GLAMERDOC++
Gravitational Lensing Code Library
Public Member Functions | List of all members
LensHaloParticlesM< DType > Class Template Reference

LensHaloParticles but where the "particles" have different masses. More...

#include <particle_halo2.h>

Inheritance diagram for LensHaloParticlesM< DType >:
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Collaboration diagram for LensHaloParticlesM< DType >:
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Public Member Functions

 LensHaloParticlesM (std::vector< Point_3d< DType > > &pvector, PosType redshift, double my_inv_area_phys, std::vector< DType > Masses, const COSMOLOGY &cosmo, int my_Nsmooth=5, float Nbucket=8, float theta=0.1, bool recenter=false, bool verbose=false)
 
 LensHaloParticlesM (LensHaloParticlesM &&h)
 
LensHaloParticlesM & operator= (LensHaloParticlesM &&h)
 
void force_halo (double *alpha, KappaType *kappa, KappaType *gamma, KappaType *phi, double const *xcm, bool subtract_point=false, PosType screening=1)
 does not zero lens quantities
 
void swapoutMasses (std::vector< DType > &Mvector)
 swap out the masses, leaving the LensHaloParticlesM empty
 
- Public Member Functions inherited from LensHaloParticles< float >
 LensHaloParticles (const std::string &simulation_filename, SimFileFormat format, PosType redshift, double my_inv_area_phys, PosType mass_particle, const COSMOLOGY &cosmo, int my_Nsmooth=5, float Nbucket=8, float theta=0.1, bool recenter=false, bool verbose=false)
 
 LensHaloParticles (std::vector< Point_3d< float > > &pvector, PosType redshift, double my_inv_area_phys, PosType mass_particle, const COSMOLOGY &cosmo, int my_Nsmooth=5, float Nbucket=8, float theta=0.1, bool recenter=false, bool verbose=false)
 construct directly from a vector of positions More...
 
 LensHaloParticles (LensHaloParticles &&h)
 
void force_halo (double *alpha, KappaType *kappa, KappaType *gamma, KappaType *phi, double const *xcm, bool subtract_point=false, PosType screening=1)
 does not zero lens quantities
 
size_t getN () const
 
Point_3d< float > CenterOfMass ()
 get current center of mass in input coordinates
 
LensHaloParticles & operator= (LensHaloParticles &&h)
 
void rotate (PosType theta_x, PosType theta_y, Point_3d< float > &xo)
 
void resetForceAngle (double theta)
 
void translate_particles (Point_3d< float > &xo)
 
void getBoundingBox (Point_3d< float > &p1, Point_3d< float > &p2) const
 
void swapout (std::vector< Point_3d< float > > &pvector)
 swap out the particle positions, leaving the LensHaloParticles empty
 
- 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 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
 
Point_2d getX () const
 
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
 
Point_2d getTheta () const
 
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< 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. More...
 

Additional Inherited Members

- Static Public Member Functions inherited from LensHaloParticles< float >
static std::vector< LensHaloParticles< float > > make (std::string filename, SimFileFormat format, float umass, float ulength, double inv_area, const COSMOLOGY &cosmo, int Nsmooth=5, float Nbucket=8, float theta=0.1, float rmax=0, Point_3d< float > xo=Point_3d< float >(0, 0, 0), bool verbose=false)
 
- 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
 
- Protected Member Functions inherited from LensHaloParticles< float >
 LensHaloParticles (PosType redshift, double my_inv_area_phys, PosType mass_particle, const COSMOLOGY &cosmo, int my_Nsmooth=5, float Nbucket=8, float theta=0.1, bool recenter=false, bool verbose=false)
 
void readPositionFileASCII (const std::string &filename)
 
void setUp (bool recenter, bool verbose)
 
- 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 inherited from LensHaloParticles< float >
Point_3d< float > mcenter
 
std::vector< Point_3d< float > > pp
 
int Nsmooth
 number of neighbours for adaptive smoothing
 
int Nbucket
 number of buckets in tree
 
double theta2
 square of opening angle for tree
 
double particle_mass
 mass
 
PosType inv_area
 
std::unique_ptr< OTreeNB< Point_3d< float >, float > > otree
 
- 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

template<typename DType = float>
class LensHaloParticlesM< DType >

LensHaloParticles but where the "particles" have different masses.

Constructor & Destructor Documentation

◆ LensHaloParticlesM()

template<typename DType = float>
LensHaloParticlesM< DType >::LensHaloParticlesM ( std::vector< Point_3d< DType > > &  pvector,
PosType  redshift,
double  my_inv_area_phys,
std::vector< DType >  Masses,
const COSMOLOGY &  cosmo,
int  my_Nsmooth = 5,
float  Nbucket = 8,
float  theta = 0.1,
bool  recenter = false,
bool  verbose = false 
)
inline
Parameters
pvectorlist of particles pdata[][i] should be the position in physical Mpc, the class takes possession of the data and leaves the vector empty
redshiftredshift of origin
my_inv_area_physinverse area for mass compensation, physical Mpc^-2
Massesrescale particle masses
cosmocosmology
my_Nsmoothnumber of neighbours for adaptive smoothing
Nbucketbuckets size in tree
thetaopening angle for tree
recenterre-center on center of mass

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