Changeset 927 in Sophya


Ignore:
Timestamp:
Apr 14, 2000, 9:28:14 AM (25 years ago)
Author:
ansari
Message:

SOphie : Adding the ingroup SkyT in each .cc file for DoxyGen Doc

Location:
trunk/SophyaLib/SkyT
Files:
12 edited

Legend:

Unmodified
Added
Removed
  • trunk/SophyaLib/SkyT/blackbody.cc

    r909 r927  
    11//--------------------------------------------------------------------------
    22// File and Version Information:
    3 //      $Id: blackbody.cc,v 1.5 2000-04-13 14:10:43 ansari Exp $
     3//      $Id: blackbody.cc,v 1.6 2000-04-14 07:28:11 ansari Exp $
    44//
    55// Description:
     
    2121
    2222/*!
    23  * \class SOPHYA::BlackBody <BR>
     23 * \class SOPHYA::BlackBody
     24 \ingroup SkyT
    2425 This class corresponds to the emission spectrum of a
    2526 blackbody radiation.
  • trunk/SophyaLib/SkyT/convtools.cc

    r607 r927  
    11//--------------------------------------------------------------------------
    22// File and Version Information:
    3 //      $Id: convtools.cc,v 1.2 1999-11-20 21:00:48 ansari Exp $
     3//      $Id: convtools.cc,v 1.3 2000-04-14 07:28:12 ansari Exp $
    44//
    55// Description:
     
    1212#include "convtools.h"
    1313
     14/*! \class SOPHYA::ConvTools
     15 * \ingroup SkyT
     16 * Definition of usual usefull constants
     17 */
    1418// Boltzman constant  J/K
    1519double ConvTools::kb =  1.380662e-23;     
    1620// Mean value of the cmb temperature (K)
    1721double ConvTools::tcmb=2.728;
    18 // constante de Planck en Js
     22// Planck constant in Js
    1923double ConvTools::hpl=6.626176e-34;   
    2024// Light speed  PDG 1992 m/s
  • trunk/SophyaLib/SkyT/derivblackbody.cc

    r909 r927  
    11//--------------------------------------------------------------------------
    22// File and Version Information:
    3 //      $Id: derivblackbody.cc,v 1.3 2000-04-13 14:10:44 ansari Exp $
     3//      $Id: derivblackbody.cc,v 1.4 2000-04-14 07:28:12 ansari Exp $
    44//
    55// Description:
     
    2222
    2323
    24 /*! \class SOPHYA::DerivBlackBody <BR>
     24/*! \class SOPHYA::DerivBlackBody
     25  \ingroup SkyT
    2526 * This class corresponds to the emission spectrum of a
    2627 * dipole (since its emission spectrum is the derivation
  • trunk/SophyaLib/SkyT/gaussfilt.cc

    r909 r927  
    11//--------------------------------------------------------------------------
    22// File and Version Information:
    3 //      $Id: gaussfilt.cc,v 1.5 2000-04-13 14:10:44 ansari Exp $
     3//      $Id: gaussfilt.cc,v 1.6 2000-04-14 07:28:12 ansari Exp $
    44//
    55// Description:
     
    2121/*!
    2222 * \class SOPHYA::GaussianFilter
     23 * \ingroup SkyT
    2324 * Gaussian detector response
    2425 */
  • trunk/SophyaLib/SkyT/nupower.cc

    r909 r927  
    11//--------------------------------------------------------------------------
    22// File and Version Information:
    3 //      $Id: nupower.cc,v 1.6 2000-04-13 14:10:44 ansari Exp $
     3//      $Id: nupower.cc,v 1.7 2000-04-14 07:28:12 ansari Exp $
    44//
    55// Description:
     
    2323
    2424/*!
    25  * \class SOPHYA::PowerLawSpectra <BR>
     25 * \class SOPHYA::PowerLawSpectra
     26 \ingroup SkyT
    2627 * This class corresponds to a power law radiation spectrum.
    2728*/
  • trunk/SophyaLib/SkyT/radspec.cc

    r909 r927  
    11//--------------------------------------------------------------------------
    22// File and Version Information:
    3 //      $Id: radspec.cc,v 1.4 2000-04-13 14:10:44 ansari Exp $
     3//      $Id: radspec.cc,v 1.5 2000-04-14 07:28:13 ansari Exp $
    44//
    55// Description:
     
    2222#include "radspec.h"
    2323#include "integ.h"
    24 
    25 /*!
    26  * \class SOPHYA::RadSpectra <BR>
     24/*!
     25   \defgroup SkyT SkyT module
     26   This module contains classes and functions which define
     27   several radiation spectra and filter responses
     28*/
     29
     30/*!
     31 * \class SOPHYA::RadSpectra
     32 * \ingroup SkyT
    2733 * This class is an abstract base class for radiation emission spectra. The flux() function returns the value of the flux (the spectral      <BR>
    2834 * energy distribution) as a function of the frequency.  As in the SpectralResponse class, the () operator has been redefined <BR>
  • trunk/SophyaLib/SkyT/radspecvector.cc

    r909 r927  
    11//--------------------------------------------------------------------------
    22// File and Version Information:
    3 //      $Id: radspecvector.cc,v 1.6 2000-04-13 14:10:45 ansari Exp $
     3//      $Id: radspecvector.cc,v 1.7 2000-04-14 07:28:13 ansari Exp $
    44//
    55// Description:
     
    2929/*!
    3030 * \class SOPHYA::RadSpectraVec
     31 \ingroup SkyT
    3132 * One may define the radiation
    3233 * spectrum with two vectors: <BR> one for the frequencies and the second for the
  • trunk/SophyaLib/SkyT/skyinit.cc

    r759 r927  
    88#include "gaussfilt.h"
    99
     10/*! \class SOPHYA::SkyTInitiator
     11 *  \ingroup SkyT
     12 */
    1013int SkyTInitiator::FgInit = 0;
    1114
  • trunk/SophyaLib/SkyT/specresp.cc

    r909 r927  
    11//--------------------------------------------------------------------------
    22// File and Version Information:
    3 //      $Id: specresp.cc,v 1.4 2000-04-13 14:10:45 ansari Exp $
     3//      $Id: specresp.cc,v 1.5 2000-04-14 07:28:13 ansari Exp $
    44//
    55// Description:
     
    2222
    2323/*!
    24  * \class SOPHYA::SpectralResponse <BR>
     24 * \class SOPHYA::SpectralResponse
     25 \ingroup SkyT
    2526 SpectralResponse corresponds to a detector filter's
    2627 response as a function of the frequency.
  • trunk/SophyaLib/SkyT/specrespvector.cc

    r909 r927  
    11//--------------------------------------------------------------------------
    22// File and Version Information:
    3 //      $Id: specrespvector.cc,v 1.7 2000-04-13 14:10:45 ansari Exp $
     3//      $Id: specrespvector.cc,v 1.8 2000-04-14 07:28:14 ansari Exp $
    44//
    55// Description:
     
    2828/*!
    2929 * \class SOPHYA::SpecRespVec
     30 \ingroup SkyT
    3031 One may also want to defined the filter of a detector by two vectors:
    3132 one for the frequencies and one for the corresponding transmission values.
  • trunk/SophyaLib/SkyT/squarefilt.cc

    r909 r927  
    11//--------------------------------------------------------------------------
    22// File and Version Information:
    3 //      $Id: squarefilt.cc,v 1.5 2000-04-13 14:10:45 ansari Exp $
     3//      $Id: squarefilt.cc,v 1.6 2000-04-14 07:28:14 ansari Exp $
    44//
    55// Description:
     
    2020/*!
    2121 * \class SOPHYA::SquareFilter
     22 \ingroup SkyT
    2223 * Square detector response
    2324 */
  • trunk/SophyaLib/SkyT/trianglefilt.cc

    r909 r927  
    11//--------------------------------------------------------------------------
    22// File and Version Information:
    3 //      $Id: trianglefilt.cc,v 1.5 2000-04-13 14:10:46 ansari Exp $
     3//      $Id: trianglefilt.cc,v 1.6 2000-04-14 07:28:14 ansari Exp $
    44//
    55// Description:
     
    2323/*!
    2424 * \class SOPHYA::TriangleFilter
     25 \ingroup SkyT
    2526 * triangle detector response
    2627 */
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