Update code documentation

Jürgen Knödlseder
1 parent 1c8a6842
Showing 5 changed files with 58 additions and 32 deletions
include/GModelSpectralBrokenPlaw.hpp
include/GModelTemporalLightCurve.hpp
include/GModelTemporalPhaseCurve.hpp
inst/cta/include/GCTAOnOffObservation.hpp
src/model/GModelSpectralBrokenPlaw.cpp
 /***************************************************************************
  *     GModelSpectralBrokenPlaw.hpp - Broken power law spectrum class      *
  * ----------------------------------------------------------------------- *
- *  copyright (C) 2013-2016 by Anneli Schulz                               *
+ *  copyright (C) 2013-2017 by Anneli Schulz                               *
  * ----------------------------------------------------------------------- *
  *                                                                         *
  *  This program is free software: you can redistribute it and/or modify   *
@@ -48,14 +48,19 @@ class GXmlElement;
  * by
  *
  * \f[
- *    S_{\rm E}(E | t) = {\tt m\_norm}
- *    \left( \frac{E}{\tt m\_breakenergy} \right)^{\tt m\_index1}
+ *    S_{\rm E}(E | t) = k_0 \times \left \{
+ *    \begin{eqnarray}
+ *     \left( \frac{E}{E_b} \right)^{\gamma_1} & {\rm if\,\,} E < E_b \\
+ *     \left( \frac{E}{E_b} \right)^{\gamma_2} & {\rm otherwise}
+ *    \end{eqnarray}
+ *    \right .
  * \f]
  *
  * where
- * - \f${\tt m\_norm}\f$ is the normalization or prefactor,
- * - \f${\tt m\_index1}\f$ is the spectral index1, and
- * - \f${\tt m\_breakenergy}\f$ is the breakenergy energy.
+ * \f$k_0\f$ is the normalization or prefactor,
+ * \f$\gamma_1\f$ is the spectral index before the break,
+ * \f$\gamma_2\f$ is the spectral index after the break, and
+ * \f$E_b\f$ is the break energy.
  ***************************************************************************/
 class GModelSpectralBrokenPlaw : public GModelSpectral {
@@ -55,9 +55,9 @@ class GXmlElement;
  * \f]
  *
  * where
- * \f$r(t)$\f is the rate defined by linear interpolation between the nodes
+ * \f$r(t)\f$ is the rate defined by linear interpolation between the nodes
  * in a FITS file, and
- * \f${\tt m\_norm}$\f is a normalisation constant.
+ * \f${\tt m\_norm}\f$ is a normalisation constant.
  ***************************************************************************/
 class GModelTemporalLightCurve : public GModelTemporal {
@@ -47,7 +47,7 @@ class GXmlElement;
  * @brief Temporal phase curve model class
  *
  * This class implements a temporal variation based on the phase
- * \f$\Phi(t)$\f that is computed using
+ * \f$\Phi(t)\f$ that is computed using
  *
  * \f[
  *    \Phi(t) = \Phi_0 + f(t-t_0) + \frac{1}{2}\dot{f} (t-t_0)^2 +
@@ -55,12 +55,12 @@ class GXmlElement;
  * \f]
  *
  * where
- * \f$t_0$\f is a reference time,
- * \f$\Phi_0$\f is the phase at the reference time,
- * \f$f$\f is the variation frequency at the reference time,
- * \f$\dot{f}$\f is the first derivative of the variation frequency at the
+ * \f$t_0\f$ is a reference time,
+ * \f$\Phi_0\f$ is the phase at the reference time,
+ * \f$f\f$ is the variation frequency at the reference time,
+ * \f$\dot{f}\f$ is the first derivative of the variation frequency at the
  * reference time, and
- * \f$\ddot{f}$\f is the second derivative of the variation frequency at the
+ * \f$\ddot{f}\f$ is the second derivative of the variation frequency at the
  * reference time.
  *
  * The temporal variation is then computed using
@@ -69,8 +69,8 @@ class GXmlElement;
  *    S_{\rm t}(t) = r(\Phi(t)) \times {\tt m\_norm}
  * \f]
  *
- * where \f$r(\Phi(t))$\f is the rate defined by linear interpolation between
- * the nodes in a FITS file, and \f${\tt m\_norm}$\f is a normalisation
+ * where \f$r(\Phi(t))\f$ is the rate defined by linear interpolation between
+ * the nodes in a FITS file, and \f${\tt m\_norm}\f$ is a normalisation
  * constant.
  ***************************************************************************/
 class GModelTemporalPhaseCurve : public GModelTemporal {
@@ -247,9 +247,9 @@ GTime GModelTemporalPhaseCurve::mjd(void) const
  * Sets the reference Modified Julian Day.
  ***************************************************************************/
 inline
-void GModelTemporalPhaseCurve::mjd(const GTime& time)
+void GModelTemporalPhaseCurve::mjd(const GTime& mjd)
 {
-    m_mjd.value(time.mjd());
+    m_mjd.value(mjd.mjd());
     return;
 }
@@ -320,7 +320,7 @@ const GRmf&amp; GCTAOnOffObservation::rmf(void) const
 inline
 int GCTAOnOffObservation::nobserved(void) const
 {
-    return (m_on_spec.counts());
+    return ((int)(m_on_spec.counts()+0.5));
 }
 #endif /* GCTAONOFFOBSERVATION_HPP */
 /***************************************************************************
  *     GModelSpectralBrokenPlaw.cpp - Broken power law spectrum class      *
  * ----------------------------------------------------------------------- *
- *  copyright (C) 2013-2016 by Anneli Schulz                               *
+ *  copyright (C) 2013-2017 by Anneli Schulz                               *
  * ----------------------------------------------------------------------- *
  *                                                                         *
  *  This program is free software: you can redistribute it and/or modify   *
@@ -294,32 +294,53 @@ GModelSpectralBrokenPlaw* GModelSpectralBrokenPlaw::clone(void) const
  * Evaluates
  *
  * \f[
- *    S_{\rm E}(E | t) = {\tt m\_norm}
- *    \left( \frac{E}{\tt m\_breakenergy} \right)^{\tt m\_index}
+ *    S_{\rm E}(E | t) = k_0 \times \left \{
+ *    \begin{eqnarray}
+ *     \left( \frac{E}{E_b} \right)^{\gamma_1} & {\rm if\,\,} E < E_b \\
+ *     \left( \frac{E}{E_b} \right)^{\gamma_2} & {\rm otherwise}
+ *    \end{eqnarray}
+ *    \right .
  * \f]
  *
  * where
- * - \f${\tt m\_norm}\f$ is the normalization or prefactor,
- * - \f${\tt m\_index}\f$ is the spectral index, and
- * - \f${\tt m\_breakenergy}\f$ is the breakenergy energy.
+ * \f$k_0\f$ is the normalization or prefactor,
+ * \f$\gamma_1\f$ is the spectral index before the break,
+ * \f$\gamma_2\f$ is the spectral index after the break, and
+ * \f$E_b\f$ is the break energy.
  *
  * If the @p gradients flag is true the method will also compute the
  * partial derivatives of the model with respect to the parameters using
  *
  * \f[
- *    \frac{\delta S_{\rm E}(E | t)}{\delta {\tt m\_norm}} =
- *      \frac{S_{\rm E}(E | t)}{{\tt m\_norm}}
+ *    \frac{\delta S_{\rm E}(E | t)}{\delta k_0} =
+ *      \frac{S_{\rm E}(E | t)}{k_0}
  * \f]
  *
  * \f[
- *    \frac{\delta S_{\rm E}(E | t)}{\delta {\tt m\_index}} =
- *      S_{\rm E}(E | t) \, \ln(E/{\tt m_breakenergy})
+ *    \frac{\delta S_{\rm E}(E | t)}{\delta \gamma_1} = \left \{
+ *    \begin{eqnarray}
+ *      S_{\rm E}(E | t) \, \ln(E/E_b) & {\rm if\,\,} E < E_b \\
+ *      0 & {\rm otherwise}
+ *    \end{eqnarray}
+ *    \right .
  * \f]
  *
  * \f[
- *    \frac{\delta S_{\rm E}(E | t)}{\delta {\tt m\_breakenergy}} =
- *      -S_{\rm E}(E | t) \,
- *      \left( \frac{{\tt m\_index}}{{\tt m\_breakenergy}} \right)
+ *    \frac{\delta S_{\rm E}(E | t)}{\delta \gamma_2} = \left \{
+ *    \begin{eqnarray}
+ *      0                              & {\rm if\,\,} E < E_b \\
+ *      S_{\rm E}(E | t) \, \ln(E/E_b) & {\rm otherwise}
+ *    \end{eqnarray}
+ *    \right .
+ * \f]
+ *
+ * \f[
+ *    \frac{\delta S_{\rm E}(E | t)}{\delta E_b} = k_0 \times \left \{
+ *    \begin{eqnarray}
+ *      -S_{\rm E}(E | t) \, \left( \frac{\gamma_1}{E_b} \right) & {\rm if\,\,} E < E_b \\
+ *      -S_{\rm E}(E | t) \, \left( \frac{\gamma_2}{E_b} \right) & {\rm otherwise}
+ *    \end{eqnarray}
+ *    \right .
  * \f]
  *
  * @todo The method expects that energy!=0. Otherwise Inf or NaN may result.