage



supplementary.tex
\section{Inclusion of supplementary material}
\label{sec:Supplementary}

Three types of supplementary material should be distinguised:
\begin{itemize}
\item{A regular appendix: lengthy equations or long tables are sometimes
better put in an appendix in order not to interrupt the main flow of a paper.
Appendices will appear in the final paper, on arXiv
and on the cds record and should be considered integral
part of a paper, and are thus to be reviewed like the rest of the paper.
An example of an LHCb paper with an appendix is Ref.~\cite{LHCb-PAPER-2013-070}.
}
\item{Supplementary material for cds: plots or tables that 
would make the paper exceed the page limit or are
not appropriate to include in the paper itself,
but are desireable to be shown in public
should be added to the paper drafts in an appendix, and
removed from the paper before submitting to arXiv or the journal.
See Appendix~\ref{sec:Supplementary-App} for further instructions.
Examples are: comparison plots of the new result with older results,
plots that illustrate cross-checks.
An example of an LHCb paper with supplementary material for cds 
is Ref.~\cite{LHCb-PAPER-2013-035}.
Supplementary material for cds cannot be referenced to in the paper.
}
\item{Supplementary material for the paper. Most journals allow
to submit files along with the paper that will not be part of the
text of the article, but will be stored on the journal server.
Examples are plain text files with numerical data corresponding to the plots
in the paper. 
The supplementary material should be referenced to in the paper, by including a reference
of the type  ``See supplementary material for [give brief description of material].''
The journal will insert a specific link here. For the arXiv record, 
a specific link to the supplementary material on the arXiv server should be 
included when the paper gets updated, after it has been published.
For the internal reviewing, an appendix should be provided illustrating
the format of the file, its purpose and providing a link where the actual
files can be found.
An example of an LHCb paper with supplementary material is Ref.~\cite{LHCb-PAPER-2011-020}
}
\end{itemize}


title-LHCb-ANA.tex
% $Id: title-LHCb-ANA.tex 39841 2013-07-26 10:31:08Z roldeman $
% ===============================================================================
% Purpose: LHCb-ANA Note title page template
% Author: 
% Created on: 2010-10-05
% ===============================================================================

%%%%%%%%%%%%%%%%%%%%%%%%%
%%%%%  TITLE PAGE  %%%%%%
%%%%%%%%%%%%%%%%%%%%%%%%%
\begin{titlepage}

% Header ---------------------------------------------------
\vspace*{-1.5cm}

\hspace*{-0.5cm}
\begin{tabular*}{\linewidth}{lc@{\extracolsep{\fill}}r}
\ifthenelse{\boolean{pdflatex}}% Logo format choice
{\vspace*{-2.7cm}\mbox{\!\!\!\includegraphics[width=.14\textwidth]{lhcb-logo.pdf}} & &}%
{\vspace*{-1.2cm}\mbox{\!\!\!\includegraphics[width=.12\textwidth]{lhcb-logo.eps}} & &}
 \\
 & & LHCb-ANA-20XX-YYY \\  % ID 
 & & \today \\ % Date - Can also hardwire e.g.: 23 March 2010
 & & \\
\hline
\end{tabular*}

\vspace*{4.0cm}

% Title --------------------------------------------------
{\bf\boldmath\huge
\begin{center}
  A template for writing LHCb documents
\end{center}
}

\vspace*{2.0cm}

% Authors -------------------------------------------------
\begin{center}
U.~Egede$^1$.
\bigskip\\
{\it\footnotesize
$ ^1$Imperial College London, London, United Kingdom\\
}
\end{center}

\vspace{\fill}

% Abstract -----------------------------------------------
\begin{abstract}
  \noindent
  Guidelines for the preparation of LHCb documents are given. This is
  a ``living'' document, that should reflect our current practice. It
  is expected that these guidelines are implemented for papers already
  before they go into the first collaboration wide review. Please
  contact the Editorial Board chair if you have suggestions for
  modifications.
\end{abstract}

\vspace*{2.0cm}
\vspace{\fill}

\end{titlepage}


\pagestyle{empty}  % no page number for the title 

%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
%%%%%  EOD OF TITLE PAGE  %%%%%%
%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%

%  empty page follows the title page ----
\newpage
\setcounter{page}{2}
\mbox{~}

\cleardoublepage

title-LHCb-CONF.tex
% $Id: title-LHCb-CONF.tex 61931 2014-10-14 09:51:37Z roldeman $
% ===============================================================================
% Purpose: LHCb-CONF Note title page template
% Author: 
% Created on: 2010-09-25
% ===============================================================================

%%%%%%%%%%%%%%%%%%%%%%%%%
%%%%%  TITLE PAGE  %%%%%%
%%%%%%%%%%%%%%%%%%%%%%%%%
\begin{titlepage}

% Header ---------------------------------------------------
\vspace*{-1.5cm}

\hspace*{-0.5cm}
\begin{tabular*}{\linewidth}{lc@{\extracolsep{\fill}}r}
\ifthenelse{\boolean{pdflatex}}% Logo format choice
{\vspace*{-2.7cm}\mbox{\!\!\!\includegraphics[width=.14\textwidth]{lhcb-logo.pdf}} & &}%
{\vspace*{-1.2cm}\mbox{\!\!\!\includegraphics[width=.12\textwidth]{lhcb-logo.eps}} & &}
 \\
 & & LHCb-CONF-20XX-YYY \\  % ID 
 & & \today \\ % Date - Can also hardwire e.g.: 23 March 2010
 & & \\
\hline
\end{tabular*}

\vspace*{4.0cm}

% Title --------------------------------------------------
{\bf\boldmath\huge
\begin{center}
  A template for writing LHCb documents
\end{center}
}

\vspace*{2.0cm}

% Authors -------------------------------------------------
\begin{center}
The LHCb collaboration
   % Identify conference in the footnote
   \footnote{Conference report prepared for the 11th international conference on template editing, Aasiaat, Greenland, 1--3 June 2011.
   % Edit to contain the names of the one or two proponents
   Contact authors: Ulrik Egede, 
   \href{mailto:U.Egede@imperial.ac.uk}{U.Egede@imperial.ac.uk} and
   Raluca Muresan, 
   \href{mailto:raluca.muresan@cern.ch}{raluca.muresan@cern.ch}.
 }
\end{center}

\vspace{\fill}

% Abstract -----------------------------------------------
\begin{abstract}
  \noindent
  Guidelines for the preparation of LHCb documents are given. This is
  a ``living'' document, that should reflect our current practice. It
  is expected that these guidelines are implemented for papers already
  before they go into the first collaboration wide review. Please
  contact the Editorial Board chair if you have suggestions for
  modifications.
\end{abstract}

\vspace*{2.0cm}
\vspace{\fill}
{\footnotesize 
\centerline{\copyright~CERN on behalf of the \lhcb collaboration, licence \href{http://creativecommons.org/licenses/by/3.0/}{CC-BY-3.0}.}}
\vspace*{2mm}


\end{titlepage}


\pagestyle{empty}  % no page number for the title 

%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
%%%%%  EOD OF TITLE PAGE  %%%%%%
%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%

%  empty page follows the title page ----
\newpage
\setcounter{page}{2}
\mbox{~}

\cleardoublepage

title-LHCb-PAPER.tex
% $Id: title-LHCb-PAPER.tex 79639 2015-08-20 18:26:37Z rwallace $
% ===============================================================================
% Purpose: LHCb-PAPER journal paper title page template
% Author: 
% Created on: 2010-09-25
% ===============================================================================

%%%%%%%%%%%%%%%%%%%%%%%%%
%%%%%  TITLE PAGE  %%%%%%
%%%%%%%%%%%%%%%%%%%%%%%%%
\begin{titlepage}
\pagenumbering{roman}

% Header ---------------------------------------------------
\vspace*{-1.5cm}
\centerline{\large EUROPEAN ORGANIZATION FOR NUCLEAR RESEARCH (CERN)}
\vspace*{1.5cm}
\hspace*{-0.5cm}
\begin{tabular*}{\linewidth}{lc@{\extracolsep{\fill}}r}
\ifthenelse{\boolean{pdflatex}}% Logo format choice
{\vspace*{-1.5cm}\mbox{\!\!\!\includegraphics[width=.14\textwidth]{lhcb-logo.pdf}} & &}%
{\vspace*{-1.5cm}\mbox{\!\!\!\includegraphics[width=.12\textwidth]{lhcb-logo.eps}} & &}%
\\
 & & CERN-PH-EP-2015-102 \\  % ID 
 & & LHCb-PAPER-2015-001 \\  % ID 
 & & Aug 20, 2015 \\ % Date - Can also hardwire e.g.: 23 March 2010
 & & \\
% not in paper \hline
\end{tabular*}

\vspace*{0.85cm}

% Title --------------------------------------------------
{\bf\boldmath\huge
\begin{center}
Measurement of the forward \PZ boson \\ production cross-section \\ in $pp$ collisions at $\sqrt{s}$ = 7 \tev
\end{center}
}

\vspace*{0.15cm}

% Authors -------------------------------------------------
\begin{center}
%In the footnote, replace 'paper' by 'letter' in case of submission to PRL or PLB 
The LHCb collaboration\footnote{Authors are listed at the end of this paper.}
\end{center}

%\vspace{\fill}
\vspace{0.25cm}
% Abstract -----------------------------------------------
\begin{abstract}
  \noindent
A measurement of the production cross-section for \PZ bosons that decay to muons is presented. 
The data were recorded by the \lhcb detector during $pp$ collisions at a centre-of-mass 
energy of 7 \tev, and correspond to an integrated luminosity of 1.0 fb$^{-1}$.
The cross-section is 
measured for muons in the 
pseudorapidity range $2.0 \nolinebreak<\nolinebreak \eta \nolinebreak<\nolinebreak 4.5$ with 
transverse momenta $\pt \nolinebreak>\nolinebreak 20\gevc$. The dimuon mass  
is restricted to  
$60 \nolinebreak<\nolinebreak M_{\mu^{+}\mu^{-}} \nolinebreak<\nolinebreak 120\gevcc$. The measured cross-section is
$$\sigma_{Z\rightarrow\mu^{+}\mu^{-}} = (76.0 \pm 0.3 \pm 0.5 \pm 1.0 \pm 1.3) \, \text{pb}$$
where the uncertainties are due to the sample size, systematic effects, the beam energy and the luminosity.\enspace
This result is in good agreement with 
theoretical predictions at next-to-next-to-leading order in perturbative quantum
chromodynamics. The cross-section is also measured differentially as a function of kinematic variables 
of the \PZ boson. 
Ratios of the production cross-sections of electroweak bosons are presented
using updated \lhcb measurements of \PW boson production. 
A precise test of the Standard Model is provided by the measurement of the ratio
$$\frac{\sigma_{W^{+}\rightarrow\mu^{+}\nu_{\mu}} + \sigma_{W^{-}\rightarrow\mu^{-}\bar{\nu}_{\mu}}}{\sigma_{\PZ\rightarrow\mu^{+}\mu^{-}}} = 20.63\pm0.09\pm0.12\pm0.05,$$ 
where the uncertainty due to luminosity cancels.
  
\end{abstract}

\vspace*{0.3cm}

\begin{center}
  Published in JHEP \ 08 \ (2015) \ 039 
%/ Phys.~Rev.~D / Phys.~Rev.~Lett. / Phys.~Lett.~B / Eur.~Phys.~J.~C / Nucl.~Phys.~B 
\end{center}

\vspace{\fill}

{\footnotesize 
\centerline{\copyright~CERN on behalf of the \lhcb collaboration, licence \href{http://creativecommons.org/licenses/by/4.0/}{CC-BY-4.0}.}}
%\vspace*{2mm}

\end{titlepage}


%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
%%%%%  EOD OF TITLE PAGE  %%%%%%
%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%

%  empty page follows the title page ----
\newpage
\setcounter{page}{2}
\mbox{~}
%\newpage
%
%% Author List ----------------------------
%%  You need to get a new author list!
%\input{LHCb_authorlist.tex}
%
%The author list for journal publications is provided by the Membership Committee shortly after 'approval to go to paper' has been given.
%%It will be made available on the page
%%\verb!http://www.physik.uzh.ch/~strauman/forMemCo/LHCb-PAPER-XXXX-XXX/! .
%It will be sent to you by email shortly after a paper number has beens assigned.
%The author list should be included already at first circulation, 
%to allow new members of the collaboration to verify whether they have been included correctly.
%Occasionally a misspelled name is corrected or associated institutions become full members.
%In that case, a new author list will be sent to you.
%In case line numbering doesn't work well after including the authorlist, try moving the \verb!\bigskip! after the last author to a separate line.
%
%
%The authorship for Conference Reports should be ``The LHCb
%  collaboration'', with a footnote giving the name(s) of the contact
%  author(s), but without the full list of collaboration names.



\cleardoublepage








typography.tex
\section{Typography}
\label{sec:typography}

The use of the Latex typesetting symbols defined in the file
\texttt{lhcb-symbols-def.tex} and detailed in the appendices of this
document is strongly encouraged as it will make it much easier to
follow the recommendation set out below.

\begin{enumerate}

\item \lhcb is typeset with a normal (roman) lowercase b.

\item Titles are in bold face, and usually only the first word is
  capitalised.

\item Mathematical symbols and particle names should also be typeset
  in bold when appearing in titles.

\item Units are in roman type, except for constants such as $c$ or $h$
  that are italic: \gev, \gevcc.  The unit should be separated from
  the value with a thin space (``\verb!\,!''),
  and they should not be broken over two lines.
  Correct spacing is automatic when using predefined units inside math mode: \verb!$3.0\gev$! $\to 3.0\gev$.
  Spacing goes wrong when using predefined units outside math mode AND forcing extra space:
  \verb!3.0\,\gev! $\to$ 3.0\,\gev or worse:   \verb!3.0~\gev! $\to$ 3.0~\gev. 

\item  It is recommended to keep the factors of $c$ for masses and
  momenta, \eg $m = 3.1\gevcc$ (or $\gev c^{-2}$). However, if they are dropped this
  should be done consistently throughout, and a note should be added
  at the first instance to indicate that units are taken with $c=1$.

\item The \% sign should not be separated from the number that precedes it: 5\%, not 5 \%. 
A thin space is also acceptable: 5\,\%, but should be applied consistently throughout the paper.

\item Ranges should be formatted consistently. The recommendend form is to use a dash with no spacing around it: 
7--8\gev, obtained as \verb!7--8\gev!. 

\item Italic is preferred for particle names (although roman is
  acceptable, if applied consistently throughout).  Particle Data
  Group conventions should generally be followed: \Bd (no need for a
  ``d'' subscript), \decay{\Bs}{\jpsi\phi}, \Bsb,
  (note the long bar, obtained with \verb!\overline!, in contrast to the discouraged short \verb!\bar{B}! resulting in $\bar{B}$), \KS (note the
  uppercase roman type ``S''). 
This is most easily achieved by using the predefined symbols described in 
  Appendix~\ref{sec:listofsymbols}.
  Unless there is a good reason not to, the charge of a particle should be
  specified if there is any possible ambiguity 
  ($m(\Kp\Km)$ instead of $m(KK)$, which could refer to neutral kaons).

\item Decay chains can be written in several ways, depending on the complexity and the number of times it occurs. Unless there is a good reason not to, usage of a particular type should be consistent within the paper.
Examples are: 
$\Dsp\to\phi\pip$, with $\phi\to\Kp\Km$; 
$\Dsp\to\phi\pip$ ($\phi\to\Kp\Km$);  
$\Dsp\to\phi(\to\Kp\Km)\pip$; or
$\Dsp\to[\Kp\Km]_\phi\pip$.



\item Variables are usually italic: $V$ is a voltage (variable), while
  1 V is a volt (unit). Also in combined expressions: $Q$-value, $z$-scale, $R$-parity \etc

\item Subscripts and superscripts are roman type when they refer to a word (such as T
  for transverse) and italic when they refer to a variable (such as
  $t$ for time): \pt, \dms, $t_{\rm rec}$.

\item Standard function names are in roman type: \eg $\cos$, $\sin$
  and $\exp$.

\item Figure, Section, Equation, Chapter and Reference should be
  abbreviated as Fig., Sect. (or alternatively Sec.), Eq., Chap.\ and
  Ref.\ respectively, when they refer to a particular (numbered) item,
  except when they start a sentence. Table and Appendix are not
  abbreviated.  The plural form of abbreviation keeps the point after
  the s, \eg Figs.~1 and~2. Equations may be referred to either with 
  (``Eq.~(1)'') or without (``Eq.~1'') parentheses, 
  but it should be consistent within the paper.

\item Common abbreviations derived from Latin such as ``for example''
  (\eg), ``in other words'' (\ie), ``and so forth'' (\etc), ``and
  others'' (\etal), ``versus'' (\vs) can be used, with the typography
  shown, but not excessively; other more esoteric abbreviations should be avoided.
  

\item Units, material and particle names are usually lower case if
  spelled out, but often capitalised if abbreviated: amps (A), gauss
  (G), lead (Pb), silicon (Si), kaon (\kaon), but proton (\proton).

%\item The prefix for 1000 (k, \eg kV) should not be confused with
%  that used in computing (K, which strictly speaking denotes $2^{10}$,
%  \eg KB).

\item Counting numbers are usually written in words if they start a
  sentence or if they have a value of ten or below in descriptive
  text (\ie not including figure numbers such as ``Fig.\ 4'', or
  values followed by a unit such as ``4\,cm'').
  The word 'unity' can be useful to express the special meaning of
  the number one in expressions such as: 
``The BDT output takes values between zero and unity''.
% Numbers should not be
%  written as words if they by nature are real numbers that happen to
%  take an integer value, such as $\chisq/\rm{ndf} < 4$.

\item Numbers larger than 9999 have a comma (or a small space, but not both) between
  the multiples of thousand: \eg 10,000 or 12,345,678.  The decimal
  point is indicated with a point rather than a comma: \eg 3.141.

\item We apply the rounding rules of the
  PDG~\cite{PDG2014}. The basic rule states that if the three
  highest order digits of the uncertainty lie between 100 and 354, we round
  to two significant digits. If they lie between 355 and 949, we round
  to one significant digit. Finally, if they lie between 950 and 999,
  we round up and keep two significant digits. In all cases,
  the central value is given with a precision that matches that of the
  uncertainty. So, for example, the result $0.827 \pm 0.119$ should be
  written as $0.83\pm 0.12$, $0.827\pm 0.367$ should turn into
  $0.8\pm 0.4$, and $14.674\pm0.964$ becomes $14.7\pm1.0$.
 When writing numbers with uncertainty components from
  different sources, \ie statistical and systematic uncertainties, the rule
  applies to the uncertainty with the best precision, so $0.827\pm
  0.367\stat\pm 0.179\syst$ goes to $0.83\pm 0.37\stat\pm 0.18\syst$ and
  $8.943\pm 0.123\stat\pm 0.995\syst$ goes to $8.94\pm 0.12\stat\pm
  1.00\syst$.

\item When rounding numbers, it should be avoided to pad with zeroes
  at the end. So $51237 \pm 4561$ should be rounded as $(5.12 \pm 0.46)
  \times 10^4$ and not $51200 \pm 4600$.

\item When rounding numbers in a table, some variation of the rounding
  rules above may be required to achieve uniformity.

\item Hyphenation should be used where necessary to avoid ambiguity,
  but not excessively. For example: ``big-toothed fish''
  (to indicate that big refers to the teeth, not to the fish),
  but ``big white fish''.
  A compound modifier often requires hyphenation 
  (\CP-violating observables, \bquark-hadron decays, final-state radiation, second-order polynomial),
  even if the same combination in an adjective-noun combination does not
  (direct \CP violation, heavy \bquark hadrons, charmless final state).
  Adverb-adjective combinations are not hyphenated if the adverb ends with 'ly':
  oppositely charged pions, kinematically similar decay.
  Cross-section, cross-check, and two-dimensional are hyphenated.
  Semileptonic, pseudorapidity, pseudoexperiment, multivariate, multidimensional, reweighted, preselection, 
  nonresonant, nonzero, nonparametric, nonrelativistic, misreconstructed and misidentified
  are single words and should not be hyphenated.

\item Minus signs should be in a proper font ($-1$), not just hyphens
  (-1); this applies to figure labels as well as the body of the text.
  In Latex, use math mode (between \verb!$$!'s) or make a dash (``\verb!--!'').
  In ROOT, use \verb!#font[122]{-}! to get a normal-sized minus sign. 

\item Inverted commas (around a title, for example) should be a
  matching set of left- and right-handed pairs: ``Title''. The use of
  these should be avoided where possible.

\item Single symbols are preferred for variables in equations, \eg\
  \BF\ rather than BF for a branching fraction.

\item Parentheses are not usually required around a value and its
  uncertainty, before the unit, unless there is possible ambiguity: so
  $\dms = 20 \pm 2\invps$ does not need parentheses, whereas $f_d =
  (40 \pm 4)$\% or $x=(1.7\pm0.3)\times 10^{-6}$ does.
  The unit does not need to be repeated in
  expressions like $1.2 < E < 2.4\gev$.

\item The same number of decimal places should be given for all values
  in any one expression (\eg $5.20 < m_B < 5.34\gevcc$).

\item Apostrophes are best avoided for abbreviations: if the abbreviated term
  is capitalised or otherwise easily identified then the plural can simply add
  an s, otherwise it is best to rephrase: \eg HPDs, \pizs, pions, rather
  than HPD's, \piz's, $\pion$s.

\item Particle labels, decay descriptors and mathematical functions are not nouns, and need often to be followed by a noun. 
Thus ``background from $\Bd\to\pi^+\pi^-$ decays'' instead of ``background from $\Bd\to\pi^+\pi^-$'',
and ``the width of the Gaussian function'' instead of ``the width of the Gaussian''.

\item In equations with multidimensional integrations or differentiations, the differential terms should be separated by a thin space. 
Thus $\int f(x,y) dx\,dy$ instead $\int f(x,y) dxdy$ and
$\frac{d^2\Gamma}{dx\,dQ^2}$ instead of $\frac{d^2\Gamma}{dxdQ^2}$.
The d's are allowed in either roman or italic font, but should be consistent throughout the paper.


\end{enumerate}

main.bbl
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\bibitem{nnlopQCD2}
R.~Hamberg, W.~L. van Neerven, and T.~Matsuura,
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\bibitem{nnlopQCD3}
W.~L. van Neerven and E.~B. Zijlstra,
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R.~V. Harlander and W.~B. Kilgore,
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C.~Anastasiou, L.~J. Dixon, K.~Melnikov, and F.~Petriello,
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R.~S. Thorne, A.~D. Martin, W.~J. Stirling, and G.~Watt,
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{\mcitedefaultendpunct}{\mcitedefaultseppunct}\relax
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\bibitem{lhcbwz}
LHCb collaboration, R.~Aaij {\em et~al.},
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LHCb collaboration, R.~Aaij {\em et~al.},
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ATLAS collaboration, G.~Aad {\em et~al.},
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CMS collaboration, S.~Chatrchyan {\em et~al.},
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