INTEGRAL/SPI instrument response function class. More...

#include <GSPIResponse.hpp>

Inheritance diagram for GSPIResponse:

Public Member Functions
	GSPIResponse (void)
	Void constructor.

	GSPIResponse (const GSPIResponse &rsp)
	Copy constructor.

	GSPIResponse (const GFilename &rspname)
	Response constructor.

virtual	~GSPIResponse (void)
	Destructor.

virtual GSPIResponse &	operator= (const GSPIResponse &rsp)
	Assignment operator.

virtual void	clear (void)
	Clear instance.

virtual GSPIResponse *	clone (void) const
	Clone instance.

virtual std::string	classname (void) const
	Return class name.

virtual bool	use_edisp (void) const
	Signal if energy dispersion will be used.

virtual bool	use_tdisp (void) const
	Signal if time dispersion will be used.

virtual double	irf (const GEvent &event, const GPhoton &photon, const GObservation &obs) const
	Return value of INTEGRAL/SPI instrument response for a photon.

virtual double	nroi (const GModelSky &model, const GEnergy &obsEng, const GTime &obsTime, const GObservation &obs) const
	Return integral of event probability for a given sky model over ROI.

virtual GEbounds	ebounds (const GEnergy &obsEnergy) const
	Return true energy boundaries for a specific observed energy.

virtual std::string	print (const GChatter &chatter=NORMAL) const
	Print INTEGRAL/SPI response information.

void	rspname (const GFilename &rspname)
	Set response name.

const GFilename &	rspname (void) const
	Get response group file name.

bool	is_precomputed (void) const
	Signals if response is precomputed.

const double &	energy_keV (void) const
	Return line IRF energy in keV.

const double &	dlogE (void) const
	Return logarithmic step size for continuum IRFs.

const double &	gamma (void) const
	Return power-law index for continuum IRFs.

void	set (const GSPIObservation &obs, const GEnergy &energy=GEnergy())
	Set response for a specific observation.

double	irf_value (const GSkyDir &srcDir, const GSPIEventBin &bin, const int &ireg) const
	Return value of INTEGRAL/SPI instrument response for sky direction and event bin.

double	zenith (const int &ipt, const GSkyDir &dir) const
	Return zenith angle of sky direction for pointing in radians.

double	azimuth (const int &ipt, const GSkyDir &dir) const
	Return azimuth angle of sky direction for pointing in radians.

void	read (const GFits &fits)
	Read SPI response from FITS object.

void	write (GFits &fits) const
	Write SPI response into FITS object.

void	load (const GFilename &filename)
	Load SPI response from file.

void	save (const GFilename &filename, const bool &clobber=false) const
	Save SPI response into file.

Public Member Functions inherited from GResponse
	GResponse (void)
	Void constructor.

	GResponse (const GResponse &rsp)
	Copy constructor.

virtual	~GResponse (void)
	Destructor.

virtual GResponse &	operator= (const GResponse &rsp)
	Assignment operator.

virtual double	convolve (const GModelSky &model, const GEvent &event, const GObservation &obs, const bool &grad=true) const
	Convolve sky model with the instrument response.

virtual GVector	convolve (const GModelSky &model, const GObservation &obs, GMatrixSparse *gradients=NULL) const
	Convolve sky model with the instrument response.

virtual double	irf_spatial (const GEvent &event, const GSource &source, const GObservation &obs) const
	Return instrument response integrated over the spatial model.

virtual GVector	irf_spatial (const GModelSky &model, const GObservation &obs, GMatrix *gradients=NULL) const
	Return instrument response vector integrated over the spatial model.

virtual void	remove_response_cache (const std::string &cache_id)
	Remove response cache for specific observation and model.

Public Member Functions inherited from GBase
virtual	~GBase (void)
	Destructor.

Private Member Functions
void	init_members (void)
	Initialise class members.

void	copy_members (const GSPIResponse &rsp)
	Copy class members.

void	free_members (void)
	Delete class members.

void	read_detids (const GFits &fits)
	Read detector identifiers from FITS object.

void	read_energies (const GFits &fits)
	Read energies from FITS object.

void	write_detids (GFits &fits) const
	Write detector identifiers into FITS object.

void	write_energies (GFits &fits) const
	Write energies into FITS object.

void	load_irfs (const int &region)
	Load Instrument Response Functions.

GSkyMap	load_irf (const GFilename &rspname) const
	Load IRF as sky map.

GSkyMap	compute_irf (const double &emin, const double &emax) const
	Compute as sky map.

void	set_wcs (const GFitsImage *image)
	Set IRF image limits.

void	set_detids (const GSPIEventCube *cube)
	Set vector of detector identifiers used by the observation.

void	set_cache (const GSPIEventCube *cube)
	Set computation cache.

void	irf_vector (const GSPIEventCube cube, const double &xpix, const double &ypix, const int &ireg, const double livetimes, GVector *irf) const
	Fill vector of INTEGRAL/SPI instrument response for IRF pixel.

int	irf_detid (const int &detid) const
	Convert detector identifier into IRF detector identifier.

double	irf_weight (const double &beta, const double &emin, const double &emax) const
	Compute weight of logarithmic energy bin.

void	irf_diffuse_map (const GModelSpatialDiffuseMap diffuse, const GObservation &obs, GVector irfs, GMatrix *gradients=NULL) const
	Return instrument response to diffuse map sky model.

void	irf_init (const GObservation &obs, GSPIResponseIrf *irf) const
	Initialise structure for projection computation of response.

void	irf_rot_matrix (const int &ipt, GSPIResponseIrf *irf) const
	Set rotation matrix for pointing.

void	irf_skydir (const int &ipt, const int &inx, GSPIResponseIrf *irf) const
	Set sky direction for pointing and IRF pixel index.

int	irf_map (const int &idet, const int &ieng, const GSPIResponseIrf *irf) const
	Return map index for detector and energy index.

virtual GVector	irf_ptsrc (const GModelSky &model, const GObservation &obs, GMatrix *gradients=NULL) const
	Return instrument response to point source sky model.

virtual GVector	irf_radial (const GModelSky &model, const GObservation &obs, GMatrix *gradients=NULL) const
	Return instrument response to radial source sky model.

virtual GVector	irf_elliptical (const GModelSky &model, const GObservation &obs, GMatrix *gradients=NULL) const
	Return instrument response to elliptical source sky model.

virtual GVector	irf_diffuse (const GModelSky &model, const GObservation &obs, GMatrix *gradients=NULL) const
	Return instrument response to diffuse source sky model.

Private Attributes
GFilename	m_rspname
	File name of response group.

std::vector< int >	m_detids
	Vector of detector IDs.

GNodeArray	m_energies
	Node array of IRF energies.

GEbounds	m_ebounds
	Energy bounaries of IRF.

GSkyMap	m_irfs
	IRFs stored as sky map.

double	m_energy_keV
	IRF line energy (optional)

double	m_dlogE
	Logarithmic energy step for IRF band.

double	m_gamma
	Power-law spectral index for IRF band.

std::vector< GSkyDir >	m_spix
	SPI pointing direction.

std::vector< double >	m_posang
	Position angle of Y axis (CEL, radians)

bool	m_has_wcs
	Has WCS information.

double	m_wcs_xmin
	Minimum X value (radians)

double	m_wcs_ymin
	Minimum Y value (radians)

double	m_wcs_xmax
	Maximum X value (radians)

double	m_wcs_ymax
	Maximum Y value (radians)

double	m_wcs_xbin
	X value bin size (radians)

double	m_wcs_ybin
	Y value bin size (radians)

double	m_wcs_xpix_max
	Maximum X pixel index.

double	m_wcs_ypix_max
	Maximum Y pixel index.

double	m_max_zenith
	Maximum zenith angle (radians)

Friends
class	spi_radial_kerns_rho

class	spi_radial_kerns_omega

class	spi_elliptical_kerns_rho

class	spi_elliptical_kerns_omega

Additional Inherited Members
Protected Member Functions inherited from GResponse
void	init_members (void)
	Initialise class members.

void	copy_members (const GResponse &rsp)
	Copy class members.

void	free_members (void)
	Delete class members.

double	eval_prob (const GModelSky &model, const GEvent &event, const GEnergy &srcEng, const GTime &srcTime, const GObservation &obs, const bool &grad) const
	Convolve sky model with the instrument response.

GVector	eval_probs (const GModelSky &model, const GObservation &obs, GMatrixSparse *gradients=NULL) const
	Convolve sky model with the instrument response.

int	size_edisp_vector (const GModelSky &model, const GObservation &obs, const bool &grad) const
	Return size of vector for energy dispersion computation.

GEbounds	ebounds_model (const GModelSky &model) const
	Return true energy intervals for sky model.

virtual double	irf_ptsrc (const GEvent &event, const GSource &source, const GObservation &obs) const
	Return instrument response to point source.

virtual double	irf_radial (const GEvent &event, const GSource &source, const GObservation &obs) const
	Return instrument response to radial source.

virtual double	irf_elliptical (const GEvent &event, const GSource &source, const GObservation &obs) const
	Return instrument response to elliptical source.

virtual double	irf_diffuse (const GEvent &event, const GSource &source, const GObservation &obs) const
	Return instrument response to diffuse source.

virtual double	irf_composite (const GEvent &event, const GSource &source, const GObservation &obs) const
	Return instrument response to composite source.

virtual GVector	irf_composite (const GModelSky &model, const GObservation &obs, GMatrix *gradients=NULL) const
	Return instrument response to composite source sky model.

Protected Attributes inherited from GResponse
bool	m_use_irf_cache
	Control usage of irf cache.

bool	m_use_nroi_cache
	Control usage of nroi cache.

int	m_irf_radial_iter_theta
	Radial model integration theta iterations.

int	m_irf_radial_iter_phi
	Radial model integration phi iterations.

int	m_irf_elliptical_iter_theta
	Elliptical model integration theta iterations.

int	m_irf_elliptical_iter_phi
	Elliptical model integration phi iterations.

double	m_irf_diffuse_resolution
	Angular resolution for diffuse model.

GResponseCache	m_irf_cache

GResponseCache	m_nroi_cache

GResponseVectorCache	m_irf_vector_cache

Detailed Description

INTEGRAL/SPI instrument response function class.

The INTEGRAL/SPI instrument response function class defines the function that translates from physical quantities to measured quantities.

Todo: Complete the class description.

Definition at line 89 of file GSPIResponse.hpp.

Constructor & Destructor Documentation

◆ GSPIResponse() [1/3]

GSPIResponse::GSPIResponse ( void )

Void constructor.

Creates an empty INTEGRAL/SPI response.

Definition at line 96 of file GSPIResponse.cpp.

References init_members().

Referenced by clone().

◆ GSPIResponse() [2/3]

GSPIResponse::GSPIResponse ( const GSPIResponse & rsp )

Copy constructor.

Parameters

[in] rsp INTEGRAL/SPI response.

Definition at line 133 of file GSPIResponse.cpp.

References copy_members(), and init_members().

◆ GSPIResponse() [3/3]

GSPIResponse::GSPIResponse ( const GFilename & rspname )

explicit

Response constructor.

Constructs an INTEGRAL/SPI response for an observation using a response group filename.

This constructor simply stores the file name of a response group, the actual loading will be done using the set() method.

Definition at line 115 of file GSPIResponse.cpp.

References init_members(), m_rspname, and rspname().

◆ ~GSPIResponse()

GSPIResponse::~GSPIResponse ( void )

virtual

Destructor.

Definition at line 149 of file GSPIResponse.cpp.

References free_members().

Member Function Documentation

◆ azimuth()

double GSPIResponse::azimuth	(	const int &	ipt,
		const GSkyDir &	dir ) const

inline

Return azimuth angle of sky direction for pointing in radians.

Parameters

[in]	ipt	Pointing index.
[in]	dir	Sky direction.

Returns: Azimuth angle (radians).

Returns azimuth angle of sky direction for pointing in radians.

Definition at line 374 of file GSPIResponse.hpp.

References azimuth(), m_posang, m_spix, and gammalib::twopi.

Referenced by azimuth(), spi_elliptical_kerns_omega::eval(), spi_radial_kerns_omega::eval(), irf_diffuse_map(), irf_ptsrc(), irf_skydir(), and irf_value().

◆ classname()

std::string GSPIResponse::classname ( void ) const

inlinevirtual

Return class name.

Returns: String containing the class name ("GSPIResponse").

Implements GResponse.

Definition at line 228 of file GSPIResponse.hpp.

◆ clear()

void GSPIResponse::clear ( void )

virtual

Clear instance.

Clears INTEGRAL/SPI response by resetting all class members to an initial state. Any information that was present before will be lost.

Implements GResponse.

Definition at line 212 of file GSPIResponse.cpp.

References GResponse::free_members(), free_members(), GResponse::init_members(), and init_members().

Referenced by GSPIObservation::init_members().

◆ clone()

GSPIResponse * GSPIResponse::clone ( void ) const

virtual

Clone instance.

Returns: Pointer to deep copy of INTEGRAL/SPI response.

Implements GResponse.

Definition at line 232 of file GSPIResponse.cpp.

References GSPIResponse().

◆ compute_irf()

GSkyMap GSPIResponse::compute_irf	(	const double &	emin,
		const double &	emax ) const

private

Compute as sky map.

Parameters

[in]	emin	Minimum energy (keV).
[in]	emax	Maximum energy (keV).

Compute IRF for an energy band specified by an energy interval. If the width of the energy interval is zero a line IRF will be computed.

Definition at line 1234 of file GSPIResponse.cpp.

References GNodeArray::inx_left(), GNodeArray::inx_right(), irf(), irf_weight(), gammalib::ln10, m_dlogE, m_energies, m_gamma, m_irfs, GSkyMap::npix(), GNodeArray::set_value(), GSkyMap::shape(), GNodeArray::wgt_left(), and GNodeArray::wgt_right().

Referenced by set().

◆ copy_members()

void GSPIResponse::copy_members ( const GSPIResponse & rsp )

private

Copy class members.

Parameters

[in] rsp INTEGRAL/SPI response function.

Definition at line 779 of file GSPIResponse.cpp.

References m_detids, m_dlogE, m_ebounds, m_energies, m_energy_keV, m_gamma, m_has_wcs, m_irfs, m_max_zenith, m_posang, m_rspname, m_spix, m_wcs_xbin, m_wcs_xmax, m_wcs_xmin, m_wcs_xpix_max, m_wcs_ybin, m_wcs_ymax, m_wcs_ymin, and m_wcs_ypix_max.

Referenced by GSPIResponse(), and operator=().

◆ dlogE()

const double & GSPIResponse::dlogE ( void ) const

inline

Return logarithmic step size for continuum IRFs.

Returns: Logarithmic step size for continuum IRFs.

Returns the logarithmic step size for the computation of continuum IRFs.

Definition at line 328 of file GSPIResponse.hpp.

References m_dlogE.

◆ ebounds()

GEbounds GSPIResponse::ebounds ( const GEnergy & obsEnergy ) const

virtual

Return true energy boundaries for a specific observed energy.

Parameters

[in] obsEnergy Observed Energy.

Returns: True energy boundaries for given observed energy.

Exceptions

GException::feature_not_implemented Method is not implemented.

Todo: Implement this method if you need energy dispersion.

Implements GResponse.

Definition at line 457 of file GSPIResponse.cpp.

References ebounds(), and G_EBOUNDS.

Referenced by ebounds().

◆ energy_keV()

const double & GSPIResponse::energy_keV ( void ) const

inline

Return line IRF energy in keV.

Returns: Line IRF energy (keV).

Returns the energy in keV for a line IRF. If the IRF is a continuum IRF the method returns 0.

Definition at line 314 of file GSPIResponse.hpp.

References m_energy_keV.

Referenced by GSPIObservation::write().

◆ free_members()

void GSPIResponse::free_members ( void )

private

Delete class members.

Definition at line 813 of file GSPIResponse.cpp.

Referenced by clear(), operator=(), and ~GSPIResponse().

◆ gamma()

const double & GSPIResponse::gamma ( void ) const

inline

Return power-law index for continuum IRFs.

Returns: Power-law index for continuum IRFs.

Returns the power-law index for the computation of continuum IRFs.

Definition at line 342 of file GSPIResponse.hpp.

References m_gamma.

◆ init_members()

void GSPIResponse::init_members ( void )

private

Initialise class members.

Definition at line 743 of file GSPIResponse.cpp.

References GEbounds::clear(), GFilename::clear(), GNodeArray::clear(), GSkyMap::clear(), gammalib::deg2rad, m_detids, m_dlogE, m_ebounds, m_energies, m_energy_keV, m_gamma, m_has_wcs, m_irfs, m_max_zenith, m_posang, m_rspname, m_spix, m_wcs_xbin, m_wcs_xmax, m_wcs_xmin, m_wcs_xpix_max, m_wcs_ybin, m_wcs_ymax, m_wcs_ymin, and m_wcs_ypix_max.

Referenced by clear(), GSPIResponse(), GSPIResponse(), GSPIResponse(), and operator=().

◆ irf()

double GSPIResponse::irf	(	const GEvent &	event,
		const GPhoton &	photon,
		const GObservation &	obs ) const

virtual

Return value of INTEGRAL/SPI instrument response for a photon.

Parameters

[in]	event	Observed event.
[in]	photon	Incident photon.
[in]	obs	Observation.

Returns: Instrument response \((cm^2 sr^{-1})\)

Exceptions

GException::invalid_argument Observation is not a INTEGRAL/SPI observation.

Returns the instrument response function for a given observed photon direction as function of the assumed true photon direction. The result is given by

\[ R(p'|p) = \]

Todo

Write down formula

Describe in detail how the response is computed.

Implements GResponse.

Definition at line 260 of file GSPIResponse.cpp.

References GPhoton::dir(), GEvents::ebounds(), GPhoton::energy(), GObservation::events(), G_IRF, GSPIEventBin::iebin(), irf(), irf_value(), gammalib::is_infinite(), gammalib::is_notanumber(), and GSPIEventBin::livetime().

Referenced by compute_irf(), irf(), irf_diffuse(), irf_elliptical(), irf_init(), irf_map(), irf_radial(), irf_rot_matrix(), irf_skydir(), irf_value(), irf_vector(), load_irf(), load_irfs(), and set().

◆ irf_detid()

int GSPIResponse::irf_detid ( const int & detid ) const

private

Convert detector identifier into IRF detector identifier.

Parameters

[in] detid SPI event detector identifier.

Returns: IRF detector identifier

Converts a SPI event detector identifier into an IRF detector identifier. TODO: Describe how this is done and why

Definition at line 1613 of file GSPIResponse.cpp.

References irf_detid().

Referenced by irf_detid(), irf_init(), irf_value(), irf_vector(), and set_detids().

◆ irf_diffuse()

GVector GSPIResponse::irf_diffuse	(	const GModelSky &	model,
		const GObservation &	obs,
		GMatrix *	gradients = NULL ) const

privatevirtual

Return instrument response to diffuse source sky model.

Parameters

[in]	model	Sky model.
[in]	obs	Observation.
[in]	gradients	Gradients matrix.

Returns: Instrument response to diffuse source sky model.

Returns the instrument response to a diffuse source sky model for all events. The methods works on response vectors that are computed per pointing. The method assumes that the spatial model component is of type GModelSpatialDiffuse and that the events in the observation are of type GSPIEventCube. No checking of these assumptions is performed by the method, and not respecting the assumptions will results in a segfault.

The computation is performed by projecting for each pointing the IRF pattern on the sky, and by evaluating the diffuse model at each IRF pixel.

Reimplemented from GResponse.

Definition at line 2203 of file GSPIResponse.cpp.

References GModelSpatialDiffuse::eval(), GObservation::events(), gammalib::get_current_clock(), irf(), GResponse::irf_diffuse(), irf_diffuse_map(), irf_init(), irf_map(), irf_rot_matrix(), irf_skydir(), GSPIEventCube::m_energy, m_irfs, GSPIEventCube::m_livetime, GSPIEventCube::m_num_det, GSPIEventCube::m_num_ebin, GSPIEventCube::m_num_pt, GModel::name(), GEvents::size(), and GModelSky::spatial().

◆ irf_diffuse_map()

void GSPIResponse::irf_diffuse_map	(	const GModelSpatialDiffuseMap *	diffuse,
		const GObservation &	obs,
		GVector *	irfs,
		GMatrix *	gradients = NULL ) const

private

Return instrument response to diffuse map sky model.

Parameters

[in]	diffuse	Pointer to diffuse map spatial model.
[in]	obs	Observation.
[out]	irfs	Pointer to IRF vector.
[in]	gradients	Gradients matrix.

Returns the instrument response to a diffuse source sky model for all events. The methods works on response vectors that are computed per pointing. The method assumes that the spatial model component is of type GModelSpatialDiffuseMap and that the events in the observation are of type GSPIEventCube. No checking of these assumptions is performed by the method, and not respecting the assumptions will results in a segfault.

Definition at line 2366 of file GSPIResponse.cpp.

References azimuth(), GObservation::events(), GSkyMap::inx2dir(), irf_vector(), GSPIEventCube::m_livetime, m_max_zenith, GSPIEventCube::m_num_det, GSPIEventCube::m_num_ebin, GSPIEventCube::m_num_pt, m_wcs_xbin, m_wcs_xmin, m_wcs_xpix_max, m_wcs_ybin, m_wcs_ymin, m_wcs_ypix_max, GModelSpatialDiffuseMap::map(), GSkyMap::npix(), GEvents::size(), GSkyMap::solidangle(), and zenith().

Referenced by irf_diffuse().

◆ irf_elliptical()

GVector GSPIResponse::irf_elliptical	(	const GModelSky &	model,
		const GObservation &	obs,
		GMatrix *	gradients = NULL ) const

privatevirtual

Return instrument response to elliptical source sky model.

Parameters

[in]	model	Sky model.
[in]	obs	Observation.
[in]	gradients	Gradients matrix.

Returns: Instrument response to ellipitical source sky model.

Returns the instrument response to a elliptical source sky model for all events. The methods works on response vectors that are computed per pointing. The method assumes that the spatial model component is of type GModelSpatialElliptical and that the events in the observation are of type GSPIEventCube. No checking of these assumptions is performed by the method, and not respecting the assumptions will results in a segfault.

The computation is performed by projecting for each pointing the IRF pattern on the sky, and by evaluating the elliptical model at each IRF pixel.

Reimplemented from GResponse.

Definition at line 1979 of file GSPIResponse.cpp.

References GModelSpatialElliptical::coordsys(), GSkyDir::dec_deg(), GModelSpatialElliptical::dir(), GSkyDir::dist(), GMatrix::eulery(), GMatrix::eulerz(), GModelSpatialElliptical::eval(), GObservation::events(), GIntegrals::fixed_iter(), gammalib::get_current_clock(), irf(), irf_init(), irf_map(), irf_rot_matrix(), irf_skydir(), m_irfs, GSPIEventCube::m_livetime, m_max_zenith, GSPIEventCube::m_num_det, GSPIEventCube::m_num_ebin, GSPIEventCube::m_num_pt, GSkyDir::posang(), GSkyDir::ra_deg(), GIntegrals::romberg(), GEvents::size(), GModelSky::spatial(), GModelSpatialElliptical::theta_max(), and zenith().

◆ irf_init()

void GSPIResponse::irf_init	(	const GObservation &	obs,
		GSPIResponseIrf *	irf ) const

private

Initialise structure for projection computation of response.

Parameters

[in]	obs	Observation.
[out]	irf	Stucture for projection computation of response.

The method initialises the irf structure that is needed for the projection computations of the response. The method initialises the following members of the structure:

nevents     : Number of events in observation
nirf        : Number of IRFs in observation
nx          : Number of pixels in x direction of IRF
ny          : Number of pixels in y direction of IRF
nxy         : Number of pixels of IRF
ndet        : Number of detectors in IRF
nreg        : Number of regions in IRF
ireg        : Used IRF region (set to 0, i.e. use photo peak response)
detids      : Vector of detector indices
zero        : Vector of booleans flagging IRF pixels that are zero
zeniths     : Zenith angles for all IRF pixels (radians)
sin_zeniths : Sine of zenith angles for all IRF pixels
cos_zeniths : Cosine of zenith angles for all IRF pixels
azimuths    : Azimuth angles for all IRF pixels (radians)
solidangle  : Solid angles for all IRF pixels

Definition at line 2477 of file GSPIResponse.cpp.

References GObservation::events(), irf(), irf_detid(), GSPIEventCube::m_detid, m_irfs, GSPIEventCube::m_num_det, GSPIEventCube::m_num_ebin, m_wcs_xbin, m_wcs_xmin, m_wcs_ybin, m_wcs_ymin, GSkyMap::nx(), GSkyMap::ny(), GSkyMap::shape(), GEvents::size(), and GSkyMap::solidangle().

Referenced by irf_diffuse(), irf_elliptical(), and irf_radial().

◆ irf_map()

int GSPIResponse::irf_map	(	const int &	idet,
		const int &	ieng,
		const GSPIResponseIrf *	irf ) const

inlineprivate

Return map index for detector and energy index.

Parameters

[in]	idet	Detector index.
[in]	ieng	Energy index.
[in]	irf	Stucture for projection computation of response.

Returns: Map index.

Returns the map index for a specific detector index idet and energy index ieng.

The client needs to make sure that the indices are comprised within the valid ranges and that the GSPIResponse::irf_init() method was called prior to invoking this method.

Definition at line 400 of file GSPIResponse.hpp.

References irf().

Referenced by irf_diffuse(), irf_elliptical(), and irf_radial().

◆ irf_ptsrc()

GVector GSPIResponse::irf_ptsrc	(	const GModelSky &	model,
		const GObservation &	obs,
		GMatrix *	gradients = NULL ) const

privatevirtual

Return instrument response to point source sky model.

Parameters

[in]	model	Sky model.
[in]	obs	Observation.
[in]	gradients	Gradients matrix.

Returns: Instrument response to point source sky model.

Returns the instrument response to a point source sky model for all events. The methods works on response vectors that are computed per pointing. The method assumes that the spatial model component is of type GModelSpatialPointSource and that the events in the observation are of type GSPIEventCube. No checking of these assumptions is performed by the method, and not respecting the assumptions will results in a segfault.

Reimplemented from GResponse.

Definition at line 1678 of file GSPIResponse.cpp.

References azimuth(), GModelSpatialPointSource::dir(), GObservation::events(), irf_vector(), GSPIEventCube::m_livetime, m_max_zenith, GSPIEventCube::m_num_det, GSPIEventCube::m_num_ebin, GSPIEventCube::m_num_pt, m_wcs_xbin, m_wcs_xmin, m_wcs_xpix_max, m_wcs_ybin, m_wcs_ymin, m_wcs_ypix_max, GEvents::size(), GModelSky::spatial(), and zenith().

◆ irf_radial()

GVector GSPIResponse::irf_radial	(	const GModelSky &	model,
		const GObservation &	obs,
		GMatrix *	gradients = NULL ) const

privatevirtual

Return instrument response to radial source sky model.

Parameters

[in]	model	Sky model.
[in]	obs	Observation.
[in]	gradients	Gradients matrix.

Returns: Instrument response to radial source sky model.

Returns the instrument response to a radial source sky model for all events. The methods works on response vectors that are computed per pointing. The method assumes that the spatial model component is of type GModelSpatialRadial and that the events in the observation are of type GSPIEventCube. No checking of these assumptions is performed by the method, and not respecting the assumptions will results in a segfault.

The computation is performed by projecting for each pointing the IRF pattern on the sky, and by evaluating the radial model at each IRF pixel.

Reimplemented from GResponse.

Definition at line 1757 of file GSPIResponse.cpp.

References GSkyDir::dec_deg(), GModelSpatialRadial::dir(), GSkyDir::dist(), GMatrix::eulery(), GMatrix::eulerz(), GModelSpatialRadial::eval(), GObservation::events(), GIntegrals::fixed_iter(), gammalib::get_current_clock(), irf(), irf_init(), irf_map(), irf_rot_matrix(), irf_skydir(), m_irfs, GSPIEventCube::m_livetime, m_max_zenith, GSPIEventCube::m_num_det, GSPIEventCube::m_num_ebin, GSPIEventCube::m_num_pt, GSkyDir::ra_deg(), GIntegrals::romberg(), GEvents::size(), GModelSky::spatial(), GModelSpatialRadial::theta_max(), and zenith().

◆ irf_rot_matrix()

void GSPIResponse::irf_rot_matrix	(	const int &	ipt,
		GSPIResponseIrf *	irf ) const

private

Set rotation matrix for pointing.

Parameters

[in]	ipt	Pointing index.
[in,out]	irf	Stucture for projection computation of response.

Sets the rotation matrix for the pointing with index ipt in the irf structure that allows rotation from the IRF coordinate system to the celestial coordinate system. The method sets the following member of the irf structure:

rot : Rotation matrix

The client needs to make sure that the pointing index is comprised within the valid range and that the GSPIResponse::irf_init() method was called prior to invoking this method.

Definition at line 2569 of file GSPIResponse.cpp.

References GMatrix::eulery(), GMatrix::eulerz(), irf(), and m_spix.

Referenced by irf_diffuse(), irf_elliptical(), and irf_radial().

◆ irf_skydir()

void GSPIResponse::irf_skydir	(	const int &	ipt,
		const int &	inx,
		GSPIResponseIrf *	irf ) const

private

Set sky direction for pointing and IRF pixel index.

Parameters

[in]	ipt	Pointing index.
[in]	inx	IRF pixel index.
[in,out]	irf	Stucture for projection computation of response.

Set the sky direction of the IRF pixel index inx for a given pointing index ipt. The method makes use of the rotation matrix that needs to be computed before by the GSPIResponse::irf_rot_matrix() method. The method sets the following member of the irf structure:

dir : Sky direction

The client needs to make sure that the pointing index and thr IRF pixel index is comprised within the valid ranges and that the GSPIResponse::irf_init() and GSPIResponse::irf_rot_matrix() methods were called prior to invoking this method.

Definition at line 2607 of file GSPIResponse.cpp.

References azimuth(), irf(), m_posang, m_wcs_xbin, m_wcs_xmin, m_wcs_ybin, m_wcs_ymin, and zenith().

Referenced by irf_diffuse(), irf_elliptical(), and irf_radial().

◆ irf_value()

double GSPIResponse::irf_value	(	const GSkyDir &	srcDir,
		const GSPIEventBin &	bin,
		const int &	ireg ) const

Return value of INTEGRAL/SPI instrument response for sky direction and event bin.

Parameters

[in]	srcDir	Sky direction.
[in]	bin	INTEGRAL/SPI event bin.
[in]	ireg	IRF region (0 = photo peak).

Returns: Instrument response \((cm^2 sr^{-1})\)

Returns the instrument response function for a given sky direction and event bin. The value of the IRF is bilinearly interpolated from the pre-computed IRFs cube that is stored in the class.

Definition at line 340 of file GSPIResponse.cpp.

References azimuth(), GSPIInstDir::detid(), GSPIEventBin::dir(), GSPIEventBin::iebin(), GSPIEventBin::ipt(), irf(), irf_detid(), m_irfs, m_max_zenith, m_wcs_xbin, m_wcs_xmin, m_wcs_xpix_max, m_wcs_ybin, m_wcs_ymin, m_wcs_ypix_max, GSkyMap::nx(), GSkyMap::shape(), and zenith().

Referenced by irf().

◆ irf_vector()

void GSPIResponse::irf_vector	(	const GSPIEventCube *	cube,
		const double &	xpix,
		const double &	ypix,
		const int &	ireg,
		const double *	livetimes,
		GVector *	irf ) const

private

Fill vector of INTEGRAL/SPI instrument response for IRF pixel.

Parameters

[in]	cube	Pointer to event cube.
[in]	xpix	Response pixel in X direction.
[in]	ypix	Response pixel in Y direction.
[in]	ireg	IRF region (0 = photo peak).
[in]	livetimes	livetimes Pointer to livetime array (dimension m_num_det).
[out]	irf	Response vector.

Computes a response vector for all detectors and energy bins for a given response pixel defined by xpix and ypix, where

xpix = (zenith * std::cos(azimuth) - m_wcs_xmin) / m_wcs_xbin
ypix = (zenith * std::sin(azimuth) - m_wcs_ymin) / m_wcs_ybin

Checking of the validity of xpix and ypix needs to be done by the client, makeing sure that

xpix > 0.0 && xpix < m_wcs_xpix_max && ypix > 0.0 && ypix < m_wcs_ypix_max

The client needs also to make sure that a vector with dimensions

m_num_det*m_num_ebin

is provided, and the method will fill all elements of the vector.

Definition at line 1521 of file GSPIResponse.cpp.

References irf(), irf_detid(), GSPIEventCube::m_detid, m_irfs, GSPIEventCube::m_num_det, GSPIEventCube::m_num_ebin, GSkyMap::nx(), and GSkyMap::shape().

Referenced by spi_elliptical_kerns_omega::eval(), spi_radial_kerns_omega::eval(), irf_diffuse_map(), and irf_ptsrc().

◆ irf_weight()

double GSPIResponse::irf_weight	(	const double &	beta,
		const double &	emin,
		const double &	emax ) const

private

Compute weight of logarithmic energy bin.

Parameters

[in]	beta	1-gamma.
[in]	emin	Logarithmic minimum energy.
[in]	emax	Logarithmic maximum energy.

Definition at line 1641 of file GSPIResponse.cpp.

References gammalib::ln10.

Referenced by compute_irf().

◆ is_precomputed()

bool GSPIResponse::is_precomputed ( void ) const

inline

Signals if response is precomputed.

Returns: True if response is precomputed.

Signals if the response was precomputed.

Definition at line 299 of file GSPIResponse.hpp.

References GEbounds::is_empty(), and m_ebounds.

◆ load()

void GSPIResponse::load ( const GFilename & filename )

Load SPI response from file.

Parameters

[in] filename Response file name.

Loads SPI response from response file.

Definition at line 628 of file GSPIResponse.cpp.

References GFits::close(), and read().

Referenced by GSPIObservation::read().

◆ load_irf()

GSkyMap GSPIResponse::load_irf ( const GFilename & irfname ) const

private

Load IRF as sky map.

Parameters

[in] irfname IRF file name.

Loads an IRF FITS file as a sky map. The sky map is returned in ARC projection that is a zenith equidistant projection, which is the projection that is natively used to store the IRFs.

Definition at line 1021 of file GSPIResponse.cpp.

References GFits::close(), gammalib::deg2rad, G_LOAD_IRF, GFits::image(), GFitsHDU::integer(), irf(), m_has_wcs, m_max_zenith, m_wcs_xbin, m_wcs_xmax, m_wcs_xmin, m_wcs_xpix_max, m_wcs_ybin, m_wcs_ymax, m_wcs_ymin, m_wcs_ypix_max, GFitsImage::pixel(), GFitsHDU::real(), and GFilename::url().

Referenced by load_irfs().

◆ load_irfs()

void GSPIResponse::load_irfs ( const int & region )

private

Load Instrument Response Functions.

Parameters

[in] region IRF region (-1 = load all regions)

The method requires that the required detector identifiers were previously setup using the set_detids() method.

Definition at line 1128 of file GSPIResponse.cpp.

References GNodeArray::append(), GNodeArray::clear(), GSkyMap::clear(), GFits::close(), G_LOAD_IRFS, irf(), load_irf(), m_detids, m_energies, m_irfs, m_rspname, GSkyMap::nmaps(), GFilename::path(), GSkyMap::shape(), gammalib::spi_hdu(), gammalib::spi_num_hdus(), and GFilename::url().

Referenced by set().

◆ nroi()

double GSPIResponse::nroi	(	const GModelSky &	model,
		const GEnergy &	obsEng,
		const GTime &	obsTime,
		const GObservation &	obs ) const

virtual

Return integral of event probability for a given sky model over ROI.

Parameters

[in]	model	Sky model.
[in]	obsEng	Observed photon energy.
[in]	obsTime	Observed photon arrival time.
[in]	obs	Observation.

Returns: 0.0

Exceptions

GException::feature_not_implemented Method is not implemented.

Implements GResponse.

Definition at line 431 of file GSPIResponse.cpp.

References G_NROI.

◆ operator=()

GSPIResponse & GSPIResponse::operator= ( const GSPIResponse & rsp )

virtual

Assignment operator.

Parameters

[in] rsp INTEGRAL/SPI response.

Returns: INTEGRAL/SPI response.

Assign INTEGRAL/SPI response to this object. The assignment performs a deep copy of all information, hence the original object from which the assignment was made can be destroyed after this operation without any loss of information.

Definition at line 176 of file GSPIResponse.cpp.

References copy_members(), free_members(), init_members(), and GResponse::operator=().

◆ print()

std::string GSPIResponse::print ( const GChatter & chatter = NORMAL ) const

virtual

Print INTEGRAL/SPI response information.

Parameters

[in] chatter Chattiness.

Returns: String containing INTEGRAL/SPI response information.

Implements GResponse.

Definition at line 677 of file GSPIResponse.cpp.

References m_dlogE, m_energy_keV, m_gamma, m_irfs, m_max_zenith, m_rspname, m_wcs_xmax, m_wcs_xmin, m_wcs_ymax, m_wcs_ymin, GSkyMap::nx(), GSkyMap::ny(), gammalib::parformat(), gammalib::rad2deg, GSkyMap::shape(), SILENT, gammalib::str(), and GFilename::url().

Referenced by GSPIObservation::print().

◆ read()

void GSPIResponse::read ( const GFits & fits )

Read SPI response from FITS object.

Parameters

[in] fits FITS object.

Reads the SPI response from FITS object.

Definition at line 576 of file GSPIResponse.cpp.

References GFits::image(), m_irfs, GSkyMap::read(), read_detids(), read_energies(), and set_wcs().

Referenced by load().

◆ read_detids()

void GSPIResponse::read_detids ( const GFits & fits )

private

Read detector identifiers from FITS object.

Parameters

[in] fits FITS object.

Read the detector identifiers from a FITS file into the m_detids member.

Definition at line 827 of file GSPIResponse.cpp.

References GFitsTableCol::integer(), m_detids, GFitsTable::nrows(), and GFits::table().

Referenced by read().

◆ read_energies()

void GSPIResponse::read_energies ( const GFits & fits )

private

Read energies from FITS object.

Parameters

[in] fits FITS object.

Read the energies from a FITS file. If the FITS file contains energy boundaries then read them, otherwise read the energy vector.

Definition at line 860 of file GSPIResponse.cpp.

References GNodeArray::append(), GEbounds::clear(), GNodeArray::clear(), GFits::contains(), gammalib::extname_ebounds, gammalib::extname_energies, GFitsHDU::has_card(), GEnergy::keV(), m_dlogE, m_ebounds, m_energies, m_energy_keV, m_gamma, GFitsTable::nrows(), GEbounds::read(), GFitsHDU::real(), GFitsTableCol::real(), GNodeArray::reserve(), GFitsHDU::string(), and GFits::table().

Referenced by read().

◆ rspname() [1/2]

void GSPIResponse::rspname ( const GFilename & rspname )

inline

Set response name.

Parameters

[in] rspname Response group file name.

Sets the response group file name.

Definition at line 270 of file GSPIResponse.hpp.

References m_rspname, and rspname().

Referenced by GSPIObservation::read(), and GSPIObservation::write().

◆ rspname() [2/2]

const GFilename & GSPIResponse::rspname ( void ) const

inline

Get response group file name.

Returns: Response group file name.

Returns the response group file name.

Definition at line 285 of file GSPIResponse.hpp.

References m_rspname.

Referenced by GSPIResponse(), and rspname().

◆ save()

void GSPIResponse::save	(	const GFilename &	filename,
		const bool &	clobber = false ) const

Save SPI response into file.

Parameters

[in]	filename	Response file name.
[in]	clobber	Overwrite existing FITS file?

Saves SPI response into response file.

Definition at line 652 of file GSPIResponse.cpp.

References GFits::close(), GFits::saveto(), and write().

◆ set()

void GSPIResponse::set	(	const GSPIObservation &	obs,
		const GEnergy &	energy = GEnergy() )

Set response for a specific observation.

Parameters

[in]	obs	INTEGRAL/SPI observation.
[in]	energy	Line energy

Sets the response for a specific INTEGRAL/SPI observation. This is the high-level method for loading and pre-computing SPI IRFs for a specific energy binning. The method loads the IRF from a response group file and pre-computes the IRFs for all energy bins of the SPI observation. If energy is positive, IRFs will be pre-computed taking a line energy specified by energy, otherwise the IRFs will be pre-computed taking the energy interval of the energy bins (continuum IRFs).

Definition at line 485 of file GSPIResponse.cpp.

References GEbounds::append(), GEbounds::clear(), GNodeArray::clear(), GSkyMap::clear(), compute_irf(), GEvents::ebounds(), GObservation::events(), irf(), GEnergy::keV(), load_irfs(), m_detids, m_ebounds, m_energies, m_energy_keV, m_has_wcs, m_irfs, GSPIEventCube::naxis(), GSkyMap::nmaps(), GSkyMap::npix(), set_cache(), set_detids(), and GSkyMap::shape().

Referenced by GSPIObservation::read().

◆ set_cache()

void GSPIResponse::set_cache ( const GSPIEventCube * cube )

private

Set computation cache.

Parameters

[in] cube INTEGRAL/SPI event cube.

Setup of two vectors for fast coordinate transformation into the instrument system. The first vector m_spix stores the SPI pointing direction (the X direction) while the second vector stores the position angle in celestial coordinates of the SPI Y direction.

Definition at line 1466 of file GSPIResponse.cpp.

References m_posang, m_spix, GSPIEventCube::naxis(), gammalib::pihalf, GSkyDir::posang(), GSPIEventCube::spi_x(), and GSPIEventCube::spi_z().

Referenced by set().

◆ set_detids()

void GSPIResponse::set_detids ( const GSPIEventCube * cube )

private

Set vector of detector identifiers used by the observation.

Parameters

[in] cube INTEGRAL/SPI event cube.

Sets the vector of detector identifiers that is used by the observation. The method scans the detector identifiers for all pointings and builds a vector of unique detector identifiers in the order they were encountered in the event cube.

Definition at line 1426 of file GSPIResponse.cpp.

References GSPIInstDir::detid(), GSPIEventCube::dir(), irf_detid(), m_detids, and GSPIEventCube::naxis().

Referenced by set().

◆ set_wcs()

void GSPIResponse::set_wcs ( const GFitsImage * image )

private

Set IRF image limits.

Parameters

[in] image IRF FITS image.

Computes the IRF image limits.

Definition at line 1380 of file GSPIResponse.cpp.

References gammalib::deg2rad, GFitsHDU::integer(), m_has_wcs, m_max_zenith, m_wcs_xbin, m_wcs_xmax, m_wcs_xmin, m_wcs_xpix_max, m_wcs_ybin, m_wcs_ymax, m_wcs_ymin, m_wcs_ypix_max, and GFitsHDU::real().

Referenced by read().

◆ use_edisp()

bool GSPIResponse::use_edisp ( void ) const

inlinevirtual

Signal if energy dispersion will be used.

Returns: False.

Todo: Implement method as needed.

Implements GResponse.

Definition at line 242 of file GSPIResponse.hpp.

◆ use_tdisp()

bool GSPIResponse::use_tdisp ( void ) const

inlinevirtual

Signal if time dispersion will be used.

Returns: False.

Todo: Implement method as needed.

Implements GResponse.

Definition at line 256 of file GSPIResponse.hpp.

◆ write()

void GSPIResponse::write ( GFits & fits ) const

Write SPI response into FITS object.

Parameters

[in,out] fits FITS object.

Writes the SPI response into FITS object.

Definition at line 605 of file GSPIResponse.cpp.

References m_irfs, GSkyMap::write(), write_detids(), and write_energies().

Referenced by save().

◆ write_detids()

void GSPIResponse::write_detids ( GFits & fits ) const

private

Write detector identifiers into FITS object.

Parameters

[in,out] fits FITS object.

Writes the detector identifiers stored into the m_detids member into a FITS object.

Definition at line 929 of file GSPIResponse.cpp.

References GFits::append(), GFitsTable::append(), GFitsHDU::extname(), and m_detids.

Referenced by write().

◆ write_energies()

void GSPIResponse::write_energies ( GFits & fits ) const

private

Write energies into FITS object.

Parameters

[in,out] fits FITS object.

Writes the energy nodes stored into the m_energies member into a FITS object. The energies are written in units of keV.

Definition at line 963 of file GSPIResponse.cpp.

References GFits::append(), GFitsTable::append(), GFitsHDU::card(), GFitsHDU::extname(), gammalib::extname_ebounds, gammalib::extname_energies, GEbounds::is_empty(), m_dlogE, m_ebounds, m_energies, m_energy_keV, m_gamma, GNodeArray::size(), GFits::table(), GFitsTableCol::unit(), and GEbounds::write().

Referenced by write().

◆ zenith()

double GSPIResponse::zenith	(	const int &	ipt,
		const GSkyDir &	dir ) const

inline

Return zenith angle of sky direction for pointing in radians.

Parameters

[in]	ipt	Pointing index.
[in]	dir	Sky direction.

Returns: Zenith angle (radians).

Returns zenith angle of sky direction for pointing in radians.

Definition at line 358 of file GSPIResponse.hpp.

References m_spix.

Referenced by spi_elliptical_kerns_omega::eval(), spi_radial_kerns_omega::eval(), irf_diffuse_map(), irf_elliptical(), irf_ptsrc(), irf_radial(), irf_skydir(), and irf_value().

Friends And Related Symbol Documentation

◆ spi_elliptical_kerns_omega

friend class spi_elliptical_kerns_omega

friend

Definition at line 95 of file GSPIResponse.hpp.

◆ spi_elliptical_kerns_rho

friend class spi_elliptical_kerns_rho

friend

Definition at line 94 of file GSPIResponse.hpp.

◆ spi_radial_kerns_omega

friend class spi_radial_kerns_omega

friend

Definition at line 93 of file GSPIResponse.hpp.

◆ spi_radial_kerns_rho

friend class spi_radial_kerns_rho

friend

Definition at line 92 of file GSPIResponse.hpp.

Member Data Documentation

◆ m_detids

std::vector<int> GSPIResponse::m_detids

private

Vector of detector IDs.

Definition at line 198 of file GSPIResponse.hpp.

Referenced by copy_members(), init_members(), load_irfs(), read_detids(), set(), set_detids(), and write_detids().

◆ m_dlogE

double GSPIResponse::m_dlogE

private

Logarithmic energy step for IRF band.

Definition at line 203 of file GSPIResponse.hpp.

Referenced by compute_irf(), copy_members(), dlogE(), init_members(), print(), read_energies(), and write_energies().

◆ m_ebounds

GEbounds GSPIResponse::m_ebounds

private

Energy bounaries of IRF.

Definition at line 200 of file GSPIResponse.hpp.

Referenced by copy_members(), init_members(), is_precomputed(), read_energies(), set(), and write_energies().

◆ m_energies

GNodeArray GSPIResponse::m_energies

private

Node array of IRF energies.

Definition at line 199 of file GSPIResponse.hpp.

Referenced by compute_irf(), copy_members(), init_members(), load_irfs(), read_energies(), set(), and write_energies().

◆ m_energy_keV

double GSPIResponse::m_energy_keV

private

IRF line energy (optional)

Definition at line 202 of file GSPIResponse.hpp.

Referenced by copy_members(), energy_keV(), init_members(), print(), read_energies(), set(), and write_energies().

◆ m_gamma

double GSPIResponse::m_gamma

private

Power-law spectral index for IRF band.

Definition at line 204 of file GSPIResponse.hpp.

Referenced by compute_irf(), copy_members(), gamma(), init_members(), print(), read_energies(), and write_energies().

◆ m_has_wcs

bool GSPIResponse::m_has_wcs

mutableprivate

Has WCS information.

Definition at line 209 of file GSPIResponse.hpp.

Referenced by copy_members(), init_members(), load_irf(), set(), and set_wcs().

◆ m_irfs

GSkyMap GSPIResponse::m_irfs

private

IRFs stored as sky map.

Definition at line 201 of file GSPIResponse.hpp.

Referenced by compute_irf(), copy_members(), init_members(), irf_diffuse(), irf_elliptical(), irf_init(), irf_radial(), irf_value(), irf_vector(), load_irfs(), print(), read(), set(), and write().

◆ m_max_zenith

double GSPIResponse::m_max_zenith

mutableprivate

Maximum zenith angle (radians)

Definition at line 218 of file GSPIResponse.hpp.

Referenced by copy_members(), init_members(), irf_diffuse_map(), irf_elliptical(), irf_ptsrc(), irf_radial(), irf_value(), load_irf(), print(), and set_wcs().

◆ m_posang

std::vector<double> GSPIResponse::m_posang

private

Position angle of Y axis (CEL, radians)

Definition at line 208 of file GSPIResponse.hpp.

Referenced by azimuth(), copy_members(), init_members(), irf_skydir(), and set_cache().

◆ m_rspname

GFilename GSPIResponse::m_rspname

private

File name of response group.

Definition at line 197 of file GSPIResponse.hpp.

Referenced by copy_members(), GSPIResponse(), init_members(), load_irfs(), print(), rspname(), and rspname().

◆ m_spix

std::vector<GSkyDir> GSPIResponse::m_spix

private

SPI pointing direction.

Definition at line 207 of file GSPIResponse.hpp.

Referenced by azimuth(), copy_members(), init_members(), irf_rot_matrix(), set_cache(), and zenith().

◆ m_wcs_xbin

double GSPIResponse::m_wcs_xbin

mutableprivate

X value bin size (radians)

Definition at line 214 of file GSPIResponse.hpp.

Referenced by copy_members(), spi_elliptical_kerns_omega::eval(), spi_radial_kerns_omega::eval(), init_members(), irf_diffuse_map(), irf_init(), irf_ptsrc(), irf_skydir(), irf_value(), load_irf(), and set_wcs().

◆ m_wcs_xmax

double GSPIResponse::m_wcs_xmax

mutableprivate

Maximum X value (radians)

Definition at line 212 of file GSPIResponse.hpp.

Referenced by copy_members(), init_members(), load_irf(), print(), and set_wcs().

◆ m_wcs_xmin

double GSPIResponse::m_wcs_xmin

mutableprivate

Minimum X value (radians)

Definition at line 210 of file GSPIResponse.hpp.

Referenced by copy_members(), spi_elliptical_kerns_omega::eval(), spi_radial_kerns_omega::eval(), init_members(), irf_diffuse_map(), irf_init(), irf_ptsrc(), irf_skydir(), irf_value(), load_irf(), print(), and set_wcs().

◆ m_wcs_xpix_max

double GSPIResponse::m_wcs_xpix_max

mutableprivate

Maximum X pixel index.

Definition at line 216 of file GSPIResponse.hpp.

Referenced by copy_members(), init_members(), irf_diffuse_map(), irf_ptsrc(), irf_value(), load_irf(), and set_wcs().

◆ m_wcs_ybin

double GSPIResponse::m_wcs_ybin

mutableprivate

Y value bin size (radians)

Definition at line 215 of file GSPIResponse.hpp.

Referenced by copy_members(), spi_elliptical_kerns_omega::eval(), spi_radial_kerns_omega::eval(), init_members(), irf_diffuse_map(), irf_init(), irf_ptsrc(), irf_skydir(), irf_value(), load_irf(), and set_wcs().

◆ m_wcs_ymax

double GSPIResponse::m_wcs_ymax

mutableprivate

Maximum Y value (radians)

Definition at line 213 of file GSPIResponse.hpp.

Referenced by copy_members(), init_members(), load_irf(), print(), and set_wcs().

◆ m_wcs_ymin

double GSPIResponse::m_wcs_ymin

mutableprivate

Minimum Y value (radians)

Definition at line 211 of file GSPIResponse.hpp.

Referenced by copy_members(), spi_elliptical_kerns_omega::eval(), spi_radial_kerns_omega::eval(), init_members(), irf_diffuse_map(), irf_init(), irf_ptsrc(), irf_skydir(), irf_value(), load_irf(), print(), and set_wcs().

◆ m_wcs_ypix_max

double GSPIResponse::m_wcs_ypix_max

mutableprivate

Maximum Y pixel index.

Definition at line 217 of file GSPIResponse.hpp.

Referenced by copy_members(), init_members(), irf_diffuse_map(), irf_ptsrc(), irf_value(), load_irf(), and set_wcs().

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

inst/spi/include/GSPIResponse.hpp
inst/spi/src/GSPIResponse.cpp

Public Member Functions

Private Member Functions

Private Attributes

Friends

Additional Inherited Members

Detailed Description

Constructor & Destructor Documentation

◆ GSPIResponse() [1/3]

◆ GSPIResponse() [2/3]

◆ GSPIResponse() [3/3]

◆ ~GSPIResponse()

Member Function Documentation

◆ azimuth()

◆ classname()

◆ clear()

◆ clone()

◆ compute_irf()

◆ copy_members()

◆ dlogE()

◆ ebounds()

◆ energy_keV()

◆ free_members()

◆ gamma()

◆ init_members()

◆ irf()

◆ irf_detid()

◆ irf_diffuse()

◆ irf_diffuse_map()

◆ irf_elliptical()

◆ irf_init()

◆ irf_map()

◆ irf_ptsrc()

◆ irf_radial()

◆ irf_rot_matrix()

◆ irf_skydir()

◆ irf_value()

◆ irf_vector()

◆ irf_weight()

◆ is_precomputed()

◆ load()

◆ load_irf()

◆ load_irfs()

◆ nroi()

◆ operator=()

◆ print()

◆ read()

◆ read_detids()

◆ read_energies()

◆ rspname() [1/2]

◆ rspname() [2/2]

◆ save()

◆ set()

◆ set_cache()

◆ set_detids()

◆ set_wcs()

◆ use_edisp()

◆ use_tdisp()

◆ write()

◆ write_detids()

◆ write_energies()

◆ zenith()

Friends And Related Symbol Documentation

◆ spi_elliptical_kerns_omega

◆ spi_elliptical_kerns_rho

◆ spi_radial_kerns_omega

◆ spi_radial_kerns_rho

Member Data Documentation

◆ m_detids

◆ m_dlogE

◆ m_ebounds

◆ m_energies

◆ m_energy_keV

◆ m_gamma

◆ m_has_wcs

◆ m_irfs

◆ m_max_zenith

◆ m_posang

◆ m_rspname

◆ m_spix

◆ m_wcs_xbin