void PanDustSystem::setupSelfBefore()
{
DustSystem::setupSelfBefore();
// if there is no dust emission, turn off the irrelevant flags just to be sure
if (!_dustemissivity)
{
setDustLib(0);
setSelfAbsorption(false);
setWriteTemperature(false);
setWriteISRF(false);
setWriteEmissivity(false);
}
// if there is dust emission, make sure that there is a dust library as well
else
{
if (!_dustlib) throw FATALERROR("There should be a dust library when dust emission is turned on");
}
// verify that the wavelength range includes the V-band center 0.55 micron (needed for normalization of dust)
WavelengthGrid* lambdagrid = find<WavelengthGrid>();
if (lambdagrid->nearest(0.55e-6) < 0)
throw FATALERROR("Wavelength range should include 0.55 micron for a panchromatic simulation with dust");
// cache size of wavelength grid
_Nlambda = lambdagrid->Nlambda();
}
Array GreyBodyDustEmissivity::emissivity(const DustMix* mix, const Array& Jv) const
{
// get basic information about the wavelength grid
WavelengthGrid* lambdagrid = find<WavelengthGrid>();
int Nlambda = lambdagrid->Nlambda();
// get basic information about the dust mix
int Npop = mix->Npop();
// accumulate the emissivities at the equilibrium temperature for all populations in the dust mix
Array ev(Nlambda);
for (int c=0; c<Npop; c++)
{
double T = mix->equilibrium(Jv,c);
PlanckFunction B(T);
for (int ell=0; ell<Nlambda; ell++)
{
ev[ell] += mix->sigmaabs(ell,c) * B(lambdagrid->lambda(ell));
}
}
// convert emissivity from "per hydrogen atom" to "per unit mass"
ev /= mix->mu();
return ev;
}
Array PanDustSystem::meanintensityv(int m) const
{
WavelengthGrid* lambdagrid = find<WavelengthGrid>();
Array Jv(lambdagrid->Nlambda());
double fac = 4.0*M_PI*volume(m);
for (int ell=0; ell<lambdagrid->Nlambda(); ell++)
{
double kappaabsrho = 0.0;
for (int h=0; h<_Ncomp; h++)
{
double kappaabs = mix(h)->kappaabs(ell);
double rho = density(m,h);
kappaabsrho += kappaabs*rho;
}
double J = Labs(m,ell) / (kappaabsrho*fac) / lambdagrid->dlambda(ell);
// guard against (rare) situations where both Labs and kappa*fac are zero
Jv[ell] = std::isfinite(J) ? J : 0.0;
}
return Jv;
}
void SED::write(const QString& filename) const
{
WavelengthGrid* lambdagrid = find<WavelengthGrid>();
Units* units = find<Units>();
ofstream file(filename.toLocal8Bit().constData());
file << setprecision(8) << scientific;
for (int ell=0; ell<lambdagrid->Nlambda(); ell++)
{
double lambda = lambdagrid->lambda(ell);
double dlambda = lambdagrid->dlambda(ell);
file << units->owavelength(lambda)
<< '\t'
<< _Lv[ell]/dlambda*lambda
<< endl;
}
file.close();
}
void QuasarSED::setupSelfBefore()
{
StellarSED::setupSelfBefore();
WavelengthGrid* lambdagrid = find<WavelengthGrid>();
double Nlambda = lambdagrid->Nlambda();
Array jv(Nlambda);
for (int ell=0; ell<Nlambda; ell++)
{
double lambda = lambdagrid->lambda(ell);
lambda *= 1e6; // conversion from m to micron (the Quasar SED is defined using microns)
double j = 0.0;
double a = 1.0;
double b = 0.003981072;
double c = 0.001258926;
double d = 0.070376103;
if (lambda<0.001)
j = 0.0;
else if (lambda<0.01)
j = a*pow(lambda,0.2);
else if (lambda<0.1)
j = b*pow(lambda,-1.0);
else if (lambda<5.0)
j = c*pow(lambda,-1.5);
else if (lambda<1000.0)
j = d*pow(lambda,-4.0);
else
j = 0.0;
jv[ell] = j;
}
setemissivities(jv);
}
void SingleFrameInstrument::calibrateAndWriteDataCubes(QList< Array*> farrays, QStringList fnames)
{
WavelengthGrid* lambdagrid = find<WavelengthGrid>();
int Nlambda = lambdagrid->Nlambda();
// calibration step 1: conversion from bolometric luminosities (units W) to monochromatic luminosities (units W/m)
for (int ell=0; ell<Nlambda; ell++)
{
double dlambda = lambdagrid->dlambda(ell);
for (int i=0; i<_Nxp; i++)
{
for (int j=0; j<_Nyp; j++)
{
int m = i + _Nxp*j + _Nxp*_Nyp*ell;
foreach (Array* farr, farrays)
{
(*farr)[m] /= dlambda;
}
}
}
}
// calibration step 2: correction for the area of the pixels of the images; the units are now W/m/sr
double xpresang = 2.0*atan(_xpres/(2.0*_distance));
double ypresang = 2.0*atan(_ypres/(2.0*_distance));
double area = xpresang*ypresang;
foreach (Array* farr, farrays)
{
(*farr) /= area;
}
// calibration step 3: conversion of the flux per pixel from monochromatic luminosity units (W/m/sr)
// to flux density units (W/m3/sr) by taking into account the distance
double fourpid2 = 4.0*M_PI*_distance*_distance;
foreach (Array* farr, farrays)
{
(*farr) /= fourpid2;
}
// conversion from program SI units (at this moment W/m3/sr) to the correct output units;
// we use lambda*flambda for the surface brightness (in units like W/m2/arcsec2)
Units* units = find<Units>();
for (int ell=0; ell<Nlambda; ell++)
{
double lambda = lambdagrid->lambda(ell);
for (int i=0; i<_Nxp; i++)
{
for (int j=0; j<_Nyp; j++)
{
int m = i + _Nxp*j + _Nxp*_Nyp*ell;
foreach (Array* farr, farrays)
{
(*farr)[m] = units->obolsurfacebrightness(lambda*(*farr)[m]);
}
}
}
}
