Class for sources described by an array of pixels. More...

#include <source.h>

Inheritance diagram for SourcePixelled:

Collaboration diagram for SourcePixelled:

Public Member Functions
	SourcePixelled (PosType my_z, PosType center, int Npixels, PosType resolution, PosType arr_val, PosType zero_point)

	SourcePixelled (const PixelMap &gal_map, PosType z, PosType factor, PosType zero_point)
	Creates a SourcePixelled from a PixelMap image. The idea is to use stamps of observed galaxies as input sources for simuations. Surface brightness of the source is conserved, taking into account the input pixel size. Factor allows for rescaling of the flux, in case one wants to simulate a different observation. More...

PosType	SurfaceBrightness (const PosType *y) const

void	printSource ()

PosType	getTotalFlux () const

PosType	getRadius () const

PosType *	getEll ()

PosType	getQuad (int i, int j)

PosType	getSize ()

PosType *	getCentroid ()

PosType	getMag ()

Public Member Functions inherited from Source
	Source (PosType r, Point_2d x, PosType z, PosType SBlimit, PosType zero_point)
	shell constructor

	Source (const Source &s)

Source &	operator= (const Source &s)

double	SBlimit_magarcsec (double limit)
	convert mag/arcsec^2 to flux units

PosType	getSBlimit ()
	Gets sb_limit in erg/cm^2/sec/rad^2/Hz.

PosType	getSBlimit_magarcsec ()
	Gets sb_limit in mag/arcsec^2.

PosType	getZ () const
	Redshift of source.

void	setZ (PosType my_z)

PosType	getRadius () const
	Radius of source in radians.

void	setRadius (PosType my_radius)
	Reset the radius of the source in radians.

Point_2d	getTheta () const
	position of source in radians

void	getTheta (PosType *x) const
	position of source in radians

void	getTheta (Point_2d &x) const
	position of source in radians

void	setTheta (PosType *xx)
	Reset the position of the source in radians.

void	setTheta (PosType my_x, PosType my_y)

void	setTheta (const Point_2d &p)

void	setSBlimit (float limit)
	Sets sb_limit in erg/cm^2/sec/rad^2/Hz.

void	setMagZeroPoint (float zeropoint)

double	getMagZeroPoint ()

PosType	changeFilter (std::string filter_in, std::string filter_out, std::string sed)
	Calculates the difference in magnitude when changing the observing filter. More...

PosType	integrateFilter (std::vector< PosType > wavel_fil, std::vector< PosType > fil)
	Calculates the integral of the filter curve given as an array of (x,y) values. More...

PosType	integrateFilterSED (std::vector< PosType > wavel_fil, std::vector< PosType > fil, std::vector< PosType > wavel_sed, std::vector< PosType > sed)
	Calculates the integral of the sed multiplied by the filter curve. More...

double	TEST_surface_brightness (double res, int N)
	test if flux in pixels matches total flux

long	getID () const

void	setID (long i)

Additional Inherited Members
Static Public Member Functions inherited from Source
static PosType *	getx (Source &source)

Protected Member Functions inherited from Source
double	flux_to_mag (double flux) const

Protected Attributes inherited from Source
PosType	source_r
	charactoristic source size

Point_2d	source_x
	center of source

PosType	zsource
	redshift of source

PosType	sb_limit

long	id

double	mag_zero_point

Detailed Description

Class for sources described by an array of pixels.

The sources are created as a square array of pixels of dimension Npixels x Npixels and pixel size equal to resolution.

Constructor & Destructor Documentation

◆ SourcePixelled() [1/2]

SourcePixelled::SourcePixelled	(	PosType	my_z,
		PosType *	my_center,
		int	my_Npixels,
		PosType	my_resolution,
		PosType *	arr_val,
		PosType	zero_point
	)

Parameters

my_z	redshift of the source
my_center	center (in rad)
my_Npixels	number of pixels per side
my_resolution	resolution (in rad)
arr_val	array of pixel values (must be of size = Npixels*Npixels)
zero_point	magnitude zero point

◆ SourcePixelled() [2/2]

SourcePixelled::SourcePixelled	(	const PixelMap &	gal_map,
		PosType	my_z,
		PosType	factor,
		PosType	zero_point
	)

Creates a SourcePixelled from a PixelMap image. The idea is to use stamps of observed galaxies as input sources for simuations. Surface brightness of the source is conserved, taking into account the input pixel size. Factor allows for rescaling of the flux, in case one wants to simulate a different observation.

Parameters

gal_map	Input image and information
my_z	redshift of the source
factor	optional rescaling factor for the flux

Member Function Documentation

◆ SurfaceBrightness()

PosType SourcePixelled::SurfaceBrightness ( const PosType * y ) const

virtual

Surface brightness of source in grid coordinates not source centered coordinates.

The units shuld be ergs / s / Hz / cm^2

Implements Source.

The documentation for this class was generated from the following files:

SLsimLib/include/source.h
SLsimLib/AnalyticNSIE/source.cpp