| 1 | //  Classes to compute simple quantities for radio / 21 cm | 
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| 2 | //  R. Ansari - June 2010 | 
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| 3 |  | 
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| 4 | #ifndef RADUTIL_SEEN | 
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| 5 | #define RADUTIL_SEEN | 
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| 6 |  | 
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| 7 | #include "machdefs.h"      // SOPHYA .h | 
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| 8 | #include "sopnamsp.h"      // SOPHYA .h | 
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| 9 |  | 
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| 10 | #include "vector3d.h"      // conversion d'angle | 
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| 11 |  | 
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| 12 | class H21Conversions { | 
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| 13 | public: | 
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| 14 | // redshift nul, angle solide du pixel en steradian | 
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| 15 | H21Conversions(double freq=0., double opix=1.e-5); | 
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| 16 |  | 
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| 17 | double toJansky(double temp);  // Conversion d'une temperature (Kelvin) en jansky | 
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| 18 | double toKelvin(double jy);    // Conversion de Jansky en  temperature (Kelvin) | 
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| 19 |  | 
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| 20 | double Mean21cmTemperature_mK();      // Temperature moyenne de l'emission a 21 cm en mK | 
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| 21 | inline double T21cm_Kelvin() { return Mean21cmTemperature_mK()/1000.;  } | 
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| 22 | inline double T21cm_mK() { return Mean21cmTemperature_mK();  } | 
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| 23 |  | 
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| 24 | void setFrequency(double nu);  // on definit la frequence en MHz | 
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| 25 | inline void setRedshift(double z)    // on definit le redshift | 
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| 26 | { setFrequency(Freq021cm_Cst/(1+z)); } | 
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| 27 | inline void setLambda(double lam)    // on definit la longueur d'onde en m | 
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| 28 | { setFrequency(SpeedOfLight_Cst/lam); } | 
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| 29 |  | 
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| 30 | inline void setOmegaPix(double opix)   // angle solide en steradian | 
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| 31 | { omegapix_ = opix; } | 
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| 32 | inline void setOmegaPixDeg2(double opix)  // angle solide en Deg^2 | 
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| 33 | { double cf=Angle(1.,Angle::Degree).ToRadian(); omegapix_ = opix*cf*cf; } | 
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| 34 | inline void setOmegaPixArcmin2(double opix)  // angle solide en Arcmin^2 | 
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| 35 | { double cf=Angle(1.,Angle::ArcMin).ToRadian(); omegapix_ = opix*cf*cf; } | 
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| 36 |  | 
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| 37 | // Definition des parametres cosmologiques utiles pour le calcul de la temperature d'emission a 21 cm | 
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| 38 | // retourne la valeur de OmegaLambda (univers plat) | 
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| 39 | double setCosmoParam(double omegamatter=0.02581, double omegabaryon=0.0441, double h100=0.719, double fracHI=0.02); | 
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| 40 | inline void setFracHI(double fracHI=0.02) { fracHI_=fracHI; } | 
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| 41 |  | 
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| 42 | inline double getRedshift() { return z_; } | 
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| 43 | inline double getFrequency() { return freq_; } | 
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| 44 | inline double getLambda() { return lambda_; } | 
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| 45 |  | 
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| 46 | inline double getOmegaPix()   // angle solide en steradian | 
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| 47 | { return omegapix_; } | 
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| 48 | inline double getOmegaPixArcmin2()  // angle solide en Arcmin^2 | 
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| 49 | { double cf=Angle(1.,Angle::ArcMin).ToRadian(); return omegapix_/cf/cf; } | 
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| 50 | inline double getOmegaPixDeg2()  // angle solide en Deg^2 | 
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| 51 | { double cf=Angle(1.,Angle::Degree).ToRadian(); return omegapix_/cf/cf; } | 
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| 52 |  | 
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| 53 |  | 
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| 54 | static double SpeedOfLight_Cst;       // Speed of light  m/sec | 
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| 55 | static double Freq021cm_Cst;       // Speed of light  m/sec | 
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| 56 | static double k_Boltzman_Cst;         // Boltzmann constant  (SI Units) | 
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| 57 |  | 
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| 58 | double z_; | 
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| 59 | double freq_; | 
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| 60 | double lambda_; | 
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| 61 | double omegapix_; | 
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| 62 |  | 
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| 63 | // Parametres cosmologiques pour calcul du coefficient de conversion Mass to T21 | 
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| 64 | double OmegaMatter_; | 
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| 65 | double OmegaBaryons_; | 
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| 66 | double OmegaLambda_; | 
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| 67 | double h100_; | 
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| 68 | double fracHI_; | 
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| 69 | }; | 
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| 70 |  | 
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| 71 | #endif | 
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