GLATResponse.cpp
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/***************************************************************************
* GLATResponse.cpp - Fermi/LAT response class *
* ----------------------------------------------------------------------- *
* copyright (C) 2008-2015 by Juergen Knoedlseder *
* ----------------------------------------------------------------------- *
* *
* This program is free software: you can redistribute it and/or modify *
* it under the terms of the GNU General Public License as published by *
* the Free Software Foundation, either version 3 of the License, or *
* (at your option) any later version. *
* *
* This program is distributed in the hope that it will be useful, *
* but WITHOUT ANY WARRANTY; without even the implied warranty of *
* MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the *
* GNU General Public License for more details. *
* *
* You should have received a copy of the GNU General Public License *
* along with this program. If not, see <http://www.gnu.org/licenses/>. *
* *
***************************************************************************/
/**
* @file GLATResponse.cpp
* @brief Fermi/LAT response class implementation
* @author Juergen Knoedlseder
*/
/* __ Includes ___________________________________________________________ */
#ifdef HAVE_CONFIG_H
#include <config.h>
#endif
#include <unistd.h> // access() function
#include <cstdlib> // std::getenv() function
#include <string>
#include "GException.hpp"
#include "GFits.hpp"
#include "GTools.hpp"
#include "GCaldb.hpp"
#include "GSource.hpp"
#include "GModelSpatialPointSource.hpp"
#include "GLATInstDir.hpp"
#include "GLATResponse.hpp"
#include "GLATObservation.hpp"
#include "GLATEventAtom.hpp"
#include "GLATEventBin.hpp"
#include "GLATEventCube.hpp"
#include "GLATException.hpp"
/* __ Method name definitions ____________________________________________ */
#define G_CALDB "GLATResponse::caldb(std::string&)"
#define G_LOAD "GLATResponse::load(std::string&)"
#define G_IRF "GLATResponse::irf(GInstDir&, GEnergy&, GTime&, GSkyDir&,"\
" GEnergy&, GTime&, GObservation&)"
#define G_NROI "GLATResponse::nroi(GModelSky&, GEnergy&, GTime&, "\
"GObservation&)"
#define G_EBOUNDS "GLATResponse::ebounds(GEnergy&)"
#define G_AEFF "GLATResponse::aeff(int&)"
#define G_PSF "GLATResponse::psf(int&)"
#define G_EDISP "GLATResponse::edisp(int&)"
#define G_IRF_ATOM "GLATResponse::irf(GLATEventAtom&, GModel&, GEnergy&,"\
"GTime&, GObservation&)"
#define G_IRF_BIN "GLATResponse::irf(GLATEventBin&, GModel&, GEnergy&,"\
"GTime&, GObservation&)"
/* __ Macros _____________________________________________________________ */
/* __ Coding definitions _________________________________________________ */
/* __ Debug definitions __________________________________________________ */
#define G_DUMP_MEAN_PSF 0 //!< Dump mean PSF allocation
#define G_DEBUG_MEAN_PSF 0 //!< Debug mean PSF computation
/* __ Constants __________________________________________________________ */
/*==========================================================================
= =
= Constructors/destructors =
= =
==========================================================================*/
/***********************************************************************//**
* @brief Void constructor
***************************************************************************/
GLATResponse::GLATResponse(void) : GResponse()
{
// Initialise members
init_members();
// Return
return;
}
/***********************************************************************//**
* @brief Copy constructor
*
* @param[in] rsp Response.
***************************************************************************/
GLATResponse::GLATResponse(const GLATResponse& rsp) : GResponse(rsp)
{
// Initialise members
init_members();
// Copy members
copy_members(rsp);
// Return
return;
}
/***********************************************************************//**
* @brief Destructor
***************************************************************************/
GLATResponse::~GLATResponse(void)
{
// Free members
free_members();
// Return
return;
}
/*==========================================================================
= =
= Operators =
= =
==========================================================================*/
/***********************************************************************//**
* @brief Assignment operator
*
* @param[in] rsp Response.
* @return Response.
***************************************************************************/
GLATResponse& GLATResponse::operator=(const GLATResponse& rsp)
{
// Execute only if object is not identical
if (this != &rsp) {
// Copy base class members
this->GResponse::operator=(rsp);
// Free members
free_members();
// Initialise members
init_members();
// Copy members
copy_members(rsp);
} // endif: object was not identical
// Return this object
return *this;
}
/*==========================================================================
= =
= Public methods =
= =
==========================================================================*/
/***********************************************************************//**
* @brief Clear response
***************************************************************************/
void GLATResponse::clear(void)
{
// Free class members (base and derived classes, derived class first)
free_members();
this->GResponse::free_members();
// Initialise members
this->GResponse::init_members();
init_members();
// Return
return;
}
/***********************************************************************//**
* @brief Clone response
*
* @return Pointer to deep copy of response.
***************************************************************************/
GLATResponse* GLATResponse::clone(void) const
{
return new GLATResponse(*this);
}
/***********************************************************************//**
* @brief Set path to the calibration database
*
* @param[in] caldb Path to calibration database
*
* @exception GException::caldb_not_found
* Calibration database repository not found.
*
* This method stores the CALDB root directory as the path to the LAT
* calibration database.
*
* @todo Make use of the LAT CALDB to translate IRF names into filenames.
***************************************************************************/
void GLATResponse::caldb(const std::string& caldb)
{
// Allocate calibration database
GCaldb db(caldb);
// Store the path to the calibration database
m_caldb = db.rootdir();
// Return
return;
}
/***********************************************************************//**
* @brief Return value of point source IRF
*
* @param[in] event Observed event.
* @param[in] photon Incident photon.
* @param[in] obs Observation.
*
* @exception GLATException::bad_instdir_type
* Instrument direction is not a valid LAT instrument direction.
*
* @todo The IRF value is not devided by ontime of the event, but it is
* already time integrated.
***************************************************************************/
double GLATResponse::irf(const GEvent& event,
const GPhoton& photon,
const GObservation& obs) const
{
// Get pointer to LAT instrument direction
const GLATInstDir* dir = dynamic_cast<const GLATInstDir*>(&(event.dir()));
if (dir == NULL) {
throw GLATException::bad_instdir_type(G_IRF);
}
// Get photon attributes
const GSkyDir& srcDir = photon.dir();
const GEnergy& srcEng = photon.energy();
// Search for mean PSF
int ipsf = -1;
for (int i = 0; i < m_ptsrc.size(); ++i) {
if (m_ptsrc[i]->dir() == srcDir) {
ipsf = i;
break;
}
}
// If mean PSF has not been found then create it now
if (ipsf == -1) {
// Allocate new mean PSF
GLATMeanPsf* psf = new GLATMeanPsf(srcDir, static_cast<const GLATObservation&>(obs));
// Set source name
std::string name = "SRC("+gammalib::str(srcDir.ra_deg()) +
"," +
gammalib::str(srcDir.dec_deg())+")";
psf->name(name);
// Push mean PSF on stack
const_cast<GLATResponse*>(this)->m_ptsrc.push_back(psf);
// Set index of mean PSF
ipsf = m_ptsrc.size()-1;
// Debug option: dump mean PSF
#if G_DUMP_MEAN_PSF
std::cout << "Added new mean PSF \""+name+"\"" << std::endl;
std::cout << *psf << std::endl;
#endif
} // endif: created new mean PSF
// Get IRF value
double offset = dir->dir().dist_deg(srcDir);
double irf = (*m_ptsrc[ipsf])(offset, srcEng.log10MeV());
// Return IRF value
return irf;
}
/***********************************************************************//**
* @brief Return value of model instrument response function
*
* @param[in] event Event.
* @param[in] source Source.
* @param[in] obs Observation.
*
* This method returns the response of the instrument to a specific source
* model. The method handles both event atoms and event bins.
***************************************************************************/
double GLATResponse::irf(const GEvent& event,
const GSource& source,
const GObservation& obs) const
{
// Get IRF value
double rsp;
if (event.is_atom()) {
rsp = irf(static_cast<const GLATEventAtom&>(event), source, obs);
}
else {
rsp = irf(static_cast<const GLATEventBin&>(event), source, obs);
}
// Return IRF value
return rsp;
}
/***********************************************************************//**
* @brief Return value of model IRF for event atom
*
* @param[in] event Event atom.
* @param[in] source Source.
* @param[in] obs Observations.
*
* @exception GException::feature_not_implemented
* Method not yet implemented.
*
* @todo Not yet implemented.
***************************************************************************/
double GLATResponse::irf(const GLATEventAtom& event,
const GSource& source,
const GObservation& obs) const
{
// Initialise IRF with "no response"
double irf = 0.0;
// Dump warning that integration is not yet implemented
throw GException::feature_not_implemented(G_IRF_ATOM);
// Return IRF value
return irf;
}
/***********************************************************************//**
* @brief Return value of model IRF for event bin
*
* @param[in] event Event bin.
* @param[in] source Source.
* @param[in] obs Observation.
*
* @exception GLATException::diffuse_not_found
* Diffuse model not found.
*
* This method first searches for a corresponding source map, and if found,
* computes the response from the source map. If no source map is present
* it checks if the source is a point source. If this is the case a mean
* PSF is allocated for the source and the response is computed from the
* mean PSF. Otherwise an GLATException::diffuse_not_found exception is
* thrown.
*
* @todo Extract event cube from observation. We do not need the cube
* pointer in the event anymore.
* @todo Implement more efficient method for response search (name search is
* not very rapid).
* @todo Instead of calling "offset = event.dir().dist_deg(srcDir)" we can
* precompute and store for each PSF the offsets. This should save
* quite some time since the distance computation is time
* consuming.
***************************************************************************/
double GLATResponse::irf(const GLATEventBin& event,
const GSource& source,
const GObservation& obs) const
{
// Initialise response value
double rsp = 0.0;
// Get pointer to event cube
const GLATEventCube* cube = event.cube();
// Get pointer on point source spatial model
const GModelSpatialPointSource* ptsrc =
dynamic_cast<const GModelSpatialPointSource*>(source.model());
// Get source energy
GEnergy srcEng = source.energy();
// Search for diffuse response in event cube
int idiff = -1;
for (int i = 0; i < cube->ndiffrsp(); ++i) {
if (cube->diffname(i) == source.name()) {
idiff = i;
break;
}
}
// If diffuse response has been found then get response from source map
if (idiff != -1) {
// Get srcmap indices and weighting factors
GNodeArray nodes = cube->enodes();
nodes.set_value(srcEng.log10MeV());
// Compute diffuse response
GSkymap* map = cube->diffrsp(idiff);
const double* pixels = map->pixels() + event.ipix();
rsp = nodes.wgt_left() * pixels[nodes.inx_left() * map->npix()] +
nodes.wgt_right() * pixels[nodes.inx_right() * map->npix()];
// Divide by solid angle and ontime since source maps are given in units of
// counts/pixel/MeV.
rsp /= (event.solidangle() * event.ontime());
} // endelse: diffuse response was present
// ... otherwise check if model is a point source. If this is true
// then return response from mean PSF
if ((idiff == -1 || m_force_mean) && ptsrc != NULL) {
// Search for mean PSF
int ipsf = -1;
for (int i = 0; i < m_ptsrc.size(); ++i) {
if (m_ptsrc[i]->name() == source.name()) {
ipsf = i;
break;
}
}
// If mean PSF has not been found then create it now
if (ipsf == -1) {
// Allocate new mean PSF
GLATMeanPsf* psf =
new GLATMeanPsf(ptsrc->dir(), static_cast<const GLATObservation&>(obs));
// Set source name
psf->name(source.name());
// Push mean PSF on stack
const_cast<GLATResponse*>(this)->m_ptsrc.push_back(psf);
// Set index of mean PSF
ipsf = m_ptsrc.size()-1;
// Debug option: dump mean PSF
#if G_DUMP_MEAN_PSF
std::cout << "Added new mean PSF \""+source.name() << "\"" << std::endl;
std::cout << *psf << std::endl;
#endif
} // endif: created new mean PSF
// Get PSF value
GSkyDir srcDir = m_ptsrc[ipsf]->dir();
double offset = event.dir().dir().dist_deg(srcDir);
double mean_psf = (*m_ptsrc[ipsf])(offset, srcEng.log10MeV()) / (event.ontime());
// Debug option: compare mean PSF to diffuse response
#if G_DEBUG_MEAN_PSF
std::cout << "Energy=" << srcEng.MeV();
std::cout << " MeanPsf=" << mean_psf;
std::cout << " DiffusePsf=" << rsp;
std::cout << " ratio(Mean/Diffuse)=" << mean_psf/rsp;
if (mean_psf/rsp < 0.99) {
std::cout << " <<< (1%)";
}
else if (mean_psf/rsp > 1.01) {
std::cout << " >>> (1%)";
}
std::cout << std::endl;
#endif
// Set response
rsp = mean_psf;
} // endif: model was point source
// ... otherwise throw an exception
if ((idiff == -1) && ptsrc == NULL) {
throw GLATException::diffuse_not_found(G_IRF_BIN, source.name());
}
// Return IRF value
return rsp;
}
/***********************************************************************//**
* @brief Return integral of event probability for a given sky model over ROI
*
* @param[in] model Sky model.
* @param[in] obsEng Observed photon energy.
* @param[in] obsTime Observed photon arrival time.
* @param[in] obs Observation.
* @return 0.0
*
* @exception GException::feature_not_implemented
* Method is not implemented.
***************************************************************************/
double GLATResponse::nroi(const GModelSky& model,
const GEnergy& obsEng,
const GTime& obsTime,
const GObservation& obs) const
{
// Method is not implemented
std::string msg = "Spatial integration of sky model over the data space "
"is not implemented.";
throw GException::feature_not_implemented(G_NROI, msg);
// Return Npred
return (0.0);
}
/***********************************************************************//**
* @brief Return true energy boundaries for a specific observed energy
*
* @param[in] obsEnergy Observed Energy.
* @return True energy boundaries for given observed energy.
*
* @exception GException::feature_not_implemented
* Method is not implemented.
***************************************************************************/
GEbounds GLATResponse::ebounds(const GEnergy& obsEnergy) const
{
// Initialise an empty boundary object
GEbounds ebounds;
// Throw an exception
std::string msg = "Energy dispersion not implemented.";
throw GException::feature_not_implemented(G_EBOUNDS, msg);
// Return energy boundaries
return (ebounds);
}
/***********************************************************************//**
* @brief Load Fermi LAT response from calibration database
*
* @param[in] rspname Response name (name/name::front/name::back).
*
* @exception GException::rsp_invalid_type
* Invalid response type encountered.
*
* Loads the specified Fermi LAT response from the calibration database.
*
* @todo Add a more generic calibration database interface. For this we need
* first to develop a clear vision about how the calibration database
* is organized. Probably it is best to introduce a generic base class
* for the calibration database and each instrument implements then
* it's specific interface.
***************************************************************************/
void GLATResponse::load(const std::string& rspname)
{
// Save calibration database name
std::string caldb = m_caldb;
// Clear instance
clear();
// Restore calibration database name
m_caldb = caldb;
// Determine response types to be loaded
std::vector<std::string> array = gammalib::split(rspname, ":");
if (array.size() == 1) {
m_rspname = array[0];
m_has_front = true;
m_has_back = true;
}
else if (array.size() == 3) {
m_rspname = array[0];
if (gammalib::strip_whitespace(gammalib::tolower(array[2])) == "front") {
m_has_front = true;
}
else if (gammalib::strip_whitespace(gammalib::tolower(array[2])) == "back") {
m_has_back = true;
}
else {
throw GException::rsp_invalid_type(G_LOAD, array[2]);
}
}
else {
throw GException::rsp_invalid_type(G_LOAD, m_rspname);
}
// Set caldb access path
caldb += "/data/glast/lat/bcf/";
// Load front IRF if requested
if (m_has_front) {
std::string aeffname = caldb + "ea/aeff_" + m_rspname + "_front.fits";
std::string psfname = caldb + "psf/psf_" + m_rspname + "_front.fits";
std::string edispname = caldb + "edisp/edisp_" + m_rspname + "_front.fits";
GLATAeff* aeff = new GLATAeff(aeffname);
GLATPsf* psf = new GLATPsf(psfname);
GLATEdisp* edisp = new GLATEdisp(edispname);
m_aeff.push_back(aeff);
m_psf.push_back(psf);
m_edisp.push_back(edisp);
}
// Load back IRF if requested
if (m_has_back) {
std::string aeffname = caldb + "ea/aeff_" + m_rspname + "_back.fits";
std::string psfname = caldb + "psf/psf_" + m_rspname + "_back.fits";
std::string edispname = caldb + "edisp/edisp_" + m_rspname + "_back.fits";
GLATAeff* aeff = new GLATAeff(aeffname);
GLATPsf* psf = new GLATPsf(psfname);
GLATEdisp* edisp = new GLATEdisp(edispname);
m_aeff.push_back(aeff);
m_psf.push_back(psf);
m_edisp.push_back(edisp);
}
// Return
return;
}
/***********************************************************************//**
* @brief Save Fermi LAT response in calibration database
*
* @param[in] rspname Response name (name/name::front/name::back).
*
* Saves Fermi LAT response in a set of FITS files with names
* aeff_<rspname>_[front/back].fits,
* psf_<rspname>_[front/back].fits, and
* edisp_<rspname>_[front/back].fits.
*
* @todo Not yet implemented.
***************************************************************************/
void GLATResponse::save(const std::string& rspname) const
{
// Allocate FITS file
GFits file;
// Open FITS file
file.open(rspname, true);
// Save effective area
//aeff_append(file);
// Append PSF HDUs
//psf_append(file);
// Save energy dispersions
//edisp_append(file);
// Save efficiency factors
//eff_append(file);
// Save FITS file
file.save();
// Return
return;
}
/***********************************************************************//**
* @brief Return pointer on effective area
*
* @param[in] index Response index (starting from 0).
***************************************************************************/
GLATAeff* GLATResponse::aeff(const int& index) const
{
// Optionally check if the index is valid
#if defined(G_RANGE_CHECK)
if (index < 0 || index >= m_aeff.size()) {
throw GException::out_of_range(G_AEFF, index, 0, m_aeff.size()-1);
}
#endif
// Return pointer on effective area
return m_aeff[index];
}
/***********************************************************************//**
* @brief Return pointer on point spread function
*
* @param[in] index Response index (starting from 0).
***************************************************************************/
GLATPsf* GLATResponse::psf(const int& index) const
{
// Optionally check if the index is valid
#if defined(G_RANGE_CHECK)
if (index < 0 || index >= m_psf.size()) {
throw GException::out_of_range(G_PSF, index, 0, m_psf.size()-1);
}
#endif
// Return pointer on point spread function
return m_psf[index];
}
/***********************************************************************//**
* @brief Return pointer on energy dispersion
*
* @param[in] index Response index (starting from 0).
***************************************************************************/
GLATEdisp* GLATResponse::edisp(const int& index) const
{
// Optionally check if the index is valid
#if defined(G_RANGE_CHECK)
if (index < 0 || index >= m_edisp.size()) {
throw GException::out_of_range(G_EDISP, index, 0, m_edisp.size()-1);
}
#endif
// Return pointer on energy dispersion
return m_edisp[index];
}
/***********************************************************************//**
* @brief Print Fermi-LAT response information
*
* @param[in] chatter Chattiness (defaults to NORMAL).
* @return String containing response information.
***************************************************************************/
std::string GLATResponse::print(const GChatter& chatter) const
{
// Initialise result string
std::string result;
// Continue only if chatter is not silent
if (chatter != SILENT) {
// Append header
result.append("=== GLATResponse ===");
// Append information
result.append("\n"+gammalib::parformat("Calibration database")+m_caldb);
result.append("\n"+gammalib::parformat("Response name")+m_rspname);
result.append("\n"+gammalib::parformat("Section(s)"));
if (m_has_front && m_has_back) {
result.append("front & back");
}
else if (m_has_front) {
result.append("front");
}
else if (m_has_back) {
result.append("back");
}
else {
result.append("unknown");
}
if (chatter > TERSE) {
for (int i = 0; i < size(); ++i) {
result.append("\n"+m_aeff[i]->print(gammalib::reduce(chatter)));
result.append("\n"+m_psf[i]->print(gammalib::reduce(chatter)));
result.append("\n"+m_edisp[i]->print(gammalib::reduce(chatter)));
}
for (int i = 0; i < m_ptsrc.size(); ++i) {
result.append("\n"+m_ptsrc[i]->print(gammalib::reduce(chatter)));
}
}
} // endif: chatter was not silent
// Return result
return result;
}
/*==========================================================================
= =
= Private methods =
= =
==========================================================================*/
/***********************************************************************//**
* @brief Initialise class members
*
* @todo Do we need the handoff stuff there???
***************************************************************************/
void GLATResponse::init_members(void)
{
// Initialise members
m_caldb.clear();
m_rspname.clear();
m_has_front = false;
m_has_back = false;
m_force_mean = false;
m_aeff.clear();
m_psf.clear();
m_edisp.clear();
m_ptsrc.clear();
// By default use HANDOFF response database.
char* handoff = std::getenv("HANDOFF_IRF_DIR");
if (handoff != NULL) {
m_caldb.assign(handoff);
}
// Return
return;
}
/***********************************************************************//**
* @brief Copy class members
*
* @param[in] rsp Response.
***************************************************************************/
void GLATResponse::copy_members(const GLATResponse& rsp)
{
// Copy members
m_caldb = rsp.m_caldb;
m_rspname = rsp.m_rspname;
m_has_front = rsp.m_has_front;
m_has_back = rsp.m_has_back;
m_force_mean = rsp.m_force_mean;
// Clone Aeff
m_aeff.clear();
for (int i = 0; i < rsp.m_aeff.size(); ++i) {
m_aeff.push_back(rsp.m_aeff[i]->clone());
}
// Clone Psf
m_psf.clear();
for (int i = 0; i < rsp.m_psf.size(); ++i) {
m_psf.push_back(rsp.m_psf[i]->clone());
}
// Clone Edisp
m_edisp.clear();
for (int i = 0; i < rsp.m_edisp.size(); ++i) {
m_edisp.push_back(rsp.m_edisp[i]->clone());
}
// Clone point sources
m_ptsrc.clear();
for (int i = 0; i < rsp.m_ptsrc.size(); ++i) {
m_ptsrc.push_back(rsp.m_ptsrc[i]->clone());
}
// Return
return;
}
/***********************************************************************//**
* @brief Delete class members
***************************************************************************/
void GLATResponse::free_members(void)
{
// Free Aeff memory
for (int i = 0; i < m_aeff.size(); ++i) {
if (m_aeff[i] != NULL) delete m_aeff[i];
m_aeff[i] = NULL;
}
m_aeff.clear();
// Free Psf memory
for (int i = 0; i < m_psf.size(); ++i) {
if (m_psf[i] != NULL) delete m_psf[i];
m_psf[i] = NULL;
}
m_psf.clear();
// Free Edisp memory
for (int i = 0; i < m_edisp.size(); ++i) {
if (m_edisp[i] != NULL) delete m_edisp[i];
m_edisp[i] = NULL;
}
m_edisp.clear();
// Free point source memory
for (int i = 0; i < m_ptsrc.size(); ++i) {
if (m_ptsrc[i] != NULL) delete m_ptsrc[i];
m_ptsrc[i] = NULL;
}
m_ptsrc.clear();
// Return
return;
}