1. ============  read  ../README ===========

2. ============ Spectrum calculation =======
 We rely on CPsuperH for computing the spectrum
 and HiggsBounds for accelerator constraints
  
3. ======= Special citations ========

%\cite{Belanger:2006qa}
\bibitem{Belanger:2006qa}
G.~Belanger, F.~Boudjema, S.~Kraml, A.~Pukhov and A.~Semenov,
%``Relic density of neutralino dark matter in the MSSM with CP violation,''
arXiv:hep-ph/0604150.

CPsuperH:

%\cite{Lee:2003nt}
\bibitem{Lee:2003nt}
J.~S.~Lee, A.~Pilaftsis, M.~Carena, S.~Y.~Choi, M.~Drees, J.~R.~Ellis and C.~E.~M.~Wagner,
%``CPsuperH: A computational tool for Higgs phenomenology in the minimal
%supersymmetric standard model with explicit CP violation,''
Comput.\ Phys.\ Commun.\  {\bf 156} (2004) 283
[arXiv:hep-ph/0307377].


HiggsBounds
%\cite{Bechtle:2008jh}
\bibitem{Bechtle:2008jh}
  P.~Bechtle, O.~Brein, S.~Heinemeyer, G.~Weiglein and K.~E.~Williams,
  %`HiggsBounds: Confronting Arbitrary Higgs Sectors with Exclusion Bounds
  %from
  %LEP and the Tevatron,''
  Comput.\ Phys.\ Commun.\  {\bf 181} (2010) 138
  [arXiv:0811.4169 [hep-ph]].
