Changeset 3516 in Sophya for trunk/Cosmo
- Timestamp:
- Sep 9, 2008, 5:50:12 PM (17 years ago)
- Location:
- trunk/Cosmo/SimLSS
- Files:
-
- 3 edited
Legend:
- Unmodified
- Added
- Removed
-
trunk/Cosmo/SimLSS/cmvdefsurv.cc
r3483 r3516 237 237 // On estime la valeur du redshift le plus grand 238 238 double bigred = redshift0 + dz/univ.Dhubble()*univ.E(redshift0) * nz/2.; 239 cout<<"big est redshift estimated to be "<<bigred<<endl;239 cout<<"biggest redshift estimated to be "<<bigred<<endl; 240 240 dzinc=bigred/100.; dzmax=dzinc*10.; 241 241 univ.SetInteg(perc,dzinc,dzmax,glorder); … … 287 287 cout<<"\n--- Cosmology for z = "<<redshift[i]<<endl; 288 288 univ.Print(redshift[i]); 289 cout<<"Nu(HI) = "<<Fr_HyperFin_Par*1000./(1.+redshift[i])<<" MHz"<<endl; 289 290 } 290 291 -
trunk/Cosmo/SimLSS/cmvobserv3d.cc
r3363 r3516 24 24 <<" -0 : use ComputeFourier0 method (defaut: no, use normal way)"<<endl 25 25 <<" -G typevol: compute Pk(z=0) and apply growth factor in real space"<<endl 26 <<" typevol=1 noiseevolved with distance / observateur (def)"<<endl27 <<" typevol=2 noiseevolved with distance to middle of Z planes"<<endl26 <<" typevol=1 evolved with distance / observateur (def)"<<endl 27 <<" typevol=2 evolved with distance to middle of Z planes"<<endl 28 28 <<" (default: no, spectrum Pk(z=z_median) for all cube)"<<endl 29 29 <<" -F : filter spectrum by pixel shape (0=no 1=yes(default)"<<endl -
trunk/Cosmo/SimLSS/genefluct3d.cc
r3365 r3516 779 779 // Using the correspondance between redshift and los comoving distance 780 780 // describe in vector "zred_" "loscom_" 781 // type_evol = 1 : evolution de la puissance du bruitavec la distance a l'observateur782 // 2 : evolution de la puissance du bruitavec la distance du plan Z781 // type_evol = 1 : evolution avec la distance a l'observateur 782 // 2 : evolution avec la distance du plan Z 783 783 // (tous les pixels d'un plan Z sont mis au meme redshift z que celui du milieu) 784 784 {
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