GResponse.cpp

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/***************************************************************************
 *                GResponse.cpp - Abstract response base class             *
 * ----------------------------------------------------------------------- *
 *  copyright (C) 2008-2025 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 GResponse.hpp
 * @brief Abstract response base class interface definition
 * @author Juergen Knoedlseder
 */
 
/* __ Includes ___________________________________________________________ */
#ifdef HAVE_CONFIG_H
#include <config.h>
#endif
#include <string>
#include <unistd.h>           // access() function
#include "GException.hpp"
#include "GTools.hpp"
#include "GMath.hpp"
#include "GVector.hpp"
#include "GMatrix.hpp"
#include "GMatrixSparse.hpp"
#include "GIntegral.hpp"
#include "GIntegrals.hpp"
#include "GResponse.hpp"
#include "GEvent.hpp"
#include "GPhoton.hpp"
#include "GEnergy.hpp"
#include "GTime.hpp"
#include "GSource.hpp"
#include "GEbounds.hpp"
#include "GObservation.hpp"
#include "GSkyMap.hpp"
#include "GModelSky.hpp"
#include "GModelSpatialPointSource.hpp"
#include "GModelSpatialRadial.hpp"
#include "GModelSpatialElliptical.hpp"
#include "GModelSpatialDiffuse.hpp"
#include "GModelSpatialDiffuseMap.hpp"
#include "GModelSpatialDiffuseCube.hpp"
#include "GModelSpatialComposite.hpp"
#include "GModelSpectralGauss.hpp"
 
/* __ Method name definitions ____________________________________________ */
#define G_CONVOLVE          "GResponse::convolve(GModelSky&, GObservation&, "\
                                                            "GMatrixSparse*)"
#define G_IRF_RADIAL               "GResponse::irf_radial(GEvent&, GSource&,"\
                                                            " GObservation&)"
#define G_IRF_ELLIPTICAL       "GResponse::irf_elliptical(GEvent&, GSource&,"\
                                                            " GObservation&)"
#define G_IRF_DIFFUSE             "GResponse::irf_diffuse(GEvent&, GSource&,"\
                                                            " GObservation&)"
 
/* __ Macros _____________________________________________________________ */
 
/* __ Coding definitions _________________________________________________ */
 
/* __ Debug definitions __________________________________________________ */
 
 
/*==========================================================================
 =                                                                         =
 =                         Constructors/destructors                        =
 =                                                                         =
 ==========================================================================*/
 
/***********************************************************************//**
 * @brief Void constructor
 ***************************************************************************/
GResponse::GResponse(void)
{
    // Initialise class members for clean destruction
    init_members();
 
    // Return
    return;
}
 
 
/***********************************************************************//**
 * @brief Copy constructor
 *
 * @param[in] rsp Response.
 ***************************************************************************/
GResponse::GResponse(const GResponse& rsp)
{
    // Initialise class members for clean destruction
    init_members();
 
    // Copy members
    copy_members(rsp);
 
    // Return
    return;
}
 
 
/***********************************************************************//**
 * @brief Destructor
 ***************************************************************************/
GResponse::~GResponse(void)
{
    // Free members
    free_members();
 
    // Return
    return;
}
 
 
/*==========================================================================
 =                                                                         =
 =                               Operators                                 =
 =                                                                         =
 ==========================================================================*/
 
/***********************************************************************//**
 * @brief Assignment operator
 *
 * @param[in] rsp Response.
 * @return Response.
 ***************************************************************************/
GResponse& GResponse::operator=(const GResponse& rsp)
{
    // Execute only if object is not identical
    if (this != &rsp) {
 
        // Free members
        free_members();
 
        // Initialise private members for clean destruction
        init_members();
 
        // Copy members
        copy_members(rsp);
 
    } // endif: object was not identical
 
    // Return this object
    return *this;
}
 
 
/*==========================================================================
 =                                                                         =
 =                             Public methods                              =
 =                                                                         =
 ==========================================================================*/
 
/***********************************************************************//**
 * @brief Convolve sky model with the instrument response
 *
 * @param[in] model Sky model.
 * @param[in] event Event.
 * @param[in] obs Observation.
 * @param[in] grad Should model gradients be computed?
 * @return Event probability.
 *
 * Computes the event probability
 *
 * \f[
 *    P(p',E',t') = \int \int \int
 *                  S(p,E,t) \times R(p',E',t'|p,E,t) \, dp \, dE \, dt
 * \f]
 *
 * without taking into account any time dispersion. Energy dispersion is
 * correctly handled by this method. If time dispersion is indeed needed,
 * an instrument specific method needs to be provided.
 ***************************************************************************/
double GResponse::convolve(const GModelSky&    model,
                           const GEvent&       event,
                           const GObservation& obs,
                           const bool&         grad) const
{
    // Set number of iterations for Romberg integration.
    static const int iter = 6;
 
    // Initialise result
    double prob = 0.0;
 
    // Continue only if the model has a spatial component
    if (model.spatial() != NULL) {
 
        // Get source time (no dispersion)
        GTime srcTime = event.time();
 
        // Case A: Integration
        if (use_edisp()) {
 
            // Retrieve true energy boundaries
            GEbounds ebounds = this->ebounds(event.energy());
 
            // Retrieve model energy boundaries
            GEbounds ebounds_model = this->ebounds_model(model);
 
            // Determine size of result array
            int size = size_edisp_vector(model, obs, grad);
 
            // Initialise vector array
            GVector array(size);
 
            // Loop over all boundaries
            for (int i = 0; i < ebounds.size(); ++i) {
 
                // Get true energy boundaries in MeV
                double etrue_min = ebounds.emin(i).MeV();
                double etrue_max = ebounds.emax(i).MeV();
 
                // Limit energy boundaries
                if (ebounds_model.size() > 0) {
                    if (ebounds_model.emin(0).MeV() > etrue_min) {
                        etrue_min = ebounds_model.emin(0).MeV();
                    }
                    if (ebounds_model.emax(0).MeV() < etrue_max) {
                        etrue_max = ebounds_model.emax(0).MeV();
                    }
                }
 
                // Continue only if valid
                if (etrue_max > etrue_min) {
 
                    // Setup integration function
                    edisp_kerns integrand(this, &obs, &model, &event, srcTime, grad);
                    GIntegrals  integral(&integrand);
 
                    // Set number of iterations
                    integral.fixed_iter(iter);
 
                    // Do Romberg integration
                    array += integral.romberg(etrue_min, etrue_max);
 
                } // endif: interval was valid
 
            } // endfor: looped over intervals
 
            // Initialise array index
            int index = 0;
 
            // Get probability
            prob = array[index++];
 
            // Set gradients
            if (grad) {
 
                // Set spectral gradients
                if (model.spectral() != NULL) {
                    for (int i = 0; i < model.spectral()->size(); ++i) {
                        GModelPar& par = (*(model.spectral()))[i];
                        if (par.is_free() && par.has_grad()) {
                            par.factor_gradient(array[index++]);
                        }
                    }
                }
 
                // Set temporal gradients
                if (model.temporal() != NULL) {
                    for (int i = 0; i < model.temporal()->size(); ++i) {
                        GModelPar& par = (*(model.temporal()))[i];
                        if (par.is_free() && par.has_grad()) {
                            par.factor_gradient(array[index++]);
                        }
                    }
                }
 
                // Optionally set scale gradient for instrument
                if (model.has_scales()) {
                    for (int i = 0; i < model.scales(); ++i) {
                        const GModelPar& par = model.scale(i);
                        if (par.name() == obs.instrument()) {
                            if (par.is_free() && par.has_grad()) {
                                par.factor_gradient(array[index++]);
                            }
                        }
                    }
                }
 
            } // endif: set gradients
 
        } // endif: Case A
 
        // Case B: No integration (assume no energy dispersion)
        else {
 
            // Get source energy (no dispersion)
            GEnergy srcEng  = event.energy();
 
            // Evaluate probability
            prob = eval_prob(model, event, srcEng, srcTime, obs, grad);
 
        } // endelse: Case B
 
        // Compile option: Check for NaN/Inf
        #if defined(G_NAN_CHECK)
        if (gammalib::is_notanumber(prob) || gammalib::is_infinite(prob)) {
            std::cout << "*** ERROR: GResponse::convolve:";
            std::cout << " NaN/Inf encountered";
            std::cout << " (prob=" << prob;
            std::cout << ", event=" << event;
            std::cout << ", srcTime=" << srcTime;
            std::cout << ")" << std::endl;
        }
        #endif
 
    } // endif: spatial component valid
 
    // Return probability
    return prob;
}
 
 
/***********************************************************************//**
 * @brief Convolve sky model with the instrument response
 *
 * @param[in] model Sky model.
 * @param[in] obs Observation.
 * @param[out] gradients Pointer to matrix of gradients.
 * @return Vector of event probabilities.
 *
 * Computes the event probability
 *
 * \f[
 *    P(p',E',t') = \int \int \int
 *                  S(p,E,t) \times R(p',E',t'|p,E,t) \, dp \, dE \, dt
 * \f]
 *
 * without taking into account any time dispersion. Energy dispersion is
 * correctly handled by this method. If time dispersion is indeed needed,
 * an instrument specific method needs to be provided.
 ***************************************************************************/
GVector GResponse::convolve(const GModelSky&    model,
                            const GObservation& obs,
                            GMatrixSparse*      gradients) const
{
    // Set number of iterations for Romberg integration.
    static const int iter = 6;
 
    // Get number of model parameters and number of events
    int npars   = model.size();
    int nevents = obs.events()->size();
 
    // Initialise gradients flag
    bool grad = (gradients != NULL);
 
    // Check matrix consistency
    if (grad) {
 
        // Check number of columns
        int ncolumns = (nevents > 0) ? npars : 0;
        if (gradients->columns() != ncolumns) {
            std::string msg = "Number of "+gammalib::str(gradients->columns())+" "
                              "columns in gradient matrix differs from expected "
                              "number of "+gammalib::str(ncolumns)+". Please "
                              "specify compatible arguments.";
            throw GException::invalid_argument(G_CONVOLVE, msg);
        }
 
        // Check number of rows
        int nrows = (ncolumns > 0) ? nevents : 0;
        if (gradients->rows() != nrows) {
            std::string msg = "Number of "+gammalib::str(gradients->rows())+" "
                              "rows in gradient matrix differs from expected "
                              "number of "+gammalib::str(nrows)+". Please "
                              "specify compatible arguments.";
            throw GException::invalid_argument(G_CONVOLVE, msg);
        }
 
    } // endif: gadient was requested
 
    // Initialise result
    GVector probs(nevents);
 
    // Continue only if the model has a spatial component
    if (model.spatial() != NULL) {
 
        // Case A: Integration
        if (use_edisp()) {
 
            // Initialise temporary vectors to hold gradients
            GVector* tmp_gradients = NULL;
            if (grad) {
                tmp_gradients = new GVector[npars];
                for (int i = 0; i < npars; ++i) {
                    tmp_gradients[i] = GVector(nevents);
                }
            }
 
            // Determine size of result array
            int size = size_edisp_vector(model, obs, grad);
 
            // Get model energy boundaries
            GEbounds ebounds_model = this->ebounds_model(model);
 
            // Loop over events
            for (int k = 0; k < nevents; ++k) {
 
                // Get reference to event
                const GEvent& event = *((*obs.events())[k]);
 
                // Get source time (no dispersion)
                GTime srcTime = event.time();
 
                // Retrieve true energy boundaries
                GEbounds ebounds = this->ebounds(event.energy());
 
                // Initialise vector array
                GVector array(size);
 
                // Loop over all boundaries
                for (int i = 0; i < ebounds.size(); ++i) {
 
                    // Get true energy boundaries in MeV
                    double etrue_min = ebounds.emin(i).MeV();
                    double etrue_max = ebounds.emax(i).MeV();
 
                    // Limit energy boundaries
                    if (ebounds_model.size() > 0) {
                        if (ebounds_model.emin(0).MeV() > etrue_min) {
                            etrue_min = ebounds_model.emin(0).MeV();
                        }
                        if (ebounds_model.emax(0).MeV() < etrue_max) {
                            etrue_max = ebounds_model.emax(0).MeV();
                        }
                    }
 
                    // Continue only if valid
                    if (etrue_max > etrue_min) {
 
                        // Setup integration function
                        edisp_kerns integrand(this, &obs, &model, &event, srcTime, grad);
                        GIntegrals  integral(&integrand);
 
                        // Set number of iterations
                        integral.fixed_iter(iter);
 
                        // Do Romberg integration
                        array += integral.romberg(etrue_min, etrue_max);
 
                    } // endif: interval was valid
 
                } // endfor: looped over intervals
 
                // Initialise array index
                int index = 0;
 
                // Get probability
                probs[k] = array[index++];
 
                // Set gradients
                if (grad) {
 
                    // Get number of spatial, spectral and temporal parameters
                    int n_spat = model.spatial()->size();
                    int n_spec = model.spectral()->size();
                    int n_temp = model.temporal()->size();
 
                    // Set spectral gradients
                    if (model.spectral() != NULL) {
                        int offset = n_spat;
                        for (int i = 0; i < n_spec; ++i) {
                            const GModelPar& par = (*(model.spectral()))[i];
                            if (par.is_free() && par.has_grad()) {
                                tmp_gradients[offset+i][k] = array[index++];
                            }
                        }
                    }
 
                    // Set temporal gradients
                    if (model.temporal() != NULL) {
                        int offset = n_spat + n_spec;
                        for (int i = 0; i < n_temp; ++i) {
                            const GModelPar& par = (*(model.temporal()))[i];
                            if (par.is_free() && par.has_grad()) {
                                tmp_gradients[offset+i][k] = array[index++];
                            }
                        }
                    }
 
                    // Optionally set scale gradient for instrument
                    if (model.has_scales()) {
                        int offset = n_spat + n_spec + n_temp;
                        for (int i = 0; i < model.scales(); ++i) {
                            const GModelPar& par = model.scale(i);
                            if (par.name() == obs.instrument()) {
                                if (par.is_free() && par.has_grad()) {
                                    tmp_gradients[offset+i][k] = array[index++];
                                }
                            }
                        }
                    }
 
                } // endif: set gradients
 
                // Compile option: Check for NaN/Inf
                #if defined(G_NAN_CHECK)
                if (gammalib::is_notanumber(probs[k]) || gammalib::is_infinite(probs[k])) {
                    std::cout << "*** ERROR: GResponse::convolve:";
                    std::cout << " NaN/Inf encountered";
                    std::cout << " (probs[" << k << "]=" << probs[k];
                    std::cout << ", event=" << event;
                    std::cout << ", srcTime=" << srcTime;
                    std::cout << ")" << std::endl;
                }
                #endif
 
            } // endfor: looped over events
 
            // Post-process gradients
            if (grad) {
 
                // Fill gradients into matrix
                for (int i = 0; i < npars; ++i) {
                    gradients->column(i, tmp_gradients[i]);
                }
 
                // Delete temporal gradients
                delete [] tmp_gradients;
 
            } // endif: post-processed gradients
 
        } // endif: Case A
 
        // Case B: No integration (assume no energy dispersion)
        else {
 
            // Evaluate probability
            probs = eval_probs(model, obs, gradients);
 
        } // endelse: Case B
 
    } // endif: spatial component valid
 
    // Return probabilities
    return probs;
}
 
 
/***********************************************************************//**
 * @brief Return instrument response integrated over the spatial model
 *
 * @param[in] event Event.
 * @param[in] source Source.
 * @param[in] obs Observation.
 * @return Instrument response to a spatial model.
 *
 * Returns the instrument response for a given event, source and observation
 * integrated over the spatial model component. The method computes
 *
 * \f[
 *    {\tt irf}(p', E', t') = \int_p M_{\rm S}(p | E, t) \,
 *                                   R(p', E', t' | p, E, t) \, d\,p
 * \f]
 *
 * where
 * * \f$M_{\rm S}(p | E, t)\f$ is the spatial model component,
 * * \f$R(p', E', t' | p, E, t)\f$ is the Instrument Response Function (IRF),
 * * \f$p'\f$ is the measured instrument direction,
 * * \f$E'\f$ is the measured or reconstructed energy,
 * * \f$t'\f$ is the measured arrival time,
 * * \f$p\f$ is the true photon arrival direction,
 * * \f$E\f$ is the true photon energy, and
 * * \f$t\f$ is the true trigger time.
 *
 * The integration is done over all relevant true sky directions \f$p\f$.
 *
 * Depending on the type of the source model the method branches to the
 * following methods to perform the actual computations
 *
 * * irf_ptsrc() - for the handling of a point source
 * * irf_radial() - for radial models
 * * irf_elliptical() - for elliptical models
 * * irf_diffuse() - for diffuse models
 * * irf_composite() - for composite models
 *
 * The method implements a caching mechanism for spatial models that have all
 * parameters fixed. For those models the instrument response for a given
 * event and observation is only computed once and then stored in an internal
 * cache from which it is fetched back in case that the method is called
 * again for the same event and observation.
 ***************************************************************************/
double GResponse::irf_spatial(const GEvent&       event,
                              const GSource&      source,
                              const GObservation& obs) const
{
    // Initialise IRF value
    double irf = 0.0;
 
    // Set IRF value attributes
    std::string     name  = obs.id() + ":" + source.name();
    const GInstDir& dir   = event.dir();
    const GEnergy&  ereco = event.energy();
    const GEnergy&  etrue = source.energy();
 
    // Signal if spatial model has free parameters
    bool has_free_pars = source.model()->has_free_pars();
 
    // If the spatial model component has free parameters, or the response
    // cache should not be used, or the cache does not contain the requested
    // IRF value then compute the IRF value for the spatial model.
    if (has_free_pars    ||
        !m_use_irf_cache ||
        !m_irf_cache.contains(name, dir, ereco, etrue, &irf)) {
 
        // Compute IRF for spatial model
        switch (source.model()->code()) {
            case GMODEL_SPATIAL_POINT_SOURCE:
                irf = irf_ptsrc(event, source, obs);
                break;
            case GMODEL_SPATIAL_RADIAL:
                irf = irf_radial(event, source, obs);
                break;
            case GMODEL_SPATIAL_ELLIPTICAL:
                irf = irf_elliptical(event, source, obs);
                break;
            case GMODEL_SPATIAL_DIFFUSE:
                irf = irf_diffuse(event, source, obs);
                break;
            case GMODEL_SPATIAL_COMPOSITE:
                irf = irf_composite(event, source, obs);
                break;
            default:
                break;
        }
 
    } // endif: computed spatial model
 
    // If the spatial model has no free parameters and the response cache
    // should be used then put the IRF value in the response cache.
    if (!has_free_pars && m_use_irf_cache) {
        m_irf_cache.set(name, dir, ereco, etrue, irf);
    }
 
    // Return IRF value
    return irf;
}
 
 
/***********************************************************************//**
 * @brief Return instrument response vector integrated over the spatial model
 *
 * @param[in] model Sky model.
 * @param[in] obs Observation.
 * @param[in] gradients Gradients matrix.
 * @return Instrument response vector to a spatial model.
 *
 * Returns the instrument response to a sky model integrated over the spatial
 * model component for all events in a given observation. The method computes
 *
 * \f[
 *    {\tt irf}(p', E', t') = \int_p M_{\rm S}(p | E, t) \,
 *                                   R(p', E', t' | p, E, t) \, d\,p
 * \f]
 *
 * where
 * * \f$M_{\rm S}(p | E, t)\f$ is the spatial model component,
 * * \f$R(p', E', t' | p, E, t)\f$ is the Instrument Response Function (IRF),
 * * \f$p'\f$ is the measured instrument direction,
 * * \f$E'\f$ is the measured or reconstructed energy,
 * * \f$t'\f$ is the measured arrival time,
 * * \f$p\f$ is the true photon arrival direction,
 * * \f$E\f$ is the true photon energy, and
 * * \f$t\f$ is the true trigger time.
 *
 * The integration is done over all relevant true sky directions \f$p\f$.
 *
 * Depending on the type of the source model the method branches to the
 * following methods to perform the actual computations
 *
 * * irf_ptsrc() - for the handling of a point source
 * * irf_radial() - for radial models
 * * irf_elliptical() - for elliptical models
 * * irf_diffuse() - for diffuse models
 * * irf_composite() - for composite models
 *
 * The method implements a caching mechanism for spatial models that have all
 * parameters fixed. For those models the instrument response for a given
 * event and observation is only computed once and then stored in an internal
 * cache from which it is fetched back in case that the method is called
 * again for the same event and observation.
 ***************************************************************************/
GVector GResponse::irf_spatial(const GModelSky&    model,
                               const GObservation& obs,
                               GMatrix*            gradients) const
{
    // Get number of model parameters and number of events
    int npars   = model.size();
    int nevents = obs.events()->size();
 
    // Initialise result
    GVector irfs(nevents);
 
    // Continue only if model has a spatial component
    if (model.spatial() != NULL) {
 
        // Set IRF cache identifier
        std::string cache_id = obs.id() + ":" + model.name();
 
        // Signal if spatial model has free parameters
        bool has_free_pars = model.spatial()->has_free_pars();
 
        // If the spatial model component has free parameters, or the response
        // cache should not be used, or the cache does not contain the requested
        // IRF value then compute the IRF value for the spatial model.
        if (has_free_pars    ||
            !m_use_irf_cache ||
            !m_irf_vector_cache.contains(cache_id, &irfs)) {
 
            // Compute IRF for spatial model
            switch (model.spatial()->code()) {
                case GMODEL_SPATIAL_POINT_SOURCE:
                    irfs = irf_ptsrc(model, obs, gradients);
                    break;
                case GMODEL_SPATIAL_RADIAL:
                    irfs = irf_radial(model, obs, gradients);
                    break;
                case GMODEL_SPATIAL_ELLIPTICAL:
                    irfs = irf_elliptical(model, obs, gradients);
                    break;
                case GMODEL_SPATIAL_DIFFUSE:
                    irfs = irf_diffuse(model, obs, gradients);
                    break;
                case GMODEL_SPATIAL_COMPOSITE:
                    irfs = irf_composite(model, obs, gradients);
                    break;
                default:
                    break;
            }
 
            // If the spatial model has no free parameters and the response cache
            // should be used then put the IRF value in the response cache.
            if (!has_free_pars && m_use_irf_cache) {
                m_irf_vector_cache.set(cache_id, irfs);
            }
 
        } // endif: computed spatial model
 
    } // endif: model had spatial component
 
    // Return IRF values
    return irfs;
}
 
 
/***********************************************************************//**
 * @brief Remove response cache for specific observation and model
 *
 * @param[in] cache_id Response cache identifier.
 *
 * Remove response cache with @p cache_id. The response cache identifier
 * @p cache_id is formed by a combination of observation identifier and
 * model name using
 *
 *     cache_id = obs.id() + ":" + model.name()
 *
 * Please make sure to respect the same format for the specified @p cache_id
 * parameter.
 ***************************************************************************/
void GResponse::remove_response_cache(const std::string& cache_id)
{
    // Remove cache_id from response caches
    m_irf_cache.remove(cache_id);
    m_nroi_cache.remove(cache_id);
    m_irf_vector_cache.remove(cache_id);
 
    // Return
    return;
}
 
 
/*==========================================================================
 =                                                                         =
 =                            Protected methods                            =
 =                                                                         =
 ==========================================================================*/
 
/***********************************************************************//**
 * @brief Initialise class members
 ***************************************************************************/
void GResponse::init_members(void)
{
    // Initialize members
    m_use_irf_cache             = true;   //!< Switched on by default
    m_use_nroi_cache            = true;   //!< Switched on by default
    m_irf_radial_iter_theta     = 6;
    m_irf_radial_iter_phi       = 6;
    m_irf_elliptical_iter_theta = 6;
    m_irf_elliptical_iter_phi   = 6;
    m_irf_diffuse_resolution    = 0.1;    //!< Angular resolution (deg)
 
    // Clear cache
    m_irf_cache.clear();
    m_nroi_cache.clear();
    m_irf_vector_cache.clear();
 
    // Return
    return;
}
 
 
/***********************************************************************//**
 * @brief Copy class members
 *
 * @param[in] rsp Response.
 ***************************************************************************/
void GResponse::copy_members(const GResponse& rsp)
{
    // Copy members
    m_use_irf_cache             = rsp.m_use_irf_cache;
    m_use_nroi_cache            = rsp.m_use_nroi_cache;
    m_irf_radial_iter_theta     = rsp.m_irf_radial_iter_theta;
    m_irf_radial_iter_phi       = rsp.m_irf_radial_iter_phi;
    m_irf_elliptical_iter_theta = rsp.m_irf_elliptical_iter_theta;
    m_irf_elliptical_iter_phi   = rsp.m_irf_elliptical_iter_phi;
    m_irf_diffuse_resolution    = rsp.m_irf_diffuse_resolution;
    m_irf_cache                 = rsp.m_irf_cache;
    m_nroi_cache                = rsp.m_nroi_cache;
    m_irf_vector_cache          = rsp.m_irf_vector_cache;
 
    // Return
    return;
}
 
 
/***********************************************************************//**
 * @brief Delete class members
 ***************************************************************************/
void GResponse::free_members(void)
{
    // Return
    return;
}
 
 
/***********************************************************************//**
 * @brief Return instrument response to point source
 *
 * @param[in] event Observed event.
 * @param[in] source Source.
 * @param[in] obs Observation.
 * @return Instrument response to point source.
 *
 * Returns the instrument response to a point source.
 ***************************************************************************/
double GResponse::irf_ptsrc(const GEvent&       event,
                            const GSource&      source,
                            const GObservation& obs) const
{
    // Get pointer to point source model
    const GModelSpatialPointSource* model =
          static_cast<const GModelSpatialPointSource*>(source.model());
 
    // Setup photon
    GPhoton photon(model->dir(), source.energy(), source.time());
 
    // Get IRF
    double irf = this->irf(event, photon, obs);
 
    // Return IRF value
    return irf;
}
 
 
/***********************************************************************//**
 * @brief Return instrument response to radial source
 *
 * @param[in] event Observed event.
 * @param[in] source Source.
 * @param[in] obs Observation.
 * @return Instrument response to radial source.
 *
 * Returns the instrument response to a radial source for a given event,
 * source and observation. The method computes
 *
 * \f[
 *    {\tt irf}(p', E', t') = \int_0^{\theta_{\rm max}}
 *                            M_{\rm S}(\theta | E, t) \, sin \, \theta
 *                            \int_0^{2\pi}
 *                            R(p', E', t' | \theta, \phi, E, t) \,
 *                            d\,\phi \, d\,\theta
 * \f]
 *
 * where
 * * \f$M_{\rm S}(\theta | E, t)\f$ is the radial model component,
 * * \f$R(p', E', t' | \theta, \phi, E, t)\f$ is the Instrument Response
 *   Function (IRF),
 * * \f$p'\f$ is the measured instrument direction,
 * * \f$E'\f$ is the measured or reconstructed energy,
 * * \f$t'\f$ is the measured arrival time,
 * * \f$\theta\f$ is the radial distance from the model centre,
 * * \f$\phi\f$ is the azimuthal angle around the model centre,
 * * \f$E\f$ is the true photon energy, and
 * * \f$t\f$ is the true trigger time.
 *
 * The azimuth integration is done over \f$2\pi\f$ using the
 * irf_radial_kern_phi::eval() method.
 * The radial integration is done out to a maximum angle
 * \f$\theta_{\rm max}\f$, given by GModelSpatialRadial::theta_max(), by the
 * irf_radial_kern_theta::eval() method.
 ***************************************************************************/
double GResponse::irf_radial(const GEvent&       event,
                             const GSource&      source,
                             const GObservation& obs) const
{
    // Initialise IRF
    double irf = 0.0;
 
    // Get pointer to radial model
    const GModelSpatialRadial* model =
          static_cast<const GModelSpatialRadial*>(source.model());
 
    // Get source attributes
    const GEnergy& srcEng  = source.energy();
    const GTime&   srcTime = source.time();
 
    // Set radial integration range (radians)
    double theta_min = 0.0;
    double theta_max = model->theta_max() - 1.0e-12; // Kludge to stay inside
                                                     // the boundary of a
                                                     // sharp edged model
 
    // Integrate if interval is valid
    if (theta_max > theta_min) {
 
        // Allocate Euler and rotation matrices
        GMatrix ry;
        GMatrix rz;
 
        // Set up rotation matrix to rotate from native model coordinates to
        // celestial coordinates
        ry.eulery( model->dir().dec_deg() - 90.0);
        rz.eulerz(-model->dir().ra_deg());
        GMatrix rot = (ry * rz).transpose();
 
        // Setup integration kernel
        irf_radial_kern_theta integrand(this,
                                        &event,
                                        &obs,
                                        model,
                                        &rot,
                                        &srcEng,
                                        &srcTime,
                                        m_irf_radial_iter_phi);
 
        // Integrate over model's radial coordinate
        GIntegral integral(&integrand);
        integral.fixed_iter(m_irf_radial_iter_theta);
 
        // Integrate kernel
        irf = integral.romberg(theta_min, theta_max, m_irf_radial_iter_theta);
 
        // Compile option: Check for NaN/Inf
        #if defined(G_NAN_CHECK)
        if (gammalib::is_notanumber(irf) || gammalib::is_infinite(irf)) {
            std::cout << "*** ERROR: GResponse::irf_radial:";
            std::cout << " NaN/Inf encountered";
            std::cout << " (irf=" << irf;
            std::cout << ", theta_min=" << theta_min;
            std::cout << ", theta_max=" << theta_max << ")";
            std::cout << std::endl;
        }
        #endif
 
    } // endif: integration interval was valid
 
    // 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.
 * @return Instrument response to elliptical source.
 *
 * Returns the instrument response to an elliptical source for a given event,
 * source and observation. The method computes
 *
 * \f[
 *    {\tt irf}(p', E', t') = \int_0^{\theta_{\rm max}} \int_0^{2\pi}
 *                            M_{\rm S}(\theta, \phi | E, t) \,
 *                            R(p', E', t' | \theta, \phi, E, t) \,
 *                            sin \, \theta \,
 *                            d\,\phi \, d\,\theta
 * \f]
 *
 * where
 * * \f$M_{\rm S}(\theta, \phi | E, t)\f$ is the elliptical model component,
 * * \f$R(p', E', t' | \theta, \phi, E, t)\f$ is the Instrument Response
 *   Function (IRF),
 * * \f$p'\f$ is the measured instrument direction,
 * * \f$E'\f$ is the measured or reconstructed energy,
 * * \f$t'\f$ is the measured arrival time,
 * * \f$\theta\f$ is the radial distance from the model centre,
 * * \f$\phi\f$ is the azimuthal angle around the model centre,
 * * \f$E\f$ is the true photon energy, and
 * * \f$t\f$ is the true trigger time.
 *
 * The azimuth integration is done over \f$2\pi\f$ using the
 * irf_elliptical_kern_phi::eval() method.
 * The radial integration is done out to a maximum angle
 * \f$\theta_{\rm max}\f$, given by GModelSpatialElliptical::theta_max(), by
 * the irf_elliptical_kern_theta::eval() method.
 ***************************************************************************/
double GResponse::irf_elliptical(const GEvent&       event,
                                 const GSource&      source,
                                 const GObservation& obs) const
{
    // Initialise IRF
    double irf = 0.0;
 
    // Get pointer to elliptical model
    const GModelSpatialElliptical* model =
          static_cast<const GModelSpatialElliptical*>(source.model());
 
    // Get source attributes
    const GEnergy& srcEng  = source.energy();
    const GTime&   srcTime = source.time();
 
    // Set radial integration range (radians)
    double theta_min = 0.0;
    double theta_max = model->theta_max() - 1.0e-6; // Kludge to stay inside
                                                    // the boundary of a
                                                    // sharp edged model
 
    // Integrate if interval is valid
    if (theta_max > theta_min) {
 
        // Allocate Euler and rotation matrices
        GMatrix ry;
        GMatrix rz;
 
        // Set up rotation matrix to rotate from native model coordinates to
        // celestial coordinates
        ry.eulery( model->dir().dec_deg() - 90.0);
        rz.eulerz(-model->dir().ra_deg());
        GMatrix rot = (ry * rz).transpose();
 
        // Setup integration kernel
        irf_elliptical_kern_theta integrand(this,
                                            &event,
                                            &obs,
                                            model,
                                            &rot,
                                            &srcEng,
                                            &srcTime,
                                            m_irf_elliptical_iter_phi);
 
        // Integrate over model's radial coordinate
        GIntegral integral(&integrand);
        integral.fixed_iter(m_irf_elliptical_iter_theta);
 
        // Integrate kernel
        irf = integral.romberg(theta_min, theta_max, m_irf_elliptical_iter_theta);
 
        // Compile option: Check for NaN/Inf
        #if defined(G_NAN_CHECK)
        if (gammalib::is_notanumber(irf) || gammalib::is_infinite(irf)) {
            std::cout << "*** ERROR: GResponse::irf_elliptical:";
            std::cout << " NaN/Inf encountered";
            std::cout << " (irf=" << irf;
            std::cout << ", theta_min=" << theta_min;
            std::cout << ", theta_max=" << theta_max << ")";
            std::cout << std::endl;
        }
        #endif
 
    } // endif: integration interval was valid
 
    // Return IRF value
    return irf;
}
 
 
/***********************************************************************//**
 * @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 diffuse source for a given event,
 * source and observation. The method computes
 *
 * \f[
 *    {\tt irf}(p', E', t') = \sum_p M_{\rm S}(p | E, t) \, \Delta(p)
 *                                   R(p', E', t' | p, E, t)
 * \f]
 *
 * where
 * * \f$M_{\rm S}(p | E, t)\f$ is the diffuse model component,
 * * \f$\Delta(p)\f$ is the solid angle of the map pixel
 * * \f$R(p', E', t' | p, E, t)\f$ is the Instrument Response Function (IRF),
 * * \f$p'\f$ is the measured instrument direction,
 * * \f$E'\f$ is the measured or reconstructed energy,
 * * \f$t'\f$ is the measured arrival time,
 * * \f$p\f$ is the true photon arrival direction,
 * * \f$E\f$ is the true photon energy, and
 * * \f$t\f$ is the true trigger time.
 *
 * The method simply adds up all sky map pixels multiplied with the IRF for
 * all diffuse model pixels. For models that do not contain sky map pixels
 * (such as the GModelSpatialDiffuseConst model) the method allocates an
 * all-sky sky map with an angular resolution that is specified by the
 * m_irf_diffuse_resolution member.
 ***************************************************************************/
double GResponse::irf_diffuse(const GEvent&       event,
                              const GSource&      source,
                              const GObservation& obs) const
{
    // Initialise IRF
    double irf = 0.0;
 
    // Get source attributes
    const GEnergy& srcEng  = source.energy();
    const GTime&   srcTime = source.time();
 
    // If model is a diffuse map model then extract sky map
    const GModelSpatialDiffuseMap* map =
          dynamic_cast<const GModelSpatialDiffuseMap*>(source.model());
    if (map != NULL) {
 
        // Get reference to sky map
        const GSkyMap& skymap = map->map();
 
        // Loop over all sky map pixels
        for (int i = 0; i < skymap.npix(); ++i) {
 
            // Get map value
            double value = skymap(i);
 
            // Go to next pixel if map value is zero
            if (value == 0.0) {
                continue;
            }
 
            // Get sky direction
            GSkyDir srcDir = skymap.inx2dir(i);
 
            // Setup photon
            GPhoton photon(srcDir, srcEng, srcTime);
 
            // Add IRF multiplied by flux in map pixel. Since the map value
            // is per steradian we have to multiply with the solid angle of
            // the map pixel
            irf += this->irf(event, photon, obs) * value * skymap.solidangle(i);
 
        } // endfor: looped over all sky map pixels
 
    } // endif: model was diffuse map
 
    // ... otherwise if model is a cube map model then extract sky map
    else {
        const GModelSpatialDiffuseCube* cube =
              dynamic_cast<const GModelSpatialDiffuseCube*>(source.model());
        if (cube != NULL) {
 
            // Get reference to sky cube
            const GSkyMap& skymap = cube->cube();
 
            // Loop over all sky map pixels
            for (int i = 0; i < skymap.npix(); ++i) {
 
                // Get sky direction
                GSkyDir srcDir = skymap.inx2dir(i);
 
                // Setup photon
                GPhoton photon(srcDir, srcEng, srcTime);
 
                // Get map value
                double value = cube->eval(photon);
 
                // Go to next pixel if map value is not positive
                if (value <= 0.0) {
                    continue;
                }
 
                // Add IRF multiplied by flux in map pixel. Since the map
                // value is per steradian we have to multiply with the solid
                // angle of the map pixel
                irf += this->irf(event, photon, obs) * value * skymap.solidangle(i);
 
            } // endfor: looped over all sky map pixels
 
        } // endelse: model was diffuse cube
 
        // ... otherwise allocate all sky map with specified resolution
        else {
 
            // Allocate sky map
            int     nx     = int(360.0/m_irf_diffuse_resolution + 0.5);
            int     ny     = int(180.0/m_irf_diffuse_resolution + 0.5);
            double  dx     = 360.0 / double(nx);
            double  dy     = 180.0 / double(ny);
            GSkyMap skymap = GSkyMap("CAR", "CEL", 0.0, 0.0, -dx, dy, nx, ny);
 
            // Get pointer to diffuse model
            const GModelSpatialDiffuse* model =
                  static_cast<const GModelSpatialDiffuse*>(source.model());
 
            // Loop over all sky map pixels
            for (int i = 0; i < skymap.npix(); ++i) {
 
                // Get sky direction
                GSkyDir srcDir = skymap.inx2dir(i);
 
                // Setup photon
                GPhoton photon(srcDir, srcEng, srcTime);
 
                // Get model value
                double value = model->eval(photon);
 
                // Go to next pixel if map value is not positive
                if (value <= 0.0) {
                    continue;
                }
 
                // Add IRF multiplied by flux in map pixel. Since the map
                // value is per steradian we have to multiply with the solid
                // angle of the map pixel
                irf += this->irf(event, photon, obs) * value * skymap.solidangle(i);
 
            } // endfor: looped over sky map pixels
 
        } // endelse: model was not a cube
 
    } // endelse: model was not a map
 
    // Return IRF value
    return irf;
}
 
 
/***********************************************************************//**
 * @brief Return instrument response to composite source
 *
 * @param[in] event Observed event.
 * @param[in] source Source.
 * @param[in] obs Observation.
 * @return Instrument response to composite source.
 *
 * Returns the instrument response to a specified composite source.
 ***************************************************************************/
double GResponse::irf_composite(const GEvent&       event,
                                const GSource&      source,
                                const GObservation& obs) const
{
    // Initialise IRF
    double irf = 0.0;
 
    // Get pointer to composite model
    const GModelSpatialComposite* composite =
          dynamic_cast<const GModelSpatialComposite*>(source.model());
 
    // Loop over model components
    for (int i = 0; i < composite->components(); ++i) {
 
        // Get pointer to spatial component
        GModelSpatial* spat = const_cast<GModelSpatial*>(composite->component(i));
 
        // Set source name
        std::string name = source.name() + ":" + composite->name(i);
 
        // Create new GSource object
        GSource src(name, spat, source.energy(), source.time());
 
        // Compute irf value
        irf += irf_spatial(event, src, obs) * composite->scale(i)->value();
 
    }
 
    // Divide by number of model components
    double sum = composite->sum_of_scales();
    if (sum > 0.0) {
        irf /= sum;
    }
 
    // Return IRF value
    return irf;
}
 
 
/***********************************************************************//**
 * @brief Return instrument response to point source sky model
 *
 * @param[in] model Sky model.
 * @param[in] obs Observation.
 * @param[in] gradients Gradients matrix.
 * @return Instrument response to point source sky model.
 *
 * Returns the instrument response to a point source sky model for all
 * events.
 ***************************************************************************/
GVector GResponse::irf_ptsrc(const GModelSky&    model,
                             const GObservation& obs,
                             GMatrix*            gradients) const
{
    // Get number of events
    int nevents = obs.events()->size();
 
    // Initialise result
    GVector irfs(nevents);
 
    // Loop over events
    for (int k = 0; k < nevents; ++k) {
 
        // Get reference to event
        const GEvent& event = *((*obs.events())[k]);
 
        // Get source energy and time (no dispersion)
        GEnergy srcEng  = event.energy();
        GTime   srcTime = event.time();
 
        // Setup source
        GSource source(model.name(), model.spatial(), srcEng, srcTime);
 
        // Get IRF value for event
        irfs[k] = this->irf_ptsrc(event, source, obs);
 
    } // endfor: looped over events
 
    // Return IRF value
    return irfs;
}
 
 
/***********************************************************************//**
 * @brief Return instrument response to radial source sky model
 *
 * @param[in] model Sky model.
 * @param[in] obs Observation.
 * @param[in] gradients Gradients matrix.
 * @return Instrument response to radial source sky model.
 *
 * Returns the instrument response to a radial source sky model for all
 * events.
 ***************************************************************************/
GVector GResponse::irf_radial(const GModelSky&    model,
                              const GObservation& obs,
                              GMatrix*            gradients) const
{
    // Get number of events
    int nevents = obs.events()->size();
 
    // Initialise result
    GVector irfs(nevents);
 
    // Loop over events
    for (int k = 0; k < nevents; ++k) {
 
        // Get reference to event
        const GEvent& event = *((*obs.events())[k]);
 
        // Get source energy and time (no dispersion)
        GEnergy srcEng  = event.energy();
        GTime   srcTime = event.time();
 
        // Setup source
        GSource source(model.name(), model.spatial(), srcEng, srcTime);
 
        // Get IRF value for event
        irfs[k] = this->irf_radial(event, source, obs);
 
    } // endfor: looped over events
 
    // Return IRF value
    return irfs;
}
 
 
/***********************************************************************//**
 * @brief Return instrument response to ellipitical source sky model
 *
 * @param[in] model Sky model.
 * @param[in] obs Observation.
 * @param[in] gradients Gradients matrix.
 * @return Instrument response to ellipitical source sky model.
 *
 * Returns the instrument response to a ellipitical source sky model for all
 * events.
 ***************************************************************************/
GVector GResponse::irf_elliptical(const GModelSky&    model,
                                  const GObservation& obs,
                                  GMatrix*            gradients) const
{
    // Get number of events
    int nevents = obs.events()->size();
 
    // Initialise result
    GVector irfs(nevents);
 
    // Loop over events
    for (int k = 0; k < nevents; ++k) {
 
        // Get reference to event
        const GEvent& event = *((*obs.events())[k]);
 
        // Get source energy and time (no dispersion)
        GEnergy srcEng  = event.energy();
        GTime   srcTime = event.time();
 
        // Setup source
        GSource source(model.name(), model.spatial(), srcEng, srcTime);
 
        // Get IRF value for event
        irfs[k] = this->irf_elliptical(event, source, obs);
 
    } // endfor: looped over events
 
    // Return IRF value
    return irfs;
}
 
 
/***********************************************************************//**
 * @brief Return instrument response to diffuse source sky model
 *
 * @param[in] model Sky model.
 * @param[in] obs Observation.
 * @param[in] gradients Gradients matrix.
 * @return Instrument response to diffuse source sky model.
 *
 * Returns the instrument response to a diffuse source sky model for all
 * events.
 ***************************************************************************/
GVector GResponse::irf_diffuse(const GModelSky&    model,
                               const GObservation& obs,
                               GMatrix*            gradients) const
{
    // Get number of events
    int nevents = obs.events()->size();
 
    // Initialise result
    GVector irfs(nevents);
 
    // Get reference to normalisation parameter
    const GModelPar& value = (*model.spatial())[0];
 
    // Loop over events
    for (int k = 0; k < nevents; ++k) {
 
        // Get reference to event
        const GEvent& event = *((*obs.events())[k]);
 
        // Get source energy and time (no dispersion)
        GEnergy srcEng  = event.energy();
        GTime   srcTime = event.time();
 
        // Setup source
        GSource source(model.name(), model.spatial(), srcEng, srcTime);
 
        // Get IRF value for event
        irfs[k] = this->irf_diffuse(event, source, obs);
 
        // Optionally compute normalisation parameter gradient
        if (gradients != NULL) {
            (*gradients)(k,0) = (value.is_free()) ? irfs[k] * value.scale() : 0.0;
        }
 
    } // endfor: looped over events
 
    // Return IRF value
    return irfs;
}
 
 
/***********************************************************************//**
 * @brief Return instrument response to composite source sky model
 *
 * @param[in] model Sky model.
 * @param[in] obs Observation.
 * @param[in] gradients Gradients matrix.
 * @return Instrument response to composite source sky model.
 *
 * Returns the instrument response to a composite source sky model for all
 * events.
 ***************************************************************************/
GVector GResponse::irf_composite(const GModelSky&    model,
                                 const GObservation& obs,
                                 GMatrix*            gradients) const
{
    // Get number of events
    int nevents = obs.events()->size();
 
    // Initialise result
    GVector irfs(nevents);
 
    // Get pointer to composite spatial model
    const GModelSpatialComposite* composite = dynamic_cast<const GModelSpatialComposite*>(model.spatial());
 
    // Create copy of sky model
    GModelSky sky = model;
 
    // Initialise spatial gradient parameter index
    int ipar = 0;
 
    // Compute sum of scales
    double sum = (composite->normalize()) ? composite->sum_of_scales() : 0.0;
 
    // Loop over model components
    for (int i = 0; i < composite->components(); ++i) {
 
        // Get spatial component
        const GModelSpatial* spatial = const_cast<GModelSpatial*>(composite->component(i));
 
        // Set spatial component of sky model
        sky.spatial(spatial);
 
        // Set model name
        sky.name(model.name()+":"+composite->name(i));
 
        // Initialise matrix to hold spatial gradients
        GMatrix spat_gradients(nevents, spatial->size());
 
        // Compute IRF values
        GVector irf = irf_spatial(sky, obs, &spat_gradients);
 
        // Add IRF values
        irfs += irf * composite->scale(i)->value();
 
        // Optionally compute gradients
        if (gradients != NULL) {
 
            // Put spatial gradients in full matrix
            for (int j = 0; j < spatial->size(); ++j, ++ipar) {
                for (int k = 0; k < nevents; ++k) {
                    (*gradients)(k,ipar) = spat_gradients(k,j);
                }
            }
 
            // Compute normalised scale
            double scale = (composite->normalize() && sum != 0.0) ?
                            composite->scale(i)->scale() *
                            (1.0 / sum - composite->scale(i)->value() / (sum*sum)) :
                            composite->scale(i)->scale();
 
            // Compute scale gradient
            for (int k = 0; k < nevents; ++k) {
                (*gradients)(k,ipar) = (composite->scale(i)->is_free()) ? irf[k] * scale : 0.0;
            }
 
            // Increment parameter index to account for scale gradient
            ipar++;
 
        }
 
    } // endfor: looped over all model components
 
    // If composite model is normalised then divide result by number of model
    // components
    if (composite->normalize() && sum != 0.0) {
        irfs /= sum;
    }
 
    // Return IRF values
    return irfs;
}
 
 
/***********************************************************************//**
 * @brief Convolve sky model with the instrument response
 *
 * @param[in] model Sky model.
 * @param[in] event Event.
 * @param[in] srcEng Source energy.
 * @param[in] srcTime Source time.
 * @param[in] obs Observation.
 * @param[in] grad Should model gradients be computed? (default: true)
 * @return Event probability.
 *
 * Computes the event probability
 *
 * \f[
 *    P(p',E',t'|E,t) = \int S(p,E,t) \times R(p',E',t'|p,E,t) \, dp
 * \f]
 *
 * for a given true energy \f$E\f$ and time \f$t\f$.
 ***************************************************************************/
double GResponse::eval_prob(const GModelSky&    model,
                            const GEvent&       event,
                            const GEnergy&      srcEng,
                            const GTime&        srcTime,
                            const GObservation& obs,
                            const bool&         grad) const
{
    // Initialise result
    double prob = 0.0;
 
    // Continue only if the model has a spatial component
    if (model.spatial() != NULL) {
 
        // Set source
        GSource source(model.name(), model.spatial(), srcEng, srcTime);
 
        // Compute IRF value
        double irf = irf_spatial(event, source, obs);
 
        // Continue only if IRF value is positive
        if (irf > 0.0) {
 
            // Optionally get scaling
            double scale = (model.has_scales())
                           ? model.scale(obs.instrument()).value() : 1.0;
 
            // Evaluate spectral and temporal components
            double spec = (model.spectral() != NULL)
                          ? model.spectral()->eval(srcEng, srcTime, grad) : 1.0;
            double temp = (model.temporal() != NULL)
                          ? model.temporal()->eval(srcTime, grad) : 1.0;
 
            // Compute probability
            prob = spec * temp * irf * scale;
 
            // Optionally compute partial derivatives
            if (grad) {
 
                // Multiply factors to spectral gradients
                if (model.spectral() != NULL) {
                    double fact = temp * irf * scale;
                    if (fact != 1.0) {
                        for (int i = 0; i < model.spectral()->size(); ++i) {
                            (*model.spectral())[i].factor_gradient((*model.spectral())[i].factor_gradient() * fact);
                        }
                    }
                }
 
                // Multiply factors to temporal gradients
                if (model.temporal() != NULL) {
                    double fact = spec * irf * scale;
                    if (fact != 1.0) {
                        for (int i = 0; i < model.temporal()->size(); ++i) {
                            (*model.temporal())[i].factor_gradient((*model.temporal())[i].factor_gradient() * fact);
                        }
                    }
                }
 
                // Optionally compute scale gradient for instrument
                if (model.has_scales()) {
                    for (int i = 0; i < model.scales(); ++i) {
                        double g_scale = 0.0;
                        if (model.scale(i).name() == obs.instrument()) {
                            if (model.scale(i).is_free()) {
                                g_scale = model.scale(i).scale() * spec * temp * irf;
                            }
                        }
                        model.scale(i).factor_gradient(g_scale);
                    }
                }
 
            } // endif: computed partial derivatives
 
            // Compile option: Check for NaN/Inf
            #if defined(G_NAN_CHECK)
            if (gammalib::is_notanumber(prob) || gammalib::is_infinite(prob)) {
                std::cout << "*** ERROR: GResponse::eval_prob:";
                std::cout << " NaN/Inf encountered";
                std::cout << " (prob=" << prob;
                std::cout << ", spec=" << spec;
                std::cout << ", temp=" << temp;
                std::cout << ", irf=" << irf;
                std::cout << ")" << std::endl;
            }
            #endif
 
        } // endif: IRF value was positive
 
        // ... otherwise if gradient computation is requested then set the
        // spectral and temporal gradients to zero
        else if (grad) {
 
            // Reset spectral gradients
            if (model.spectral() != NULL) {
                for (int i = 0; i < model.spectral()->size(); ++i) {
                    (*model.spectral())[i].factor_gradient(0.0);
                }
            }
 
            // Reset temporal gradients
            if (model.temporal() != NULL) {
                for (int i = 0; i < model.temporal()->size(); ++i) {
                    (*model.temporal())[i].factor_gradient(0.0);
                }
            }
 
            // Optionally reset scale gradients
            if (model.has_scales()) {
                for (int i = 0; i < model.scales(); ++i) {
                    model.scale(i).factor_gradient(0.0);
                }
            }
 
        } // endelse: IRF value was not positive
 
    } // endif: Gamma-ray source model had a spatial component
 
    // Return event probability
    return prob;
}
 
 
/***********************************************************************//**
 * @brief Convolve sky model with the instrument response
 *
 * @param[in] model Sky model.
 * @param[in] obs Observation.
 * @param[out] gradients Pointer to matrix of gradients.
 * @return Event probabilities.
 *
 * Computes the event probability
 *
 * \f[
 *    P(p',E',t'|E,t) = \int S(p,E,t) \times R(p',E',t'|p,E,t) \, dp
 * \f]
 *
 * for a all events.
 ***************************************************************************/
GVector GResponse::eval_probs(const GModelSky&    model,
                              const GObservation& obs,
                              GMatrixSparse*      gradients) const
{
    // Get number of model parameters and number of events
    int npars   = model.size();
    int nevents = obs.events()->size();
 
    // Initialise gradients flag
    bool grad = (gradients != NULL);
 
    // Initialise result
    GVector probs(nevents);
 
    // Continue only if the model has a spatial component
    if (model.spatial() != NULL) {
 
        // Initialise matrix to hold spatial gradients
        GMatrix spat_gradients(nevents, model.spatial()->size());
 
        // Compute IRF value
        probs = irf_spatial(model, obs, &spat_gradients);
 
        // Get global model scaling
        double scale = (model.has_scales())
                       ? model.scale(obs.instrument()).value() : 1.0;
 
        // Initialise temporary vectors to hold gradients
        GVector* tmp_gradients = NULL;
        if (grad) {
            tmp_gradients = new GVector[npars];
            for (int i = 0; i < npars; ++i) {
                tmp_gradients[i] = GVector(nevents);
            }
        }
 
        // Loop over events
        for (int k = 0; k < nevents; ++k) {
 
            // Get probability
            double spat = probs[k];
 
            // Continue only if spatial value is positive
            if (spat > 0.0) {
 
                // Get reference to event
                const GEvent& event = *((*obs.events())[k]);
 
                // Get source energy and time
                GEnergy srcEng  = event.energy();
                GTime   srcTime = event.time();
 
                // Evaluate spectral and temporal components
                double spec = (model.spectral() != NULL)
                              ? model.spectral()->eval(srcEng, srcTime, grad)
                              : 1.0;
                double temp = (model.temporal() != NULL)
                              ? model.temporal()->eval(srcTime, grad)
                              : 1.0;
 
                // Compute probability
                probs[k] = spat * spec * temp * scale;
 
                // Optionally compute partial derivatives
                if (grad) {
 
                    // Get number of spatial, spectral and temporal parameters
                    int n_spat = model.spatial()->size();
                    int n_spec = model.spectral()->size();
                    int n_temp = model.temporal()->size();
 
                    // Multiply factors to spatial gradients
                    if (model.spatial() != NULL) {
                        double fact = spec * temp * scale;
                        for (int i = 0; i < n_spat; ++i) {
                            tmp_gradients[i][k] = spat_gradients(k,i) * fact;
                        }
                    }
 
                    // Multiply factors to spectral gradients
                    if (model.spectral() != NULL) {
                        int    offset = n_spat;
                        double fact   = spat * temp * scale;
                        for (int i = 0; i < n_spec; ++i) {
                            tmp_gradients[offset+i][k] =
                                (*(model.spectral()))[i].factor_gradient() * fact;
                        }
                    }
 
                    // Multiply factors to temporal gradients
                    if (model.temporal() != NULL) {
                        int    offset = n_spat + n_spec;
                        double fact   = spat * spec * scale;
                        for (int i = 0; i < n_temp; ++i) {
                            tmp_gradients[offset+i][k] =
                                (*(model.temporal()))[i].factor_gradient() * fact;
                        }
                    }
 
                    // Optionally set scale gradient for instrument
                    if (model.has_scales()) {
                        int    offset = n_spat + n_spec + n_temp;
                        double fact   = spat * spec * temp;
                        for (int i = 0; i < model.scales(); ++i) {
                            const GModelPar& par     = model.scale(i);
                            double           g_scale = 0.0;
                            if (par.name() == obs.instrument()) {
                                if (par.is_free()) {
                                    tmp_gradients[offset+i][k] = par.scale() * fact;
                                }
                            }
                        }
                    }
 
                } // endif: computed partial derivatives
 
            } // endif: IRF spatial value was positive
 
            // Compile option: Check for NaN/Inf
            #if defined(G_NAN_CHECK)
            if (gammalib::is_notanumber(probs[k]) || gammalib::is_infinite(probs[k])) {
                std::cout << "*** ERROR: GResponse::eval_prob:";
                std::cout << " NaN/Inf encountered";
                std::cout << " (probs[" << k << "]=" << probs[k];
                std::cout << ", spat=" << spat;
                std::cout << ")" << std::endl;
            }
            #endif
 
        } // endfor: looped over events
 
        // Post-process gradients
        if (grad) {
 
            // Fill gradients into matrix
            for (int i = 0; i < npars; ++i) {
                gradients->column(i, tmp_gradients[i]);
            }
 
            // Delete temporal gradients
            delete [] tmp_gradients;
 
        } // endif: gradient post processing
 
    } // endif: Gamma-ray source model had a spatial component
 
    // Return event probabilities
    return probs;
}
 
 
/***********************************************************************//**
 * @brief Return size of vector for energy dispersion computation
 *
 * @param[in] model Sky model.
 * @param[in] obs Observation.
 * @param[out] grad Signals whether gradients should be computed.
 * @return Size of vector for energy dispersion computation.
 *
 * Computes the size of the vector that will be computed for the computation
 * of the energy dispersion.
 ***************************************************************************/
int GResponse::size_edisp_vector(const GModelSky&    model,
                                 const GObservation& obs,
                                 const bool&         grad) const
{
    // Initialise vector size
    int size = 1;
 
    // Determine size of gradient part
    if (grad) {
        if (model.spectral() != NULL) {
            for (int i = 0; i < model.spectral()->size(); ++i) {
                GModelPar& par = (*(model.spectral()))[i];
                if (par.is_free() && par.has_grad()) {
                    size++;
                }
            }
        }
        if (model.temporal() != NULL) {
            for (int i = 0; i < model.temporal()->size(); ++i) {
                GModelPar& par = (*(model.temporal()))[i];
                if (par.is_free() && par.has_grad()) {
                    size++;
                }
            }
        }
        if (model.has_scales()) {
            for (int i = 0; i < model.scales(); ++i) {
                GModelPar& par = const_cast<GModelPar&>(model.scale(i));
                if (par.name() == obs.instrument()) {
                    if (par.is_free() && par.has_grad()) {
                        size++;
                    }
                }
            }
        }
    }
 
    // Return size
    return size;
}
 
 
/***********************************************************************//**
 * @brief Constructor for energy dispersion integration kernels class
 *
 * @param[in] parent Pointer to response.
 * @param[in] obs Pointer to observation.
 * @param[in] model Pointer to sky model.
 * @param[in] event Pointer to event.
 * @param[in] srcTime True time.
 * @param[in] grad Evaluate gradients?
 *
 * This method constructs the integration kernel needed for the energy
 * dispersion computation.
 ***************************************************************************/
GResponse::edisp_kerns::edisp_kerns(const GResponse*    parent,
                                    const GObservation* obs,
                                    const GModelSky*    model,
                                    const GEvent*       event,
                                    const GTime&        srcTime,
                                    const bool&         grad)
{
    // Set members
    m_parent  = parent;
    m_obs     = obs;
    m_model   = model;
    m_event   = event;
    m_size    = 1;
    m_srcTime = srcTime;
    m_grad    = grad;
 
    // If gradients are requested then put pointers to all relevant parameter
    // in the parameter pointer vector
    m_pars.clear();
    if (m_grad) {
 
        // Add free spectral parameters with analytical gradients
        if (m_model->spectral() != NULL) {
            for (int i = 0; i < m_model->spectral()->size(); ++i) {
                GModelPar& par = (*(m_model->spectral()))[i];
                if (par.is_free() && par.has_grad()) {
                    m_pars.push_back(&par);
                }
            }
        }
 
        // Add free temporal parameters with analytical gradients
        if (m_model->temporal() != NULL) {
            for (int i = 0; i < m_model->temporal()->size(); ++i) {
                GModelPar& par = (*(m_model->temporal()))[i];
                if (par.is_free() && par.has_grad()) {
                    m_pars.push_back(&par);
                }
            }
        }
 
        // Add free scaling factors
        if (m_model->has_scales()) {
            for (int i = 0; i < m_model->scales(); ++i) {
                GModelPar& par = const_cast<GModelPar&>(m_model->scale(i));
                if (par.name() == m_obs->instrument()) {
                    if (par.is_free() && par.has_grad()) {
                        m_pars.push_back(&par);
                    }
                }
            }
        }
 
        // Update size
        m_size += m_pars.size();
 
    } // endif: gradients were requested
 
    // Return
    return;
}
 
 
/***********************************************************************//**
 * @brief Return true energy intervals for sky model
 *
 * @param[in] model Sky model.
 * @return True energy intervals.
 *
 * Returns the true energy intervals for a sky model. For all spectral
 * models other than the GModelSpectralGauss model the method will return
 * an empty energy boundaries structure. For the GModelSpectralGauss model
 * the method will return the interval [mean - 5 * sigma, mean + 5 * sigma].
 ***************************************************************************/
GEbounds GResponse::ebounds_model(const GModelSky& model) const
{
    // Initialise empty energy boundaries
    GEbounds ebounds;
 
    // If the spectral model is a Gaussian line then return
    const GModelSpectralGauss* gauss =
          dynamic_cast<const GModelSpectralGauss*>(model.spectral());
    if (gauss != NULL) {
 
        // Define width of energy interval
        const double width = 5.0;
 
        // Compute energy boundaries
        GEnergy mean       = gauss->mean();
        GEnergy sigma      = gauss->sigma();
        GEnergy ebound_min = mean - width * sigma;
        GEnergy ebound_max = mean + width * sigma;
 
        // Make sure that energies are not negative positive
        if (ebound_min.MeV() < 0.0) {
            ebound_min.MeV(0.0);
        }
        if (ebound_max.MeV() < 0.0) {
            ebound_max.MeV(0.0);
        }
 
        // If energy boundaries define a positive interval then append them
        if (ebound_max > ebound_min) {
            ebounds.append(ebound_min, ebound_max);
        }
 
    } // endif: spectral model was a Gaussian
 
    // Return energy boudnaries
    return ebounds;
}
 
 
/***********************************************************************//**
 * @brief Evaluate energy dispersion integration kernel
 *
 * @param[in] etrue True photon energy in MeV.
 *
 * This method implements the integration kernel needed for the
 * GResponse::edisp_kern() class.
 ***************************************************************************/
GVector GResponse::edisp_kerns::eval(const double& etrue)
{
    // Initialise result
    GVector kernels(m_size);
 
    // Initialise Ndarray array index
    int index = 0;
 
    // Set true energy
    GEnergy srcEng;
    srcEng.MeV(etrue);
 
    // Get function value
    kernels[index++] = m_parent->eval_prob(*m_model, *m_event,
                                           srcEng, m_srcTime, *m_obs,
                                           m_grad);
 
    // If gradients are requested then extract them and put them into the
    // array
    if (m_grad) {
        for (int i = 0; i < m_pars.size(); ++i, ++index) {
            kernels[index] = m_pars[i]->factor_gradient();
        }
    }
 
    // Compile option: Check for NaN
    #if defined(G_NAN_CHECK)
    if (gammalib::is_notanumber(kernels[0]) || gammalib::is_infinite(kernels[0])) {
        std::cout << "*** ERROR: GResponse::edisp_kern::eval";
        std::cout << "(etrue=" << etrue << "): NaN/Inf encountered";
        std::cout << " (value=" << kernels[0] << ")" << std::endl;
    }
    #endif
 
    // Return kernels
    return kernels;
}
 
 
/***********************************************************************//**
 * @brief Zenith angle integration kernel for radial model
 *
 * @param[in] theta Zenith angle (radians).
 * @return IRF value.
 *
 * Integrated the IRF multiplied by the model value for a given zenith angle
 * over all azimuth angles.
 ***************************************************************************/
double GResponse::irf_radial_kern_theta::eval(const double& theta)
{
    // Initialise result
    double irf = 0.0;
 
    // Continue only for positive zenith angles (otherwise the integral will
    // be zero)
    if (theta > 0.0) {
 
        // Evaluate sky model
        double model = m_model->eval(theta, *m_srcEng, *m_srcTime);
 
        // Continue only if model is positive
        if (model > 0.0) {
 
            // Set azimuthal integration range
            double phi_min = 0.0;
            double phi_max = gammalib::twopi;
 
            // Setup integration kernel
            irf_radial_kern_phi integrand(m_rsp,
                                          m_event,
                                          m_obs,
                                          m_rot,
                                          theta,
                                          m_srcEng,
                                          m_srcTime);
 
            // Setup integration
            GIntegral integral(&integrand);
            integral.fixed_iter(m_iter_phi);
 
            // Integrate over phi
            irf = integral.romberg(phi_min, phi_max, m_iter_phi) *
                  model * std::sin(theta);
 
        } // endif: model was positive
 
    } // endif: theta was positive
 
    // Return result
    return irf;
}
 
 
/***********************************************************************//**
 * @brief Azimuth angle integration kernel for radial model
 *
 * @param[in] phi Azimuth angle (radians).
 * @return IRF value.
 *
 * Computes the IRF at a given zenith and azimuth angle with respect to a
 * specified centre.
 ***************************************************************************/
double GResponse::irf_radial_kern_phi::eval(const double& phi)
{
    // Set up native coordinate vector
    double  cos_phi = std::cos(phi);
    double  sin_phi = std::sin(phi);
    GVector native(-cos_phi*m_sin_theta, sin_phi*m_sin_theta, m_cos_theta);
 
    // Rotate vector into celestial coordinates
    GVector vector = (*m_rot) * native;
 
    // Convert vector into sky direction
    GSkyDir dir(vector);
 
    // Setup photon
    GPhoton photon(dir, *m_srcEng, *m_srcTime);
 
    // Evaluate IRF for photon
    double irf = m_rsp->irf(*m_event, photon, *m_obs);
 
    // Return
    return irf;
}
 
 
/***********************************************************************//**
 * @brief Zenith angle integration kernel for elliptical model
 *
 * @param[in] theta Zenith angle (radians).
 * @return IRF value.
 *
 * Integrated the IRF multiplied by the model value for a given zenith angle
 * over all azimuth angles.
 ***************************************************************************/
double GResponse::irf_elliptical_kern_theta::eval(const double& theta)
{
    // Initialise result
    double irf = 0.0;
 
    // Continue only for positive zenith angles (otherwise the integral will
    // be zero)
    if (theta > 0.0) {
 
        // Set azimuthal integration range
        double phi_min = 0.0;
        double phi_max = gammalib::twopi;
 
        // Setup integration kernel
        irf_elliptical_kern_phi integrand(m_rsp,
                                          m_event,
                                          m_obs,
                                          m_model,
                                          m_rot,
                                          theta,
                                          m_srcEng,
                                          m_srcTime);
 
        // Setup integration
        GIntegral integral(&integrand);
        integral.fixed_iter(m_iter_phi);
 
        // Integrate over phi
        irf = integral.romberg(phi_min, phi_max, m_iter_phi) * std::sin(theta);
 
    } // endif: theta was positive
 
    // Return result
    return irf;
}
 
 
/***********************************************************************//**
 * @brief Azimuth angle integration kernel for elliptical model
 *
 * @param[in] phi Azimuth angle (radians).
 * @return IRF value.
 *
 * Computes the IRF at a given zenith and azimuth angle with respect to a
 * specified centre.
 ***************************************************************************/
double GResponse::irf_elliptical_kern_phi::eval(const double& phi)
{
    // Initialise result
    double irf = 0.0;
 
    // Evaluate sky model
    double model = m_model->eval(m_theta, phi, *m_srcEng, *m_srcTime);
 
    // Continue only if model is positive
    if (model > 0.0) {
 
        // Set up native coordinate vector
        double  cos_phi = std::cos(phi);
        double  sin_phi = std::sin(phi);
        GVector native(-cos_phi*m_sin_theta, sin_phi*m_sin_theta, m_cos_theta);
 
        // Rotate vector into celestial coordinates
        GVector vector = (*m_rot) * native;
 
        // Convert vector into sky direction
        GSkyDir dir(vector);
 
        // Setup photon
        GPhoton photon(dir, *m_srcEng, *m_srcTime);
 
        // Evaluate IRF for photon
        irf = m_rsp->irf(*m_event, photon, *m_obs) * model;
 
    } // endif: model was positive
 
    // Return
    return irf;
}