/***********************************************************************//**
* @brief Return instrument response to diffuse source
*
* @param[in] event Observed event.
* @param[in] source Source.
* @param[in] obs Observation.
* @return Instrument response to diffuse source.
*
* Returns the instrument response to a specified diffuse source.
*
* The method uses a pre-computation cache to store the instrument response
* for the spatial model component. The pre-computation cache is initialised
* if no cache has yet been allocated, or if at the beginning of a scan over
* the events, the model parameters have changed. The beginning of a scan is
* defined by an event bin index of 0.
***************************************************************************/
double GCTAResponseCube::irf_diffuse(const GEvent& event,
const GSource& source,
const GObservation& obs) const
{
// Initialise IRF
double irf = 0.0;
// Get pointer to CTA event bin
if (!event.is_bin()) {
std::string msg = "The current event is not a CTA event bin. "
"This method only works on binned CTA data. Please "
"make sure that a CTA observation containing binned "
"CTA data is provided.";
throw GException::invalid_value(G_IRF_DIFFUSE, msg);
}
const GCTAEventBin* bin = static_cast<const GCTAEventBin*>(&event);
// Get pointer to source cache. We first search the cache for a model
// with the source name. If no model was found we initialise a new
// cache entry for that model. Otherwise, we simply return the actual
// cache entry.
GCTACubeSourceDiffuse* cache(NULL);
int index = cache_index(source.name());
if (index == -1) {
// No cache entry was found, thus allocate and initialise a new one
cache = new GCTACubeSourceDiffuse;
cache->set(source.name(), *source.model(), obs);
m_cache.push_back(cache);
} // endif: no cache entry was found
else {
// Check that the cache entry is of the expected type
if (m_cache[index]->code() != GCTA_CUBE_SOURCE_DIFFUSE) {
std::string msg = "Cached model \""+source.name()+"\" is not "
"an extended source model. This method only "
"applies to extended source models.";
throw GException::invalid_value(G_IRF_DIFFUSE, msg);
}
cache = static_cast<GCTACubeSourceDiffuse*>(m_cache[index]);
} // endelse: there was a cache entry for this model
// Determine IRF value
irf = cache->irf(bin->ipix(), bin->ieng());
// Compile option: Check for NaN/Inf
#if defined(G_NAN_CHECK)
if (gammalib::is_notanumber(irf) || gammalib::is_infinite(irf)) {
std::cout << "*** ERROR: GCTAResponseCube::irf_diffuse:";
std::cout << " NaN/Inf encountered";
std::cout << " irf=" << irf;
std::cout << std::endl;
}
#endif
// Return IRF value
return irf;
}
/***********************************************************************//**
* @brief Return instrument response to elliptical source
*
* @param[in] event Observed event.
* @param[in] source Source.
* @param[in] obs Observation (not used).
* @return Instrument response to elliptical source.
*
* Returns the instrument response to a specified elliptical source.
***************************************************************************/
double GCTAResponseCube::irf_elliptical(const GEvent& event,
const GSource& source,
const GObservation& obs) const
{
// Initialise IRF
double irf = 0.0;
// Get pointer to CTA event bin
if (!event.is_bin()) {
std::string msg = "The current event is not a CTA event bin. "
"This method only works on binned CTA data. Please "
"make sure that a CTA observation containing binned "
"CTA data is provided.";
throw GException::invalid_value(G_IRF_RADIAL, msg);
}
const GCTAEventBin* bin = static_cast<const GCTAEventBin*>(&event);
// Get event attribute references
const GSkyDir& obsDir = bin->dir().dir();
const GEnergy& obsEng = bin->energy();
const GTime& obsTime = bin->time();
// Get pointer to elliptical model
const GModelSpatialElliptical* model = static_cast<const GModelSpatialElliptical*>(source.model());
// Compute angle between model centre and measured photon direction and
// position angle (radians)
double rho_obs = model->dir().dist(obsDir);
double posangle_obs = model->dir().posang(obsDir);
// Get livetime (in seconds)
double livetime = exposure().livetime();
// Continue only if livetime is >0 and if we're sufficiently close to
// the model centre to get a non-zero response
if ((livetime > 0.0) && (rho_obs <= model->theta_max()+psf().delta_max())) {
// Get exposure
irf = exposure()(obsDir, obsEng);
// Continue only if exposure is positive
if (irf > 0.0) {
// Recover effective area from exposure
irf /= livetime;
// Get PSF component
irf *= psf_elliptical(model, rho_obs, posangle_obs, obsDir, obsEng, obsTime);
// Apply deadtime correction
irf *= exposure().deadc();
} // endif: exposure was positive
} // endif: we were sufficiently close and livetime >0
// Compile option: Check for NaN/Inf
#if defined(G_NAN_CHECK)
if (gammalib::is_notanumber(irf) || gammalib::is_infinite(irf)) {
std::cout << "*** ERROR: GCTAResponseCube::irf_elliptical:";
std::cout << " NaN/Inf encountered";
std::cout << " irf=" << irf;
std::cout << std::endl;
}
#endif
// Return IRF value
return irf;
}
/***********************************************************************//**
* @brief Return instrument response to point source
*
* @param[in] event Observed event.
* @param[in] source Source.
* @param[in] obs Observation (not used).
* @return Instrument response to point source.
*
* Returns the instrument response to a specified point source.
***************************************************************************/
double GCTAResponseCube::irf_ptsrc(const GEvent& event,
const GSource& source,
const GObservation& obs) const
{
// Initialise IRF
double irf = 0.0;
// Get pointer to model source model
const GModelSpatialPointSource* ptsrc = static_cast<const GModelSpatialPointSource*>(source.model());
// Get point source direction
GSkyDir srcDir = ptsrc->dir();
// Get pointer on CTA event bin
if (!event.is_bin()) {
std::string msg = "The current event is not a CTA event bin. "
"This method only works on binned CTA data. Please "
"make sure that a CTA observation containing binned "
"CTA data is provided.";
throw GException::invalid_value(G_IRF_PTSRC, msg);
}
const GCTAEventBin* bin = static_cast<const GCTAEventBin*>(&event);
// Determine angular separation between true and measured photon
// direction in radians
double delta = bin->dir().dir().dist(srcDir);
// Get maximum angular separation for PSF (in radians)
double delta_max = psf().delta_max();
// Get livetime (in seconds)
double livetime = exposure().livetime();
// Continue only if livetime is >0 and if we're sufficiently close
// to the PSF
if ((livetime > 0.0) && (delta <= delta_max)) {
// Get exposure
irf = exposure()(srcDir, source.energy());
// Multiply-in PSF
if (irf > 0.0) {
// Recover effective area from exposure
irf /= livetime;
// Get PSF component
irf *= psf()(srcDir, delta, source.energy());
// Apply deadtime correction
irf *= exposure().deadc();
} // endif: exposure was non-zero
} // endif: we were sufficiently close to PSF and livetime >0
// Compile option: Check for NaN/Inf
#if defined(G_NAN_CHECK)
if (gammalib::is_notanumber(irf) || gammalib::is_infinite(irf)) {
std::cout << "*** ERROR: GCTAResponseCube::irf_ptsrc:";
std::cout << " NaN/Inf encountered";
std::cout << " irf=" << irf;
std::cout << std::endl;
}
#endif
// Return IRF value
return irf;
}