- Timestamp:
- Apr 6, 2007, 3:00:38 PM (18 years ago)
- File:
-
- 1 edited
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trunk/Cosmo/SimLSS/cmvobserv3d.cc
r3199 r3200 21 21 { 22 22 cout<<"cmvobserv3d [...options...]"<<endl 23 <<" -a : init auto de l aleatoire"<<endl24 <<" -0 : use methode ComputeFourier0"<<endl23 <<" -a : auto init random seed (needed for multiple simul)"<<endl 24 <<" -0 : use ComputeFourier0 method (defaut: no, use normal way)"<<endl 25 25 <<" -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 32 34 <<" -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 36 39 <<" -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 38 42 <<endl; 39 43 }
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