Changeset 3261 in Sophya for trunk/Cosmo/SimLSS/cmvdefsurv.cc
- Timestamp:
- Jun 4, 2007, 7:02:03 PM (18 years ago)
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- 1 edited
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trunk/Cosmo/SimLSS/cmvdefsurv.cc
r3252 r3261 301 301 <<","<<hifactor*Msol2FluxHI(mhiref,dlumlim[1])<<"] W/m^2"<<endl; 302 302 double sfhi = fhi / (dnuhiz*1e9) / Jansky2Watt_cst; 303 cout<<"If spread over "<<dnuhiz<<" GHz, flux density = "<<sfhi<<" Jy"<<endl;303 cout<<"If spread over pixel depth ("<<dnuhiz<<" GHz), flux density = "<<sfhi<<" Jy"<<endl; 304 304 305 305 // --- Signal analysis … … 337 337 cout<<"Synchrotron: T="<<Tsynch408<<" K ("<<nuhaslam<<" GHz), " 338 338 <<tsynch<<" K ("<<nuhiz<<" GHz)"<<endl 339 <<" P="<<psynch<<" W "<<endl;340 cout<<" flux density = "<<ssynch<<" Jy "<<endl;339 <<" P="<<psynch<<" W for pixel"<<endl; 340 cout<<" flux density = "<<ssynch<<" Jy for pixel solid angle"<<endl; 341 341 342 342 // CMB … … 345 345 double pcmb = facpolar * planck(nuhiz*1.e+9) * surfeff * angsol * (dnuhiz*1e9); 346 346 double scmb = pcmb / surfeff / (dnuhiz*1.e+9) / Jansky2Watt_cst; 347 cout<<"CMB: T="<<tcmb<<" K -> P="<<pcmb<<" W "<<endl;348 cout<<" flux density = "<<scmb<<" Jy "<<endl;347 cout<<"CMB: T="<<tcmb<<" K -> P="<<pcmb<<" W for pixel"<<endl; 348 cout<<" flux density = "<<scmb<<" Jy for pixel solid angle"<<endl; 349 349 350 350 // AGN
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