A class that includes the MOKA lens map. More...

#include <MOKAlens.h>

Inheritance diagram for LensHaloMassMap:

Collaboration diagram for LensHaloMassMap:

Public Member Functions
	LensHaloMassMap (const std::string &filename, PixelMapType maptype, int pixel_map_zeropad, bool my_zeromean, const COSMOLOGY &lenscosmo)
	loads a mass map from a given filename

	LensHaloMassMap (const PixelMap< double > &MassMap, double massconvertion, double redshift, int pixel_map_zeropad, bool my_zeromean, const COSMOLOGY &lenscosmo)
	Create a LensHalo from a PixelMap representing the mass.

	LensHaloMassMap (const PixelMap< float > &MassMap, double massconvertion, double redshift, int pixel_map_zeropad, bool my_zeromean, const COSMOLOGY &lenscosmo)

	LensHaloMassMap (double mass, Point_2d center, Point_2d range, double resolution, int zeropadding, double redshift, const COSMOLOGY &cosmo)
	This makes a uniform rectangular mass sheat.

	LensHaloMassMap (const LensHaloMassMap &h)

	LensHaloMassMap (LensHaloMassMap &&h)

LensHaloMassMap &	operator= (LensHaloMassMap &h)

LensHaloMassMap &	operator= (LensHaloMassMap &&h)

void	assignParams (InputParams &params)

void	checkCosmology ()
	checks the cosmology against the MOKA map parameters

void	force_halo (double alpha, KappaType kappa, KappaType gamma, KappaType phi, double const *xcm, bool subtract_point=false, PosType screening=1.0)
	Routine for obtaining the deflection and other lensing quantities for a LensHaloMassMap for just one ray!!

void	getDims ()

void	readMap ()
	reads in the fits file for the MOKA or mass map and saves it in the structure map

template<typename T>
void	setMap (const PixelMap< T > &inputmap, double convertionfactor, double z)

void	writeImage (std::string fn)
	write the fits file of the new MOKA map from the structure map

Point_2d	getCenter () const
	return center in physical Mpc

double	getRangeRad () const
	return range of input map in rad

double	getRangeMpc () const
	return range of input map in physical Mpc

size_t	getN () const
	/// return number of pixels on a side in original map

size_t	getNx () const
	return number of pixels on a x-axis side in original map

size_t	getNy () const
	return number of pixels on a y-axis side in original map

Public Member Functions inherited from LensHalo
	LensHalo ()
	Shell constructor.

	LensHalo (PosType z, const COSMOLOGY &cosmo)

	LensHalo (const LensHalo &h)

	LensHalo (LensHalo &&h)

LensHalo &	operator= (const LensHalo &h)

LensHalo &	operator= (LensHalo &&h)

float	get_Rmax () const
	this can be used to tag types of LensHalos

float	getRsize () const
	get the Rsize which is the size of the halo in Mpc

float	get_mass () const
	get the mass solar units

float	get_rscale () const
	get the scale radius in Mpc

PosType	getZlens () const
	get the redshift

void	getX (PosType *MyPosHalo) const
	get the position of the Halo in physical Mpc on the lens plane

PosType	operator[] (int i) const
	returns position of the Halo in physical Mpc on the lens plane

void	setTheta (PosType PosX, PosType PosY)
	set the position of the Halo in radians

void	setTheta (PosType *PosXY)
	set the position of the Halo in radians

void	setTheta (const Point_2d &p)
	set the position of the Halo in radians

void	getTheta (PosType *MyPosHalo) const
	get the position of the Halo in radians

void	setDist (COSMOLOGY &co)
	Set the angular size distance to the halo. This should be the distance to the lens plane.

PosType	getDist () const

void	displayPos ()

virtual void	initFromFile (float my_mass, long *seed, float vmax, float r_halfmass)
	initialize from a simulation file

virtual void	initFromMassFunc (float my_mass, float my_Rsize, float my_rscale, PosType my_slope, long *seed)
	initialize from a mass function

virtual void	set_RsizeRmax (float my_Rsize)
	set Rsize (in Mpc) and reset Rmax

void	set_mass (float my_mass)
	set mass (in solar masses)

virtual void	set_rscale (float my_rscale)
	set scale radius (in Mpc)

void	setZlens (PosType my_zlens, const COSMOLOGY &cosmo)
	set redshift

void	setRsize (PosType R)

void	setZlensDist (PosType my_zlens, const COSMOLOGY &cos)

void	setMass (PosType m)

virtual void	set_slope (PosType my_slope)
	set slope

virtual PosType	get_slope ()
	get slope

bool	get_flag_elliptical ()
	flag=True if halo elliptical

void	set_flag_elliptical (bool ell)

bool	get_switch_flag ()

void	set_switch_flag (bool swt)
	flag permits case distinction in force_halo_asym for elliptical NFWs only (get_switch_flag==true), in latter case the mass_norm_factor^2 is used instead of mass_norm_factor.

virtual void	setCosmology (const COSMOLOGY &cosmo)
	used for elliptical NFWs only, in that case get_switch_flag==true

bool	compareZ (PosType z)
	force tree calculation for stars

EllipMethod	getEllipMethod () const
	stars

std::vector< double >	get_mod ()
	get vector of Fourier modes, which are calculated in the constructors of the LensHaloes when main_ellip_method is set to 'Fourier'

virtual std::size_t	Nparams () const
	get the number of halo parameters

virtual PosType	getParam (std::size_t p) const
	get the value of a scaled halo parameter by index

virtual PosType	setParam (std::size_t p, PosType value)
	set the value of a scaled halo parameter by index

virtual void	printCSV (std::ostream &, bool header=false) const
	print the halo parameters in CSV format

PosType	MassBy2DIntegation (PosType R)
	Prints star parameters; if show_stars is true, prints data for single stars.

PosType	MassBy1DIntegation (PosType R)
	calculates the mass within radius R by integating alpha on a ring and using Gauss' law, used only for testing

PosType	test_average_gt (PosType R)
	calculates the average gamma_t for LensHalo::test()

PosType	test_average_kappa (PosType R)

void	set_norm_factor ()

void	set_rsize (float my_rsize)
	set radius rsize beyond which interpolation values between alpha_ellip and alpha_iso are computed

float	get_rsize ()

bool	test ()
	perform some basic consistancy checks for halo

size_t	getID () const

void	setID (size_t id)

PosType	renormalization (PosType r_max)

PixelMap< double >	map_variables (LensingVariable lensvar, size_t Nx, size_t Ny, double res)
	Map a PixelMap of the surface, density, potential and potential gradient centred on (0,0) in LensHalo coordinates.

Public Attributes
std::string	MOKA_input_file

int	flag_MOKA_analyze
	if >=1 (true), do analyzis only; if = 0 (false) change units to internal GLAMER units and prepare for ray-shooting

int	flag_background_field

Public Attributes inherited from LensHalo
int	tag =0

Protected Member Functions
	LensHaloMassMap (COSMOLOGY &c)

Protected Member Functions inherited from LensHalo
PosType	alpha_int (PosType x) const
	Calculates potential (phi_int) from alpha_h. If flag is_alphah_a_table is True it takes and integrates directly the gfunction instead of alpha_h. The gfunction is used for the InterpolationTable used in alpha_h. Setting the flag to False speeds up the calculation of phi_h.

PosType	norm_int (PosType r_max)

void	force_halo_sym (PosType alpha, KappaType kappa, KappaType gamma, KappaType phi, PosType const *xcm, bool subtract_point=false, PosType screening=1.0)
	returns the lensing quantities of a ray in center of mass coordinates for a symmetric halo

void	force_halo_asym (PosType alpha, KappaType kappa, KappaType gamma, KappaType phi, PosType const *xcm, bool subtract_point=false, PosType screening=1.0)

bool	force_point (PosType alpha, KappaType kappa, KappaType gamma, KappaType phi, PosType const *xcm, PosType rcm2, bool subtract_point, PosType screening)

void	assignParams (InputParams &params, bool needRsize)
	read in parameters from a parameterfile in InputParams params

void	error_message1 (std::string name, std::string filename)
	read in star parameters. This is valid for all halos and not overloaded.

virtual PosType	alpha_h (PosType x) const

virtual KappaType	kappa_h (PosType x) const

virtual KappaType	gamma_h (PosType x) const

virtual KappaType	phi_h (PosType x) const

virtual KappaType	phi_int (PosType x) const

virtual PosType	ffunction (PosType x) const

virtual PosType	gfunction (PosType x) const

virtual PosType	dgfunctiondx (PosType x)

virtual PosType	bfunction (PosType x)

virtual PosType	dhfunction (PosType x) const

virtual PosType	ddhfunction (PosType x, bool numerical)

virtual PosType	dddhfunction (PosType x, bool numerical)

virtual PosType	bnumfunction (PosType x)

virtual PosType	dbfunction (PosType x)

virtual PosType	ddbfunction (PosType x)

virtual PosType	dmoddb (int whichmod, PosType q, PosType b)

virtual PosType	ddmoddb (int whichmod, PosType q, PosType b)

virtual PosType	dmoddq (int whichmod, PosType q, PosType b)

virtual PosType	ddmoddq (int whichmod, PosType q, PosType b)

void	faxial (PosType x, PosType theta, PosType f[])
	If set to true the correct normalization is applied for asymmetric NFW profiles, the mass_norm_factor is different for the other halos.

void	faxial0 (PosType theta, PosType f0[])

void	faxial1 (PosType theta, PosType f1[])

void	faxial2 (PosType theta, PosType f2[])

void	gradial (PosType r, PosType g[])
	Derivatives of the potential damping factor with respect to r ... TODO: come up with a better damping faction.

void	gradial2 (PosType r, PosType mu, PosType sigma, PosType g[])

void	felliptical (PosType x, PosType q, PosType theta, PosType f[], PosType g[])
	Calculate the derivatives of the G function = r*sqrt(cos(theta)^2 + q(r)^2 sin(theta))

virtual void	gamma_asym (PosType x, PosType theta, PosType gamma[])

virtual PosType	kappa_asym (PosType x, PosType theta)

virtual void	alphakappagamma_asym (PosType x, PosType theta, PosType alpha[], PosType kappa, PosType gamma[], PosType phi)
	Pseudo-elliptical profiles by Phi(G)-Ansatz.

virtual void	alphakappagamma1asym (PosType x, PosType theta, PosType alpha[2], PosType kappa, PosType gamma[], PosType phi)
	Elliptical profiles by Fourier-Ansatz.

virtual void	alphakappagamma2asym (PosType x, PosType theta, PosType alpha[2], PosType kappa, PosType gamma[], PosType phi)

virtual void	alphakappagamma3asym (PosType x, PosType theta, PosType alpha[2], PosType kappa, PosType gamma[], PosType phi)

virtual PosType	alpha_ell (PosType x, PosType theta)

double	fourier_coeff (double n, double q, double beta)
	Calculates fourier-coefficients for power law halo.

double	IDAXDM (double lambda, double a2, double b2, double x[], double rmax, double mo)

double	IDAYDM (double lambda, double a2, double b2, double x[], double rmax, double mo)

double	SCHRAMMKN (double n, double x[], double rmax)

double	SCHRAMMJN (double n, double x[], double rmax)

double	SCHRAMMI (double x[], double rmax)

void	calcModes (double q, double beta, double rottheta, PosType newmod[])
	Calculates the modes for fourier expansion of power law halo. All the modes are relative to the zero mode to conserve mass throughout the calculation of kappa etc.

void	calcModesB (PosType x, double q, double beta, double rottheta, PosType newmod[])

void	calcModesC (PosType beta_r, double q, double rottheta, PosType newmod[])

virtual PosType	InterpolateModes (int whichmod, PosType q, PosType b)

void	analModes (int modnumber, PosType my_beta, PosType q, PosType amod[3])

Additional Inherited Members
Static Public Member Functions inherited from LensHalo
static const int	get_Nmod ()
	get length of mod array, which is Nmod. Not to be confused with getNmodes in the class LensHaloFit

Protected Attributes inherited from LensHalo
float	Rsize = 0

float	mass

PosType	Dist

PosType	mnorm

float	Rmax

PosType	beta

float	Rmax_to_Rsize_ratio = 1.2
	The factor by which Rmax is larger than Rsize.

float	rscale
	scale length or core size. Different meaning in different cases. Not used in NSIE case.

EllipMethod	main_ellip_method

PosType	xmax

PosType	mass_norm_factor =1
	This is Rsize/rscale !!

float	pa

float	fratio =1.0

bool	elliptical_flag = false

bool	switch_flag = false

PosType	mod [Nmod]

PosType	mod1 [Nmod]

PosType	mod2 [Nmod]

PosType	r_eps

Static Protected Attributes inherited from LensHalo
static const int	Nmod = 32

Detailed Description

A class that includes the MOKA lens map.

The class represents a pixelixed mass map as a lens. The mass map can come from the output of a nbody/hydro simulation or from anywhere else.

An alternative way of using the output of a particle-based simulation is to use a LensHaloParticles.

Note: To use this class requires setting the ENABLE_FITS compiler flag and linking the cfits library.

Constructor & Destructor Documentation

◆ LensHaloMassMap() [1/3]

LensHaloMassMap::LensHaloMassMap	(	const PixelMap< double > &	MassMap,
		double	massconvertion,
		double	redshift,
		int	pixel_map_zeropad,
		bool	my_zeromean,
		const COSMOLOGY &	lenscosmo )

Create a LensHalo from a PixelMap representing the mass.

This is especially useful for representing the visible stars from an image in the lens model.

constructor for making lens halo directly from a mass map

The pixel map should be defined with physical Mpc dimensions.

Parameters

MassMap	mass map, resolution/range in radians, PixelMapUnits setting is ignored
massconvertion	convertion factor from pixel units to solar masses
redshift	redshift of lens
pixel_map_zeropad	factor by which to zero pad in FFTs, ex. 4
my_zeromean	if true, subtracts average density
lenscosmo	cosmology

◆ LensHaloMassMap() [2/3]

LensHaloMassMap::LensHaloMassMap	(	const PixelMap< float > &	MassMap,
		double	massconvertion,
		double	redshift,
		int	pixel_map_zeropad,
		bool	my_zeromean,
		const COSMOLOGY &	lenscosmo )

Parameters

MassMap	mass map, resolution/range in radians, PixelMapUnits setting is ignored
massconvertion	convertion factor from pixel units to solar masses
redshift	redshift of lens
pixel_map_zeropad	factor by which to zero pad in FFTs, ex. 4
my_zeromean	if true, subtracts average density
lenscosmo	cosmology

◆ LensHaloMassMap() [3/3]

LensHaloMassMap::LensHaloMassMap	(	double	mass,
		Point_2d	center,
		Point_2d	range,
		double	resolution,
		int	zeropadding,
		double	redshift,
		const COSMOLOGY &	cosmo )

This makes a uniform rectangular mass sheat.

Parameters

mass	total mass in rectangle
center	center of rectangle
range	width and hight in radians
resolution	resolution in radians
zeropadding	factor by which to zero pad in FFTs, ex. 1 is no padding, 2 FFT grid is twice as big as original map
redshift	redshift of plane

Member Function Documentation

◆ assignParams()

void LensHaloMassMap::assignParams ( InputParams & params )

Sets many parameters within the MOKA lens model

not really used

◆ checkCosmology()

void LensHaloMassMap::checkCosmology ( )

checks the cosmology against the MOKA map parameters

checks that cosmology in the header of the input fits map is the same as the one set

◆ force_halo()

void LensHaloMassMap::force_halo	(	double *	alpha,
		KappaType *	kappa,
		KappaType *	gamma,
		KappaType *	phi,
		double const *	xx,
		bool	subtract_point = false,
		PosType	screening = 1.0 )

virtual

Routine for obtaining the deflection and other lensing quantities for a LensHaloMassMap for just one ray!!

Parameters

xx	position in physical Mpc

Reimplemented from LensHalo.

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

SLsimLib/include/MOKAlens.h
SLsimLib/MultiPlane/MOKAfits.cpp
SLsimLib/MultiPlane/MOKAlens.cpp

Public Member Functions

Public Attributes

Protected Member Functions

Additional Inherited Members

Detailed Description

Constructor & Destructor Documentation

◆ LensHaloMassMap() [1/3]

◆ LensHaloMassMap() [2/3]

◆ LensHaloMassMap() [3/3]

Member Function Documentation

◆ assignParams()

◆ checkCosmology()

◆ force_halo()