/*************************************************************************** * GResponse.hpp - Abstract response base class * * ----------------------------------------------------------------------- * * copyright (C) 2008-2012 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 "GEvent.hpp" #include "GPhoton.hpp" #include "GSource.hpp" #include "GEnergy.hpp" #include "GTime.hpp" #include "GModelRadial.hpp" #include "GFunction.hpp" #include "GMatrix.hpp" /* __ Forward declarations _______________________________________________ */ class GObservation; /***********************************************************************//** * @class GResponse * * @brief Abstract interface for the instrument response function * * 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 source model as function of the true photon energy * and the true photon arrival time. * The npred method returns the integral of the instrument response function * over the dataspace. This method is only required for unbinned analysis. ***************************************************************************/ 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 bool hasedisp(void) const = 0; virtual bool hastdisp(void) const = 0; virtual double irf(const GEvent& event, const GPhoton& photon, const GObservation& obs) const = 0; virtual double npred(const GPhoton& photon, const GObservation& obs) const = 0; virtual std::string print(void) const = 0; // Virtual methods virtual double irf(const GEvent& event, const GSource& source, const GObservation& obs) const; virtual double irf_ptsrc(const GEvent& event, const GSource& source, const GObservation& obs) const; virtual double irf_extended(const GEvent& event, const GSource& source, const GObservation& obs) const; virtual double irf_diffuse(const GEvent& event, const GSource& source, const GObservation& obs) const; virtual double npred(const GSource& source, const GObservation& obs) const; virtual double npred_ptsrc(const GSource& source, const GObservation& obs) const; virtual double npred_extended(const GSource& source, const GObservation& obs) const; virtual double npred_diffuse(const GSource& source, const GObservation& obs) const; protected: // Protected methods void init_members(void); void copy_members(const GResponse& rsp); void free_members(void); // Npred theta integration kernel class npred_kern_theta : public GFunction { public: npred_kern_theta(const GResponse* rsp, const GModelRadial* radial, const GEnergy* srcEng, const GTime* srcTime, const GObservation* obs, const GMatrix* rot) : m_rsp(rsp), m_radial(radial), m_srcEng(srcEng), m_srcTime(srcTime), m_obs(obs), m_rot(rot) { } double eval(double theta); protected: const GResponse* m_rsp; //!< Pointer to response const GModelRadial* m_radial; //!< Pointer to radial spatial model const GEnergy* m_srcEng; //!< Pointer to true photon energy const GTime* m_srcTime; //!< Pointer to true photon arrival time const GObservation* m_obs; //!< Pointer to observation const GMatrix* m_rot; //!< Pointer to rotation matrix }; // Npred phi integration kernel class npred_kern_phi : public GFunction { public: npred_kern_phi(const GResponse* rsp, const GEnergy* srcEng, const GTime* srcTime, const GObservation* obs, const GMatrix* rot, double theta, double sin_theta) : m_rsp(rsp), m_srcEng(srcEng), m_srcTime(srcTime), m_obs(obs), m_rot(rot), m_theta(theta), m_cos_theta(std::cos(theta)), m_sin_theta(sin_theta) { } double eval(double phi); protected: const GResponse* m_rsp; //!< Pointer to response const GEnergy* m_srcEng; //!< Pointer to true photon energy const GTime* m_srcTime; //!< Pointer to true photon arrival time const GObservation* m_obs; //!< Pointer to observation const GMatrix* m_rot; //!< Pointer to rotation matrix double m_theta; //!< Offset angle (radians) double m_cos_theta; //!< cosine of offset angle double m_sin_theta; //!< Sine of offset angle }; }; #endif /* GRESPONSE_HPP */