Changeset 3557 in Sophya

Timestamp:

Dec 19, 2008, 5:22:23 PM (17 years ago)

Author:

cmv

Message:

juste qques details de cosmetique, cmv 19/12/2008

Location:

trunk/Cosmo/SimLSS

Files:

• cmvdefsurv.cc (modified) (1 diff)
• cmvobserv3d.cc (modified) (1 diff)

trunk/Cosmo/SimLSS/cmvdefsurv.cc

@@ -754 +754 @@
      cout<<"\n...Observation limits for a N (large) telescope interferometer (with complex correlator)"<<endl
          <<"     (weak source limit sensitivity in a synthetised image)"<<endl
-         <<"     Also valid for a single dish telescope"<<endl
+         <<"     Also valid for a single dish telescope(with collecting area N*A)"<<endl
          <<"          (add factor sqrt(2) if ON-OFF with T_ON=t_OFF)"<<endl;
    } else continue;

trunk/Cosmo/SimLSS/cmvobserv3d.cc

@@ -24 +24 @@
      <<" -0 : use ComputeFourier0 method (defaut: no, use normal way)"<<endl
      <<" -G typevol: compute Pk(z=0) and apply growth factor in real space"<<endl
-     <<"             typevol=1 evolved with distance / observateur (def)"<<endl
-     <<"             typevol=2 evolved with distance to middle of Z planes"<<endl
-     <<"      (default: no, spectrum Pk(z=z_median) for all cube)"<<endl
+     <<"       typevol=1 evolved with distance / observateur (def)"<<endl
+     <<"       typevol=2 evolved with distance to middle of Z planes"<<endl
+     <<"       else : no evol, spectrum Pk(z=z_median) for all cube (def)"<<endl
      <<" -F : filter spectrum by pixel shape (0=no 1=yes(default)"<<endl
      <<" -U typ =0 compute <NGal>, poisson fluctuate then convert to HI mass (def)"<<endl