/*************************************************************************** * GResponse.hpp - Abstract response base class * * ----------------------------------------------------------------------- * * copyright (C) 2008-2015 by Juergen Knoedlseder * * ----------------------------------------------------------------------- * * * * This program is free software: you can redistribute it and/or modify * * it under the terms of the GNU General Public License as published by * * the Free Software Foundation, either version 3 of the License, or * * (at your option) any later version. * * * * This program is distributed in the hope that it will be useful, * * but WITHOUT ANY WARRANTY; without even the implied warranty of * * MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the * * GNU General Public License for more details. * * * * You should have received a copy of the GNU General Public License * * along with this program. If not, see . * * * ***************************************************************************/ /** * @file GResponse.hpp * @brief Abstract response base class definition * @author Juergen Knoedlseder */ #ifndef GRESPONSE_HPP #define GRESPONSE_HPP /* __ Includes ___________________________________________________________ */ #include #include "GBase.hpp" #include "GFunction.hpp" #include "GTime.hpp" /* __ Forward declarations _______________________________________________ */ class GEvent; class GPhoton; class GSource; class GEnergy; class GEbounds; class GObservation; class GModelSky; /***********************************************************************//** * @class GResponse * * @brief Abstract instrument response base class * * The response function provides conversion between physical parameters * (such as source position, flux, ...) and the measured instrumental * parameters (such as measured energy, photon interaction, ...). * * For a given observation, the irf method returns the instrument response * for a given event and photon. An alternative method exists that returns * the response for a specific source. * * The nroi method returns the spatial integral of the instrument response * function times the sky model over the region of interest. This method is * only required for unbinned analysis. * * The ebounds method returns the true energy boundaries for a specified * measured event energy. This method is used for computing the energy * dispersion. ***************************************************************************/ class GResponse : public GBase { public: // Constructors and destructors GResponse(void); GResponse(const GResponse& rsp); virtual ~GResponse(void); // Operators virtual GResponse& operator=(const GResponse& rsp); // Pure virtual methods virtual void clear(void) = 0; virtual GResponse* clone(void) const = 0; virtual std::string classname(void) const = 0; virtual bool use_edisp(void) const = 0; virtual bool use_tdisp(void) const = 0; virtual double irf(const GEvent& event, const GPhoton& photon, const GObservation& obs) const = 0; virtual double irf(const GEvent& event, const GSource& source, const GObservation& obs) const = 0; virtual double nroi(const GModelSky& model, const GEnergy& obsEng, const GTime& obsTime, const GObservation& obs) const = 0; virtual GEbounds ebounds(const GEnergy& obsEng) const = 0; virtual std::string print(const GChatter& chatter = NORMAL) const = 0; // Virtual methods virtual double convolve(const GModelSky& model, const GEvent& event, const GObservation& obs, const bool& grad = true) const; protected: // Protected methods void init_members(void); void copy_members(const GResponse& rsp); void free_members(void); double eval_prob(const GModelSky& model, const GEvent& event, const GEnergy& srcEng, const GTime& srcTime, const GObservation& obs, const bool& grad) const; // Protected classes class edisp_kern : public GFunction { public: edisp_kern(const GResponse* parent, const GObservation* obs, const GModelSky* model, const GEvent* event, const GTime& srcTime, const bool& grad) : m_parent(parent), m_obs(obs), m_model(model), m_event(event), m_srcTime(srcTime), m_grad(grad) { } double eval(const double& x); protected: const GResponse* m_parent; //!< Response const GObservation* m_obs; //!< Observation const GModelSky* m_model; //!< Sky model const GEvent* m_event; //!< Event GTime m_srcTime; //!< True arrival time bool m_grad; //!< Gradient flag }; }; #endif /* GRESPONSE_HPP */