Changeset 3261 in Sophya for trunk/Cosmo/SimLSS/cmvobserv3d.cc
- Timestamp:
- Jun 4, 2007, 7:02:03 PM (18 years ago)
- File:
-
- 1 edited
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trunk/Cosmo/SimLSS/cmvobserv3d.cc
r3252 r3261 435 435 cout<<"1+rgen: ("<<nm<<") Mean = "<<rm<<", Sigma^2 = " 436 436 <<rs2<<" -> "<<sqrt(rs2)<<endl; 437 nm = fluct3d.MeanSigma2(rm,rs2,0.,1e200,true,0.); 438 cout<<"1+rgen with_neg_a_zero: ("<<nm<<") Mean = "<<rm<<", Sigma^2 = " 439 <<rs2<<" -> "<<sqrt(rs2)<<endl; 437 440 PrtTim(">>>> End Converting fluctuations into mass"); 438 441 … … 441 444 cout<<rm<<" galaxies put into survey"<<endl; 442 445 nm = fluct3d.MeanSigma2(rm,rs2,0.); 443 cout<<"galaxy: ("<<nm<<") Mean = "<<rm<<", Sigma^2 = " 446 cout<<"galaxy mass: ("<<nm<<") Mean = "<<rm<<", Sigma^2 = " 447 <<rs2<<" -> "<<sqrt(rs2)<<endl; 448 nm = fluct3d.MeanSigma2(rm,rs2,0.,1e200,true,0.); 449 cout<<"galaxy mass with_neg_a_zero: ("<<nm<<") Mean = "<<rm<<", Sigma^2 = " 444 450 <<rs2<<" -> "<<sqrt(rs2)<<endl; 445 451 PrtTim(">>>> End Converting mass into galaxy number"); 446 452 447 cout<<"\n--- Set negative pixels to BAD"<<endl;453 cout<<"\n--- Set negative and null pixels to BAD"<<endl; 448 454 nm = fluct3d.SetToVal(0.,1e+200,-999.); 449 455 cout<<nm<<" negative in survey set to BAD"<<endl; 450 456 nm = fluct3d.MeanSigma2(rm,rs2,-998.); 451 cout<<"galaxy : ("<<nm<<") Mean = "<<rm<<", Sigma^2 = "457 cout<<"galaxy mass: ("<<nm<<") Mean = "<<rm<<", Sigma^2 = " 452 458 <<rs2<<" -> "<<sqrt(rs2)<<endl; 453 459 PrtTim(">>>> End Set negative pixels to BAD etc..."); … … 457 463 cout<<nm<<" galaxies into survey after poisson"<<endl; 458 464 nm = fluct3d.MeanSigma2(rm,rs2,-998.); 459 cout<<"galaxy: ("<<nm<<") Mean = "<<rm<<", Sigma^2 = " 465 cout<<"galaxy number: ("<<nm<<") Mean = "<<rm<<", Sigma^2 = " 466 <<rs2<<" -> "<<sqrt(rs2)<<endl; 467 nm = fluct3d.MeanSigma2(rm,rs2,0.,1e200,true,0.); 468 cout<<"galaxy number with_neg_a_zero: ("<<nm<<") Mean = "<<rm<<", Sigma^2 = " 460 469 <<rs2<<" -> "<<sqrt(rs2)<<endl; 461 470 PrtTim(">>>> End Apply poisson on galaxy number"); … … 474 483 double mhi = fluct3d.TurnNGal2Mass(tirhmdndm,true); 475 484 cout<<mhi<<" MSol in survey / "<<mass_by_mpc3*fluct3d.GetVol()<<endl; 476 nm = fluct3d.MeanSigma2(rm,rs2, 0.);485 nm = fluct3d.MeanSigma2(rm,rs2,-998.); 477 486 cout<<"HI mass: ("<<nm<<") Mean = "<<rm<<", Sigma^2 = " 478 487 <<rs2<<" -> "<<sqrt(rs2)<<endl; 479 488 cout<<"Equivalent: "<<rm*nm/fluct3d.NPix()<<" Msol / pixels"<<endl; 489 nm = fluct3d.MeanSigma2(rm,rs2,0.,1e200,true,0.); 490 cout<<"HI mass with_neg_a_zero: ("<<nm<<") Mean = "<<rm<<", Sigma^2 = " 491 <<rs2<<" -> "<<sqrt(rs2)<<endl; 480 492 PrtTim(">>>> End Convert Galaxy number to HI mass"); 481 493
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