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Gravitational Lensing Code Library
Public Member Functions | Protected Member Functions | Protected Attributes | List of all members
LensHaloUniform Class Reference

A uniform surface density and shear lens. More...

#include <uniform_lens.h>

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Public Member Functions

 LensHaloUniform (double zlens, double Sigma, Point_2d &Shear, COSMOLOGY &cosmo)
 Direct constructor without any stars. More...
 
float getSigma () const
 surface density in Msun/Mpc^2
 
Point_2d getShear () const
 shear in Msun/Mpc^2
 
void resetGamma (const Point_2d &Shear)
 reset the shear keeping the redshift of the plane fixed More...
 
void resetKappa (double Sigma)
 reset the convergence keeping the redshift of the plane fixed More...
 
void force_halo (PosType *alpha, KappaType *kappa, KappaType *gamma, KappaType *phi, PosType const *xcm, bool subtract_point=false, PosType screening=1.0)
 
 LensHaloUniform (const LensHaloUniform &h)
 
LensHaloUniformoperator= (const LensHaloUniform &h)
 
- Public Member Functions inherited from LensHalo
 LensHalo ()
 Shell constructor.
 
 LensHalo (PosType z, const COSMOLOGY &cosmo)
 
 LensHalo (const LensHalo &h)
 
 LensHalo (LensHalo &&h)
 
LensHalooperator= (const LensHalo &h)
 
LensHalooperator= (LensHalo &&h)
 
float get_Rmax () const
 this can be used to tag types of LensHalos More...
 
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 More...
 
bool compareZ (PosType z)
 force tree calculation for stars More...
 
EllipMethod getEllipMethod () const
 stars More...
 
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. More...
 
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 More...
 
size_t getID () const
 
void setID (size_t id)
 
PosType renormalization (PosType r_max)
 
PixelMap 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. More...
 

Protected Member Functions

PosType lens_expand (PosType *mod, PosType const *x, PosType *alpha, KappaType *gamma, KappaType *phi)
 first two are shear
 
- 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 More...
 
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. More...
 
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. More...
 
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)) More...
 
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. More...
 
virtual void alphakappagamma1asym (PosType x, PosType theta, PosType alpha[2], PosType *kappa, PosType gamma[], PosType *phi)
 Elliptical profiles by Fourier-Ansatz. More...
 
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])
 

Protected Attributes

PosType perturb_modes [3]
 
- 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
 

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
 
- Public Attributes inherited from LensHalo
int tag =0
 
- Static Protected Attributes inherited from LensHalo
static const int Nmod = 32
 

Detailed Description

A uniform surface density and shear lens.

Note the units of the input shear and surface density are not Sigma_crit's. This lens will extend to infinity in the angular directions.

If the magnitude g and position angle, theta, are specified then

Shear[0] = g * cos( 2*theta ) Shear[1] = g * sin( 2*theta )

Constructor & Destructor Documentation

◆ LensHaloUniform()

LensHaloUniform::LensHaloUniform ( double  zlens,
double  Sigma,
Point_2d Shear,
COSMOLOGY &  cosmo 
)

Direct constructor without any stars.

Parameters
zlenslens redshift
Sigmasurface density of lens in Msun/Mpc^2
Shearshear in M_sun/Mpc^2 ie gamma * Sigma_crit

Member Function Documentation

◆ force_halo()

void LensHaloUniform::force_halo ( PosType *  alpha,
KappaType *  kappa,
KappaType *  gamma,
KappaType *  phi,
PosType const *  xcm,
bool  subtract_point = false,
PosType  screening = 1.0 
)
virtual
Parameters
alphamass/Mpc
subtract_pointif true contribution from a point mass is subtracted

Reimplemented from LensHalo.

◆ resetGamma()

void LensHaloUniform::resetGamma ( const Point_2d Shear)
inline

reset the shear keeping the redshift of the plane fixed

Parameters
ShearShear in units of critical density Msun/Mpc^2, ie gamma * Sigma_crit

◆ resetKappa()

void LensHaloUniform::resetKappa ( double  Sigma)
inline

reset the convergence keeping the redshift of the plane fixed

Parameters
SigmaSurface density in Msun/Mpc^2, ie kappa * Sigma_crit

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