160 lines
5.4 KiB
C++
160 lines
5.4 KiB
C++
/*+
|
|
ARES/HADES/BORG Package -- ./libLSS/data/schechter_completeness.hpp
|
|
Copyright (C) 2014-2020 Guilhem Lavaux <guilhem.lavaux@iap.fr>
|
|
Copyright (C) 2009-2020 Jens Jasche <jens.jasche@fysik.su.se>
|
|
|
|
Additional contributions from:
|
|
Guilhem Lavaux <guilhem.lavaux@iap.fr> (2023)
|
|
|
|
+*/
|
|
#ifndef __LIBLSS_SCHECHTER_COMPLETENESS_HPP
|
|
#define __LIBLSS_SCHECHTER_COMPLETENESS_HPP
|
|
|
|
#include <cmath>
|
|
#include <functional>
|
|
#include <boost/format.hpp>
|
|
#include "libLSS/tools/console.hpp"
|
|
#include "libLSS/physics/cosmo.hpp"
|
|
#include "libLSS/tools/gslIntegrate.hpp"
|
|
#include <CosmoTool/hdf5_array.hpp>
|
|
#include "libLSS/data/spectro_gals.hpp"
|
|
#include "libLSS/data/galaxies.hpp"
|
|
#include "libLSS/data/projection.hpp"
|
|
|
|
namespace LibLSS {
|
|
|
|
typedef std::function<bool(const BaseGalaxyDescriptor &)> GalaxySelector;
|
|
|
|
struct GalaxySampleSelection {
|
|
double bright_apparent_magnitude_cut;
|
|
double faint_apparent_magnitude_cut;
|
|
double bright_absolute_magnitude_cut;
|
|
double faint_absolute_magnitude_cut;
|
|
|
|
double zmin, zmax;
|
|
double dmin, dmax;
|
|
|
|
double low_mass_cut;
|
|
double high_mass_cut;
|
|
double small_radius_cut;
|
|
double large_radius_cut;
|
|
double low_spin_cut;
|
|
double high_spin_cut;
|
|
|
|
// This is required to satisfy C++ object layout
|
|
// Otherwise the struct GalaxySampleSelection is not "trivial".
|
|
std::shared_ptr<GalaxySelector> selector;
|
|
ProjectionDataModel projection;
|
|
};
|
|
|
|
static inline std::shared_ptr<GalaxySelector> makeSelector(GalaxySelector f) {
|
|
return std::make_shared<GalaxySelector>(f);
|
|
}
|
|
|
|
struct SchechterParameters {
|
|
double Mstar, alpha;
|
|
};
|
|
|
|
namespace details {
|
|
|
|
static inline double
|
|
_integrand_luminosity(const SchechterParameters ¶ms, double x) {
|
|
return std::pow(x, params.alpha) * exp(-x);
|
|
}
|
|
|
|
static inline double integral_luminosity(
|
|
const SchechterParameters ¶ms, double x_min, double x_max) {
|
|
return gslIntegrate(
|
|
std::bind(_integrand_luminosity, params, std::placeholders::_1),
|
|
x_min, x_max, 1e-8);
|
|
}
|
|
|
|
static inline double computeSchechterCompleteness(
|
|
const Cosmology &cosmo, double z, double d_comoving,
|
|
const GalaxySampleSelection &selection,
|
|
const SchechterParameters ¶ms,
|
|
CorrectionFunction zcorrection = nullCorrection) {
|
|
using boost::format;
|
|
ConsoleContext<LOG_DEBUG> ctx("computeSchechterCompleteness");
|
|
|
|
double d_lum = cosmo.d2dlum(z, d_comoving);
|
|
double corr = zcorrection(z);
|
|
|
|
double absolute_mu0 = selection.faint_apparent_magnitude_cut -
|
|
5 * std::log10(d_lum) - 25 - corr;
|
|
double absolute_ml0 = selection.bright_apparent_magnitude_cut -
|
|
5 * std::log10(d_lum) - 25 - corr;
|
|
|
|
double abmu =
|
|
std::min(absolute_mu0, selection.faint_absolute_magnitude_cut);
|
|
double abml =
|
|
std::max(absolute_ml0, selection.bright_absolute_magnitude_cut);
|
|
|
|
ctx.print(
|
|
format("z = %lg d_lum = %lg abmu = %lg abml = %lg") % z % d_lum %
|
|
abmu % abml);
|
|
|
|
abmu = std::max(abmu, abml);
|
|
|
|
double xl0 = std::pow(10.0, 0.4 * (params.Mstar - abmu));
|
|
double xu0 = std::pow(10.0, 0.4 * (params.Mstar - abml));
|
|
|
|
double xl1 = std::pow(
|
|
10.0, 0.4 * (params.Mstar - selection.faint_absolute_magnitude_cut));
|
|
double xu1 = std::pow(
|
|
10.0, 0.4 * (params.Mstar - selection.bright_absolute_magnitude_cut));
|
|
|
|
ctx.print(
|
|
format("xl0 = %lg, xu0 = %lg, xl1 = %lg, xu1 = %lg") % xl0 % xu0 %
|
|
xl1 % xu1);
|
|
|
|
double Phi0 = integral_luminosity(params, xl0, xu0);
|
|
double Phi1 = integral_luminosity(params, xl1, xu1);
|
|
|
|
return std::max(0.0, Phi0 / Phi1);
|
|
}
|
|
|
|
} // namespace details
|
|
|
|
template <typename Array>
|
|
void buildCompletenessFromSchechterFunction(
|
|
const Cosmology &cosmo, const GalaxySampleSelection &selection,
|
|
const SchechterParameters ¶ms, Array &completeness, double Dmax,
|
|
CorrectionFunction zcorr = details::nullCorrection) {
|
|
|
|
ConsoleContext<LOG_DEBUG> ctx("buildCompletenessFromSchechterFunction");
|
|
long N = completeness.num_elements();
|
|
for (long i = 1; i < N; i++) {
|
|
double d = i * Dmax / N;
|
|
double z = cosmo.a2z(cosmo.com2a(cosmo.comph2com(d)));
|
|
|
|
if (z < selection.zmin || z > selection.zmax)
|
|
completeness[i] = 0;
|
|
else
|
|
completeness[i] = details::computeSchechterCompleteness(
|
|
cosmo, z, d, selection, params, zcorr);
|
|
//ctx.print(boost::format("d = %lg, z = %lg, C = %lg") % d % z % completeness[i]);
|
|
}
|
|
// zero distance is hard, just copy the one next to it. If sampling is sufficient that will not matter.
|
|
completeness[0] = completeness[1];
|
|
}
|
|
|
|
} // namespace LibLSS
|
|
|
|
CTOOL_STRUCT_TYPE(
|
|
LibLSS::GalaxySampleSelection, HDF5T_GalaxySampleSelection,
|
|
((double,
|
|
bright_apparent_magnitude_cut))((double, faint_apparent_magnitude_cut))(
|
|
(double, bright_absolute_magnitude_cut))(
|
|
(double, faint_absolute_magnitude_cut))((double, zmin))((double, zmax))(
|
|
(double, dmin))((double, dmax))((double, low_mass_cut))(
|
|
(double, high_mass_cut))((double, small_radius_cut))(
|
|
(double, large_radius_cut))((double, low_spin_cut))(
|
|
(double, high_spin_cut))((LibLSS::ProjectionDataModel, projection)));
|
|
|
|
CTOOL_STRUCT_TYPE(
|
|
LibLSS::SchechterParameters, HDF5T_SchechterParameters,
|
|
((double, Mstar))((double, alpha)));
|
|
|
|
#endif
|