GCTACubeExposure.cpp
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/***************************************************************************
* GCTACubeExposure.cpp - CTA cube analysis exposure class *
* ----------------------------------------------------------------------- *
* copyright (C) 2014-2018 by Chia-Chun Lu *
* ----------------------------------------------------------------------- *
* *
* 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 GCTACubeExposure.cpp
* @brief CTA cube analysis exposure class implementation
* @author Chia-Chun Lu
*/
/* __ Includes ___________________________________________________________ */
#ifdef HAVE_CONFIG_H
#include <config.h>
#endif
#include "GTools.hpp"
#include "GMath.hpp"
#include "GLog.hpp"
#include "GObservations.hpp"
#include "GSkyRegionCircle.hpp"
#include "GCTALib.hpp"
/* __ Method name definitions ____________________________________________ */
#define G_FILL_CUBE "GCTACubeExposure::fill_cube(GCTAObservation&, GLog*)"
/* __ Macros _____________________________________________________________ */
/* __ Coding definitions _________________________________________________ */
/* __ Debug definitions __________________________________________________ */
/* __ Constants __________________________________________________________ */
/*==========================================================================
= =
= Constructors/destructors =
= =
==========================================================================*/
/***********************************************************************//**
* @brief Void constructor
***************************************************************************/
GCTACubeExposure::GCTACubeExposure(void)
{
// Initialise class members
init_members();
// Return
return;
}
/***********************************************************************//**
* @brief Copy constructor
*
* @param[in] cube Exposure cube.
***************************************************************************/
GCTACubeExposure::GCTACubeExposure(const GCTACubeExposure& cube)
{
// Initialise class members
init_members();
// Copy members
copy_members(cube);
// Return
return;
}
/***********************************************************************//**
* @brief File constructor
*
* @param[in] filename Exposure cube filename.
*
* Construct exposure cube by loading the information from an exposure cube
* file.
***************************************************************************/
GCTACubeExposure::GCTACubeExposure(const GFilename& filename)
{
// Initialise class members
init_members();
// Load exposure cube from file
load(filename);
// Return
return;
}
/***********************************************************************//**
* @brief Event cube constructor
*
* @param[in] cube Event cube.
*
* Construct exposure cube using the same binning and sky projection that is
* used for the event cube.
***************************************************************************/
GCTACubeExposure::GCTACubeExposure(const GCTAEventCube& cube)
{
// Initialise class members
init_members();
// Store energy boundaries
m_energies.set(cube.ebounds());
// Set GNodeArray used for interpolation
set_eng_axis();
// Set exposure cube to event cube
m_cube = cube.counts();
m_cube.nmaps(m_energies.size());
// Set all exposure cube pixels to zero as we want to have a clean map
// upon construction
m_cube = 0.0;
// Return
return;
}
/***********************************************************************//**
* @brief Exposure cube constructor
*
* @param[in] wcs World Coordinate System.
* @param[in] coords Coordinate System (CEL or GAL).
* @param[in] x X coordinate of sky map centre (deg).
* @param[in] y Y coordinate of sky map centre (deg).
* @param[in] dx Pixel size in x direction at centre (deg/pixel).
* @param[in] dy Pixel size in y direction at centre (deg/pixel).
* @param[in] nx Number of pixels in x direction.
* @param[in] ny Number of pixels in y direction.
* @param[in] energies Energies.
*
* Constructs an exposure cube by specifying the sky map grid and the
* energies.
***************************************************************************/
GCTACubeExposure::GCTACubeExposure(const std::string& wcs,
const std::string& coords,
const double& x,
const double& y,
const double& dx,
const double& dy,
const int& nx,
const int& ny,
const GEnergies& energies)
{
// Initialise class members
init_members();
// Store energies
m_energies = energies;
// Set GNodeArray used for interpolation
set_eng_axis();
// Create sky map
m_cube = GSkyMap(wcs, coords, x, y, dx, dy, nx, ny, m_energies.size());
// Return
return;
}
/***********************************************************************//**
* @brief Destructor
***************************************************************************/
GCTACubeExposure::~GCTACubeExposure(void)
{
// Free members
free_members();
// Return
return;
}
/*==========================================================================
= =
= Operators =
= =
==========================================================================*/
/***********************************************************************//**
* @brief Assignment operator
*
* @param[in] cube Exposure cube.
* @return Exposure cube.
***************************************************************************/
GCTACubeExposure& GCTACubeExposure::operator=(const GCTACubeExposure& cube)
{
// Execute only if object is not identical
if (this != &cube) {
// Free members
free_members();
// Initialise private members
init_members();
// Copy members
copy_members(cube);
} // endif: object was not identical
// Return this object
return *this;
}
/***********************************************************************//**
* @brief Return exposure (in units of cm2 s)
*
* @param[in] dir Coordinate of the true photon position.
* @param[in] energy Energy of the true photon.
* @return Exposure (in units of cm2 s)
***************************************************************************/
double GCTACubeExposure::operator()(const GSkyDir& dir, const GEnergy& energy) const
{
// Set indices and weighting factors for interpolation
update(energy.log10TeV());
// Perform interpolation
double exposure = m_wgt_left * m_cube(dir, m_inx_left) +
m_wgt_right * m_cube(dir, m_inx_right);
// Make sure that exposure does not become negative
if (exposure < 0.0) {
exposure = 0.0;
}
// Return exposure
return exposure;
}
/*==========================================================================
= =
= Public methods =
= =
==========================================================================*/
/***********************************************************************//**
* @brief Clear instance
*
* This method properly resets the object to an initial state.
***************************************************************************/
void GCTACubeExposure::clear(void)
{
// Free class members
free_members();
// Initialise members
init_members();
// Return
return;
}
/***********************************************************************//**
* @brief Clone exposure cube
*
* @return Deep copy of exposure cube instance.
***************************************************************************/
GCTACubeExposure* GCTACubeExposure::clone(void) const
{
return new GCTACubeExposure(*this);
}
/***********************************************************************//**
* @brief Set exposure cube for one CTA observation
*
* @param[in] obs CTA observation.
*
* Set the exposure cube for one CTA observation. The cube pixel values are
* computed as product of the effective area and the livetime.
***************************************************************************/
void GCTACubeExposure::set(const GCTAObservation& obs)
{
// Clear GTIs, reset livetime and exposure cube pixels
m_gti.clear();
m_livetime = 0.0;
m_cube = 0.0;
// Fill exposure cube
fill_cube(obs);
// Return
return;
}
/***********************************************************************//**
* @brief Fill exposure cube from observation container
*
* @param[in] obs Observation container.
* @param[in] log Pointer to logger.
*
* Set the exposure cube by summing the exposure for all CTA observations in
* an observation container. The cube pixel values are computed as the sum
* over the products of the effective area and the livetime.
***************************************************************************/
void GCTACubeExposure::fill(const GObservations& obs, GLog* log)
{
// Clear GTIs, reset livetime and exposure cube pixels
m_gti.clear();
m_livetime = 0.0;
m_cube = 0.0;
// Loop over all observations in container
for (int i = 0; i < obs.size(); ++i) {
// Get observation and continue only if it is a CTA observation
const GCTAObservation* cta = dynamic_cast<const GCTAObservation*>
(obs[i]);
// Skip observation if it's not CTA
if (cta == NULL) {
if (log != NULL) {
*log << "Skipping ";
*log << obs[i]->instrument();
*log << " observation ";
*log << "\"" << obs[i]->name() << "\"";
*log << " (id=" << obs[i]->id() << ")" << std::endl;
}
continue;
}
// Skip observation if we have a binned observation
if (cta->eventtype() == "CountsCube") {
if (log != NULL) {
*log << "Skipping binned ";
*log << cta->instrument();
*log << " observation ";
*log << "\"" << cta->name() << "\"";
*log << " (id=" << cta->id() << ")" << std::endl;
}
continue;
}
// Fill exposure cube
fill_cube(*cta, log);
} // endfor: looped over observations
// Return
return;
}
/***********************************************************************//**
* @brief Read exposure cube from FITS object
*
* @param[in] fits FITS object.
*
* Read the exposure cube from a FITS object.
***************************************************************************/
void GCTACubeExposure::read(const GFits& fits)
{
// Clear object
clear();
// Get HDUs
const GFitsImage& hdu_expcube = *fits.image("Primary");
const GFitsTable& hdu_energies = *fits.table(gammalib::extname_energies);
const GFitsTable& hdu_gti = *fits.table(gammalib::extname_gti);
// Read cube
m_cube.read(hdu_expcube);
// Read cube attributes
read_attributes(hdu_expcube);
// Read energies
m_energies.read(hdu_energies);
// Read GTIs
m_gti.read(hdu_gti);
// Set energy node array
set_eng_axis();
// Return
return;
}
/***********************************************************************//**
* @brief Write CTA exposure cube into FITS file.
*
* @param[in] fits FITS file.
*
* Writes the exposure cube image, the energies and the Good Time Intervals
* into the FITS file.
***************************************************************************/
void GCTACubeExposure::write(GFits& fits) const
{
// Write cube
m_cube.write(fits);
// Get last HDU and write attributes
GFitsHDU& hdu = *fits[fits.size()-1];
write_attributes(hdu);
// Write energies
m_energies.write(fits);
// Write GTIs
m_gti.write(fits);
// Return
return;
}
/***********************************************************************//**
* @brief Load exposure cube from FITS file
*
* @param[in] filename Performance table file name.
*
* Loads the exposure cube from a FITS file into the object.
***************************************************************************/
void GCTACubeExposure::load(const GFilename& filename)
{
// Put into OpenMP criticial zone
#pragma omp critical(GCTACubeExposure_load)
{
// Open FITS file
GFits fits(filename);
// Read PSF cube
read(fits);
// Close FITS file
fits.close();
} // end of OpenMP critical zone
// Store filename
m_filename = filename;
// Return
return;
}
/***********************************************************************//**
* @brief Save exposure cube into FITS file
*
* @param[in] filename Exposure cube FITS file name.
* @param[in] clobber Overwrite existing file?
*
* Save the exposure cube into a FITS file.
***************************************************************************/
void GCTACubeExposure::save(const GFilename& filename, const bool& clobber) const
{
// Put into OpenMP criticial zone
#pragma omp critical(GCTACubeExposure_save)
{
// Create FITS file
GFits fits;
// Write exposure cube
write(fits);
// Save FITS file
fits.saveto(filename, clobber);
// Close Edisp file
fits.close();
} // end of OpenMP critical zone
// Store filename
m_filename = filename;
// Return
return;
}
/***********************************************************************//**
* @brief Print exposure cube information
*
* @param[in] chatter Chattiness.
* @return String containing exposure cube information.
*
* @todo Add content
***************************************************************************/
std::string GCTACubeExposure::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("=== GCTACubeExposure ===");
// Append information
result.append("\n"+gammalib::parformat("Filename")+m_filename);
result.append("\n"+gammalib::parformat("Livetime"));
result.append(gammalib::str(m_livetime)+" sec");
// Append energies
if (m_energies.size() > 0) {
result.append("\n"+m_energies.print(chatter));
}
else {
result.append("\n"+gammalib::parformat("Energies") +
"not defined");
}
// Append GTIs
if (m_gti.size() > 0) {
result.append("\n"+m_gti.print(chatter));
}
else {
result.append("\n"+gammalib::parformat("Good Time Intervals") +
"not defined");
}
// Append skymap definition
result.append("\n"+m_cube.print(chatter));
} // endif: chatter was not silent
// Return result
return result;
}
/*==========================================================================
= =
= Private methods =
= =
==========================================================================*/
/***********************************************************************//**
* @brief Initialise class members
***************************************************************************/
void GCTACubeExposure::init_members(void)
{
// Initialise members
m_filename.clear();
m_cube.clear();
m_energies.clear();
m_elogmeans.clear();
m_gti.clear();
m_livetime = 0.0;
// Initialise cache
m_inx_left = 0;
m_inx_right = 0;
m_wgt_left = 0.0;
m_wgt_right = 0.0;
// Set CTA time reference for GTIs
m_gti.reference(GTimeReference(G_CTA_MJDREF, "s", "TT", "LOCAL"));
// Return
return;
}
/***********************************************************************//**
* @brief Copy class members
*
* @param[in] cube Exposure cube
***************************************************************************/
void GCTACubeExposure::copy_members(const GCTACubeExposure& cube)
{
// Copy members
m_filename = cube.m_filename;
m_cube = cube.m_cube;
m_energies = cube.m_energies;
m_elogmeans = cube.m_elogmeans;
m_gti = cube.m_gti;
m_livetime = cube.m_livetime;
// Copy cache
m_inx_left = cube.m_inx_left;
m_inx_right = cube.m_inx_right;
m_wgt_left = cube.m_wgt_left;
m_wgt_right = cube.m_wgt_right;
// Return
return;
}
/***********************************************************************//**
* @brief Delete class members
***************************************************************************/
void GCTACubeExposure::free_members(void)
{
// Return
return;
}
/***********************************************************************//**
* @brief Fill exposure cube for one observation
*
* @param[in] obs Observation.
* @param[in] log Pointer to logger.
*
* @exception GException::invalid_value
* No RoI or response found in CTA observation.
*
* Fill the exposure cube from one CTA observations. The exposure cube pixel
* values are computed as the product of the effective area and the livetime.
***************************************************************************/
void GCTACubeExposure::fill_cube(const GCTAObservation& obs, GLog* log)
{
// Set energy margin
static const GEnergy margin(1.0, "MeV");
// Only continue if we have an event list
if (obs.eventtype() == "EventList") {
// Extract pointing direction, energy boundaries and ROI from
// observation
GSkyDir pnt = obs.pointing().dir();
GEbounds obs_ebounds = obs.ebounds();
GCTARoi roi = obs.roi();
// Check for RoI sanity
if (!roi.is_valid()) {
std::string msg = "No RoI information found in "+obs.instrument()+
" observation \""+obs.name()+"\". Run ctselect "
"to specify an RoI for this observation.";
throw GException::invalid_value(G_FILL_CUBE, msg);
}
// Convert RoI into a circular region for overlap checking
GSkyRegionCircle roi_reg(roi.centre().dir(), roi.radius());
// Extract response from observation
const GCTAResponseIrf* rsp = dynamic_cast<const GCTAResponseIrf*>
(obs.response());
if (rsp == NULL) {
std::string msg = "No valid instrument response function found in "+
obs.instrument()+" observation \""+obs.name()+
"\". Please specify the instrument response "
"function for this observation.";
throw GException::invalid_value(G_FILL_CUBE, msg);
}
// Skip observation if livetime is zero
if (obs.livetime() == 0.0) {
if (log != NULL) {
*log << "Skipping unbinned ";
*log << obs.instrument();
*log << " observation ";
*log << "\"" << obs.name() << "\"";
*log << " (id=" << obs.id() << ") due to zero livetime";
*log << std::endl;
}
}
// Skip observation if observation is outside the bounds of the cube
else if (!m_cube.overlaps(roi_reg)) {
if (log != NULL) {
*log << "Skipping unbinned ";
*log << obs.instrument();
*log << " observation ";
*log << "\"" << obs.name() << "\"";
*log << " (id=" << obs.id() << ") since it does not overlap ";
*log << "with the exposure cube.";
*log << std::endl;
}
}
// ... otherwise continue
else {
// Announce observation usage
if (log != NULL) {
*log << "Including ";
*log << obs.instrument();
*log << " observation \"" << obs.name();
*log << "\" (id=" << obs.id() << ")";
*log << " in exposure cube computation." << std::endl;
}
// Loop over all pixels in sky map
for (int pixel = 0; pixel < m_cube.npix(); ++pixel) {
// Get pixel sky direction
GSkyDir dir = m_cube.inx2dir(pixel);
// Skip pixel if it is outside the RoI
if (roi.centre().dir().dist_deg(dir) > roi.radius()) {
continue;
}
// Compute theta angle with respect to pointing direction in
// radians
double theta = pnt.dist(dir);
// Loop over all exposure cube energies
for (int iebin = 0; iebin < m_energies.size(); ++iebin){
// Skip exposure cube energy if the energy is outside the
// observation energy. The exposure cube energies are true
// energies while the observation energy boundaries are
// reconstructed energies, hence this is only an
// approximation, but probably the only we can really do.
// We allow here for a small margin in case of rounding
// errors in the energy boundaries.
if (!(obs_ebounds.contains(m_energies[iebin]) ||
obs_ebounds.contains(m_energies[iebin]-margin) ||
obs_ebounds.contains(m_energies[iebin]+margin))) {
continue;
}
// Get logE/TeV
double logE = m_energies[iebin].log10TeV();
// Add to exposure cube (effective area * livetime)
m_cube(pixel, iebin) += rsp->aeff(theta, 0.0, 0.0, 0.0, logE) *
obs.livetime();
} // endfor: looped over energy bins
} // endfor: looped over all pixels
// Append GTIs and increment livetime
m_gti.extend(obs.gti());
m_livetime += obs.livetime();
} // endelse: livetime was not zero
} // endif: observation contained an event list
// Return
return;
}
/***********************************************************************//**
* @brief Update 1D cache
*
* @param[in] logE Log10 energy in TeV.
*
* Updates the 1D interpolation cache. The interpolation cache is composed
* of two indices and weights that define 2 data values of the 2D skymap
* that are used for linear interpolation.
*
* @todo Write down formula
***************************************************************************/
void GCTACubeExposure::update(const double& logE) const
{
// Set value for node array
m_elogmeans.set_value(logE);
// Set indices and weighting factors for interpolation
m_inx_left = m_elogmeans.inx_left();
m_inx_right = m_elogmeans.inx_right();
m_wgt_left = m_elogmeans.wgt_left();
m_wgt_right = m_elogmeans.wgt_right();
// Return
return;
}
/***********************************************************************//**
* @brief Set nodes for a logarithmic (base 10) energy axis
*
* Set axis nodes so that each node is the logarithm of the energy values.
***************************************************************************/
void GCTACubeExposure::set_eng_axis(void)
{
// Get number of bins
int bins = m_energies.size();
// Clear node array
m_elogmeans.clear();
// Compute nodes
for (int i = 0; i < bins; ++i) {
// Get logE/TeV
m_elogmeans.append(m_energies[i].log10TeV());
} // endfor: looped over energy bins
// Return
return;
}
/***********************************************************************//**
* @brief Read exposure attributes
*
* @param[in] hdu FITS HDU.
*
* Reads CTA exposure attributes from the HDU.
***************************************************************************/
void GCTACubeExposure::read_attributes(const GFitsHDU& hdu)
{
// Read mandatory attributes
m_livetime = (hdu.has_card("LIVETIME")) ? hdu.real("LIVETIME") : 0.0;
// Return
return;
}
/***********************************************************************//**
* @brief Write attributes to exposure extension
*
* @param[in] hdu FITS HDU.
***************************************************************************/
void GCTACubeExposure::write_attributes(GFitsHDU& hdu) const
{
// Compute some attributes
double tstart = m_gti.tstart().convert(m_gti.reference());
double tstop = m_gti.tstop().convert(m_gti.reference());
double telapse = m_gti.telapse();
double ontime = m_gti.ontime();
double deadc = (ontime > 0.0 && m_livetime > 0.0) ?
m_livetime / ontime : 1.0;
std::string utc_obs = m_gti.tstart().utc();
std::string utc_end = m_gti.tstop().utc();
std::string date_obs = utc_obs.substr(0, 10);
std::string time_obs = utc_obs.substr(11, 8);
std::string date_end = utc_end.substr(0, 10);
std::string time_end = utc_end.substr(11, 8);
// Set observation information
hdu.card("CREATOR", "GammaLib", "Program which created the file");
hdu.card("TELESCOP", "unknown", "Telescope");
hdu.card("OBS_ID", "unknown", "Observation identifier");
hdu.card("DATE-OBS", date_obs, "Observation start date");
hdu.card("TIME-OBS", time_obs, "Observation start time");
hdu.card("DATE-END", date_end, "Observation end date");
hdu.card("TIME-END", time_end, "Observation end time");
// Set observation time information
hdu.card("TSTART", tstart, "[s] Mission time of start of observation");
hdu.card("TSTOP", tstop, "[s] Mission time of end of observation");
m_gti.reference().write(hdu);
hdu.card("TELAPSE", telapse, "[s] Mission elapsed time");
hdu.card("ONTIME", ontime, "[s] Total good time including deadtime");
hdu.card("LIVETIME", m_livetime, "[s] Total livetime");
hdu.card("DEADC", deadc, "Deadtime correction factor");
hdu.card("TIMEDEL", 1.0, "Time resolution");
// Return
return;
}