/*************************************************************************** * GModelSpatialRadialShell.hpp - Radial shell source model class * * ----------------------------------------------------------------------- * * copyright (C) 2011-2013 by Christoph Deil * * ----------------------------------------------------------------------- * * * * 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 GModelSpatialRadialShell.hpp * @brief Radial shell model class interface definition * @author Christoph Deil */ #ifndef GMODELSPATIALRADIALSHELL_HPP #define GMODELSPATIALRADIALSHELL_HPP /* __ Includes ___________________________________________________________ */ #include #include "GModelSpatialRadial.hpp" #include "GModelPar.hpp" #include "GSkyDir.hpp" #include "GXmlElement.hpp" /************************************************************************** * @class GModelSpatialRadialShell * * @brief Shell source model class * * This class implements the spatial component of the factorised source * model for a shell source (can be used e.g. as a toy supernova remnant * model). The shell is simply the volume between an inner and outer radius * (a large sphere with a smaller sphere cut out) with constant volume * emissivity and no absorption. To determine the surface brightness * distribution on the sky, the shell is analytically integrated along lines * of sight. * The shell is parametrised by the inner shell radius and the shell width. * Obviously, the shell width has to be a positive quantity. To assure * positivity, 1 arcsec is added internally to the shell width. This should * be negligible compared to shell widths encountered (and detectable) in * the gamma-ray domain, and improves the convergence of the fitting * algorithms. ***************************************************************************/ class GModelSpatialRadialShell : public GModelSpatialRadial { public: // Constructors and destructors GModelSpatialRadialShell(void); explicit GModelSpatialRadialShell(const GSkyDir& dir, const double& radius, const double& width, const bool& small_angle = true); explicit GModelSpatialRadialShell(const GXmlElement& xml); GModelSpatialRadialShell(const GModelSpatialRadialShell& model); virtual ~GModelSpatialRadialShell(void); // Operators virtual GModelSpatialRadialShell& operator=(const GModelSpatialRadialShell& model); // Implemented pure virtual methods virtual void clear(void); virtual GModelSpatialRadialShell* clone(void) const; virtual std::string type(void) const { return "ShellFunction"; } virtual double eval(const double& theta) const; virtual double eval_gradients(const double& theta) const; virtual GSkyDir mc(GRan& ran) const; virtual double theta_max(void) const; virtual void read(const GXmlElement& xml); virtual void write(GXmlElement& xml) const; virtual std::string print(void) const; // Other methods double radius(void) const { return m_radius.real_value(); } double width(void) const { return m_width.real_value(); } bool small_angle(void) const { return m_small_angle; } void radius(const double& radius) { m_radius.real_value(radius); } void width(const double& width) { m_width.real_value(width); } void small_angle(const bool& small_angle) { m_small_angle = small_angle; } protected: // Protected methods void init_members(void); void copy_members(const GModelSpatialRadialShell& model); void free_members(void); void update(void) const; static double f1(double x); static double f2(double x); // Protected members GModelPar m_radius; //!< Inner shell radius (deg) GModelPar m_width; //!< Shell thickness (deg) bool m_small_angle; //!< Use small angle approximate formulae // Cached members used for pre-computations mutable double m_last_radius; //!< Last shell radius (deg) mutable double m_last_width; //!< Last shell width (deg) mutable double m_theta_in; //!< Inner shell radius (rad) mutable double m_x_in; //!< m_theta_in^2 or sin(m_theta_in)^2 mutable double m_theta_out; //!< Outer shell radius (rad) mutable double m_x_out; //!< m_theta_out^2 or sin(m_theta_out)^2 mutable double m_norm; //!< Shell normalization }; #endif /* GMODELSPATIALRADIALSHELL_HPP */