Citations guide for ROOT files 2013-2016:
If you use numbers provided on this webpage you must cite the following papers:

    HIGLU program
        Spira:1995mt 
    SusHi program
        Harlander:2012pb 
    FeynHiggs program
        Heinemeyer:1998yj, Heinemeyer:1998np, Degrassi:2002fi, Frank:2006yh, Hahn:2013ria 
    ggH@NNLO program
        Harlander:2002wh 
    bbh@nnlo (5FS) program
        Harlander:2003ai 
    bbH NLO (4FS)
        Dittmaier:2003ej, Dawson:2003kb 
    ggH NLO massive
        Spira:1995rr 
    ggH NNLO for scalar Higgs
        Anastasiou:2002yz, Ravindran:2003um 
    ggH NNLO for pseudoscalar Higgs
        Harlander:2002vv, Anastasiou:2002wq 
    Electroweak corrections by light fermions
        Aglietti:2004nj, Bonciani:2010ms 
    (N)NLO (S)QCD corrections for h/H/A
        Harlander:2004tp (NLO-stop scalar mh=0)
        Harlander:2005rq (NLO-top/bottom)
        Degrassi:2010eu (NLO-sbottom scalar)
        Degrassi:2011vq (NLO-stop/sbottom pseudo mA != 0)
        Degrassi:2012vt (NLO-stop scalar mH != 0) 
    HDECAY
        Djouadi:1997yw, Djouadi:2006bz 
    Last but not least acknowledge the work of the BR subgroup, which is based upon the publications given in this tex-file. 

Example usage of references in public document:

In the first place, please cite the LHC Higgs cross-section working group for providing cross-sections and BRs (by citing the Yellow Reports).

For all except the hMSSM, Higgs masses and mixing (and effective Yukawa couplings) have been calculated with Feynhiggs [3].

Cross sections:

    For the gluon-fusion process inclusive cross sections are obtained with SusHi [2], which includes NLO supersymmetric-QCD corrections [7,11], N^3LO QCD corrections for the top-quark contribution in the effective theory of a heavy top quark [4,8,9,tbc] and electroweak effects by light quarks [10]. (HIGLU [1] is used for "classic" mhmax scenario - see details below.) 

    For the bbH process we now use the SCET/FONLL scheme provided by the bbh subgroup. Outdated cross sections are the five flavour NNLO QCD inclusive cross sections calculated with SusHi [2] based on bbh@nnlo [5] and the four flavour NLO QCD calculation [6]. 

Branching ratios:

Whereas in the hMSSM branching ratios are solely computed with HDECAY [12], all other scenarios combine the most precise results of HDECAY [12], FeynHiggs [3] and PROPHECY4f. Relevant references are listed in [13], see LHCHXSWG-2015-002, page 10 bottom, for an example how to cite them.