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

2. ============  Spectrum Calculation ======================
For computing the spectrum we rely on NMSSMTools.
Two options are available,  mSUGRA and LowScaleInput depending whether input 
parameters are defined at the GUT scale or at the EWSB scale. 
To work with LowScaleInput comment the
    #define SUGRA 
instruction at the  top of main.c [main.F].

Example of SUGRA call 
   ./main 1000 130 -1500 10 0.1 -50 1 171.4
and for  LowScaleInput
   ./main data1.par

In both cases if you launch 'main' without parameters, the parameters needed are
specified on the screen. 

3. ======= Special citations ========
  
  %\cite{Belanger:2005kh}
\ \bibitem{Belanger:2005kh}
  G.~Belanger, F.~Boudjema, C.~Hugonie, A.~Pukhov and A.~Semenov,
  %``Relic density of dark matter in the NMSSM,''
  JCAP {\bf 0509} (2005) 001
  [arXiv:hep-ph/0505142].
  %%CITATION = JCAPA,0509,001;%%


  %\cite{Ellwanger:2006rn}
  \bibitem{Ellwanger:2006rn}
  U.~Ellwanger and C.~Hugonie,
  %``NMSPEC: A Fortran code for the sparticle and Higgs masses in the NMSSM with
  %GUT scale boundary conditions,''
  Comput.\ Phys.\ Commun.\  {\bf 177} (2007) 399
  [arXiv:hep-ph/0612134].
  %%CITATION = CPHCB,177,399;%%

