Changeset 3200 in Sophya for trunk/Cosmo/SimLSS


Ignore:
Timestamp:
Apr 6, 2007, 3:00:38 PM (18 years ago)
Author:
cmv
Message:

add commentary for users cmv 06/04/2007

File:
1 edited

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  • trunk/Cosmo/SimLSS/cmvobserv3d.cc

    r3199 r3200  
    2121{
    2222 cout<<"cmvobserv3d [...options...]"<<endl
    23      <<" -a : init auto de l aleatoire"<<endl
    24      <<" -0 : use methode ComputeFourier0"<<endl
     23     <<" -a : auto init random seed (needed for multiple simul)"<<endl
     24     <<" -0 : use ComputeFourier0 method (defaut: no, use normal way)"<<endl
    2525     <<" -G : compute Pk(z=0) and apply growth factor in real space"<<endl
    26      <<" -x nx,dx : taille en x (npix,Mpc)"<<endl
    27      <<" -y ny,dy : taille en y (npix,Mpc)"<<endl
    28      <<" -z nz,dz : taille en z (npix,Mpc)"<<endl
    29      <<" -Z zref : redshift median"<<endl
    30      <<" -s snoise : sigma du bruit en Msol"<<endl
    31      <<" -2 : compute 2D spectrum"<<endl
     26     <<"      (default: no, spectrum Pk(z=z_median) for all cube)"<<endl
     27     <<" -x nx,dx : size along x axis (npix,Mpc)"<<endl
     28     <<" -y ny,dy : size along y axis (npix,Mpc)"<<endl
     29     <<"            if ny or dy <=0 take same value as for x"<<endl
     30     <<" -z nz,dz : size along z axis (redshift axis, npix,Mpc)"<<endl
     31     <<" -Z zref : redshift for the center of the simulation cube"<<endl
     32     <<" -s snoise : gaussian noise sigma in equivalent Msol"<<endl
     33     <<" -2 : compute also 2D spectrum (default: no)"<<endl
    3234     <<" -M schmin,schmax,nsch : min,max mass and nb points for schechter HI"<<endl
    33      <<" -A <log10(S_agn en Jy)>,sigma,powlaw : distribution des AGN par pixel"<<endl
    34      <<" -K : on utilise le calcul de spectre bricole pour les AGN (bidon!)"<<endl
    35      <<" -W : write cube in FITS format"<<endl
     35     <<" -A <log10(S_agn in Jy at 1.4 GHz)>,sigma,powlaw :"<<endl
     36     <<"    AGN mean and sigma gaussian equiv. distrib. for solid angle of centeral pixel"<<endl
     37     <<"    powlaw: apply S_agn evolution as (Nu/1.4)^powlaw"<<endl
     38     <<" -W : write cube in FITS format (complex cube is coded as real cube)"<<endl
    3639     <<" -P : write cube in PPF format"<<endl
    37      <<" -V : compute variance from real space"<<endl
     40     <<" -V : compute variance from real space (for check, default: no)"<<endl
     41     <<" -K : use power spectrum computation adapted for AGN (bidon!)"<<endl
    3842     <<endl;
    3943}
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