35 #ifndef __MODELLINGTWOPOINT1D__
36 #define __MODELLINGTWOPOINT1D__
69 std::shared_ptr<modelling::twopt::STR_data_HOD>
m_data_HOD;
225 void set_data_model (
const cbl::cosmology::Cosmology cosmology,
const double redshift,
const std::string method_Pk=
"CAMB",
const double sigmaNL_perp=0.,
const double sigmaNL_par=0.,
const bool NL=
true,
const double bias=1.,
const double pimax=40.,
const double r_min=1.,
const double r_max=350.,
const double k_min=1.e-4,
const double k_max=100.,
const int step=500,
const std::string output_dir=
par::defaultString,
const std::string output_root=
"test",
const int norm=-1,
const double aa=0.,
const bool GSL=
true,
const double prec=1.e-3,
const std::string file_par=
par::defaultString,
const double Delta=200.,
const bool isDelta_critical=
true,
const std::vector<double> cluster_redshift={},
const std::vector<double> cluster_mass_proxy={},
const std::vector<double> cluster_mass_proxy_error={},
const std::string model_bias=
"Tinker",
const std::string meanType=
"mean_bias",
const int seed=666,
const cbl::cosmology::Cosmology cosmology_mass={},
const std::vector<double> redshift_source={});
311 void set_data_model (
const cbl::cosmology::Cosmology cosmology,
const double redshift,
const std::vector<double> cluster_redshift,
const std::vector<double> cluster_mass_proxy,
const double redshift_pivot,
const double proxy_pivot,
double mass_pivot,
const double log_base,
const std::string method_Pk=
"CAMB",
const bool NL=
true,
const double r_min=1.,
const double r_max=350.,
const double k_min=1.e-4,
const double k_max=100.,
const int step=500,
const std::string output_dir=
par::defaultString,
const std::string output_root=
"test",
const int norm=-1,
const double prec=1.e-3,
const std::string file_par=
par::defaultString,
const double Delta=200.,
const bool isDelta_critical=
true,
const std::string model_bias=
"Tinker");
407 void set_data_model (
const double z_abs_err,
const double proxy_rel_err,
const cbl::cosmology::Cosmology cosmology,
const double redshift,
const std::vector<double> cluster_redshift,
const std::vector<double> cluster_mass_proxy,
const double redshift_pivot,
const double proxy_pivot,
double mass_pivot,
const double log_base,
const std::string method_Pk=
"CAMB",
const bool NL=
true,
const double r_min=1.,
const double r_max=350.,
const double k_min=1.e-4,
const double k_max=100.,
const int step=500,
const std::string output_dir=
par::defaultString,
const std::string output_root=
"test",
const int norm=-1,
const double prec=1.e-3,
const std::string file_par=
par::defaultString,
const double Delta=200.,
const bool isDelta_critical=
true,
const std::string model_bias=
"Tinker");
526 void set_data_HOD (
const cbl::cosmology::Cosmology cosmology={},
const double redshift=0.,
const std::string model_MF=
"Tinker",
const std::string model_bias=
"Tinker",
const double Mh_min=0.,
const double Mh_max=1.e16,
const double pi_max=100.,
const double r_max_int=100.,
const double r_min=1.e-3,
const double r_max=350.,
const double k_min=1.e-4,
const double k_max=100.,
const int step=200,
const double m_min=1.e7,
const double m_max=1.e17,
const int m_step=100,
const std::string method_Pk=
"CAMB",
const bool NL=
true,
const std::string output_root=
"test",
const double Delta=200.,
const double kk=0.,
const std::string interpType=
"Linear",
const int norm=-1,
const double prec=1.e-2,
const std::string input_file=
par::defaultString,
const bool is_parameter_file=
true,
const std::string model_cM=
"Duffy",
const std::string profile=
"NFW",
const std::string halo_def=
"vir");
606 void set_data_model_cluster_selection_function (
const cbl::cosmology::Cosmology cosmology,
const cbl::cosmology::Cosmology test_cosmology,
const double mean_redshift,
const std::string model_MF,
const std::string model_bias,
const std::string selection_function_file,
const std::vector<int> selection_function_column={},
const double z_min=
par::defaultDouble,
const double z_max=
par::defaultDouble,
const double Mass_min=
par::defaultDouble,
const double Mass_max=
par::defaultDouble,
const std::string file_par=
par::defaultString,
const double Delta=200,
const bool isDelta_critical=
false,
const std::string method_Pk=
"CAMB",
const std::string output_dir=
par::defaultString,
const double k_min=1.e-4,
const double k_max=100,
const double prec=1.e-2,
const int step=200,
const int mass_step=50);
Global functions to model 1D two-point correlation functions of any type.
The class Modelling_TwoPointCorrelation.
The class Modelling_TwoPointCorrelation1D.
void set_data_model(const cbl::cosmology::Cosmology cosmology, const double redshift, const std::string method_Pk="CAMB", const double sigmaNL_perp=0., const double sigmaNL_par=0., const bool NL=true, const double bias=1., const double pimax=40., const double r_min=1., const double r_max=350., const double k_min=1.e-4, const double k_max=100., const int step=500, const std::string output_dir=par::defaultString, const std::string output_root="test", const int norm=-1, const double aa=0., const bool GSL=true, const double prec=1.e-3, const std::string file_par=par::defaultString, const double Delta=200., const bool isDelta_critical=true, const std::vector< double > cluster_redshift={}, const std::vector< double > cluster_mass_proxy={}, const std::vector< double > cluster_mass_proxy_error={}, const std::string model_bias="Tinker", const std::string meanType="mean_bias", const int seed=666, const cbl::cosmology::Cosmology cosmology_mass={}, const std::vector< double > redshift_source={})
set the data used to construct generic models of the two-point correlation function
void set_data_HOD(const cbl::cosmology::Cosmology cosmology={}, const double redshift=0., const std::string model_MF="Tinker", const std::string model_bias="Tinker", const double Mh_min=0., const double Mh_max=1.e16, const double pi_max=100., const double r_max_int=100., const double r_min=1.e-3, const double r_max=350., const double k_min=1.e-4, const double k_max=100., const int step=200, const double m_min=1.e7, const double m_max=1.e17, const int m_step=100, const std::string method_Pk="CAMB", const bool NL=true, const std::string output_root="test", const double Delta=200., const double kk=0., const std::string interpType="Linear", const int norm=-1, const double prec=1.e-2, const std::string input_file=par::defaultString, const bool is_parameter_file=true, const std::string model_cM="Duffy", const std::string profile="NFW", const std::string halo_def="vir")
set the data used to construct the HOD model
void set_data_model_cluster_selection_function(const cbl::cosmology::Cosmology cosmology, const cbl::cosmology::Cosmology test_cosmology, const double mean_redshift, const std::string model_MF, const std::string model_bias, const std::string selection_function_file, const std::vector< int > selection_function_column={}, const double z_min=par::defaultDouble, const double z_max=par::defaultDouble, const double Mass_min=par::defaultDouble, const double Mass_max=par::defaultDouble, const std::string file_par=par::defaultString, const double Delta=200, const bool isDelta_critical=false, const std::string method_Pk="CAMB", const std::string output_dir=par::defaultString, const double k_min=1.e-4, const double k_max=100, const double prec=1.e-2, const int step=200, const int mass_step=50)
set the data used to construct the model for clustering analyses using the selection function
Modelling_TwoPointCorrelation1D()=default
default constuctor
std::shared_ptr< modelling::twopt::STR_data_HOD > data_HOD()
get the member m_data_HOD
virtual ~Modelling_TwoPointCorrelation1D()=default
default destructor
std::shared_ptr< modelling::twopt::STR_data_HOD > m_data_HOD
the container of parameters for the HOD modelling of the two-point correlation function
The class Modelling_TwoPointCorrelation.
measure::twopt::TwoPType twoPType()
get the member m_twoPType
static const std::string defaultString
default std::string value
static const double defaultDouble
default double value
TwoPType
the two-point correlation function type
double bias(const double Mmin, const double sigmalgM, const double M0, const double M1, const double alpha, const std::shared_ptr< void > inputs)
the mean galaxy bias
The global namespace of the CosmoBolognaLib