are given in the table below (to be used with Version ≥ 1.7.0).
Our input involves A_t, A_b and A_τ instead of X_t.
A_t = A_b (= A_τ) = X_t + μ / tan(β).
The values of X_t and μ are provided in the tables.
A_τ needs to be adjusted in the M_h^125, M_h^125(χ) scenarios.
is set to N^3LO through setting blockentry SUSHI(5) to 3.
SusHi needs to be compiled with "make predef=FHINT".
the choice of the SUSY spectrum in each point of the plane and tar.gz-files with the corresponding SusHi input files.
are given in the tables below (to be used with Version ≥ 1.0.4).
The values of X_t are provided in the tables.
compatible with the light Higgs at 125GeV in zipped form here.
It is named 'lowtanb' scenario and the file names contain the values of M_A and tan(β)*10.