Commit 26a627b093bd1fd4412f86237f602cbff85eeef0
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Remove home file and update GammaLib introduction text.
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doc/source/_templates/index.html
| @@ -16,16 +16,32 @@ body %} | @@ -16,16 +16,32 @@ body %} | ||
| 16 | abstract data analysis framework that enables simultaneous | 16 | abstract data analysis framework that enables simultaneous |
| 17 | multi-mission analysis. {%endtrans%}</p> | 17 | multi-mission analysis. {%endtrans%}</p> |
| 18 | 18 | ||
| 19 | +<p>{%trans%} GammaLib does not rely on any third-party software, except | ||
| 20 | +of HEASARC's cfitsio library that is used to implement the FITS interface. | ||
| 21 | +Large parts of the code treat gamma-ray observations in an abstract | ||
| 22 | +representation, and do neither depend on the characteristics of the | ||
| 23 | +employed instrument, nor on the particular formats in which data and | ||
| 24 | +instrument response functions are delivered. Instrument specific | ||
| 25 | +aspects are implemented as isolated and well defined modules that | ||
| 26 | +interact with the rest of the library through a common interface. This | ||
| 27 | +philosophy also enables the joint analysis of data from different | ||
| 28 | +instruments, providing a framework that allows for consistent | ||
| 29 | +broad-band spectral fitting or imaging. So far, GammaLib supports | ||
| 30 | +analysis of COMPTEL, Fermi/LAT, and Cherenkov telescope data | ||
| 31 | +(CTA, H.E.S.S., MAGIC, VERITAS). {%endtrans%}</p> | ||
| 32 | + | ||
| 33 | +<p>{%trans%} GammaLib is free software distributed under the | ||
| 34 | +<a href="http://www.gnu.org/licenses/gpl.html">GNU GPL license version 3</a> {%endtrans%}</p> | ||
| 35 | + | ||
| 19 | <h2 style="margin-bottom: 0">{%trans%}Documentation{%endtrans%}</h2> | 36 | <h2 style="margin-bottom: 0">{%trans%}Documentation{%endtrans%}</h2> |
| 20 | 37 | ||
| 21 | <ul> | 38 | <ul> |
| 22 | -<li><a class="smalllink" href="{{ pathto("home") }}">{%trans%}What is GammaLib?{%endtrans%}</a></li> | ||
| 23 | <li><a class="smalllink" href="{{ pathto("installation") }}">{%trans%}Installation{%endtrans%}</a></li> | 39 | <li><a class="smalllink" href="{{ pathto("installation") }}">{%trans%}Installation{%endtrans%}</a></li> |
| 24 | <li><a class="smalllink" href="{{ pathto("quickstart") }}">{%trans%}Quickstart{%endtrans%}</a></li> | 40 | <li><a class="smalllink" href="{{ pathto("quickstart") }}">{%trans%}Quickstart{%endtrans%}</a></li> |
| 25 | <li><a class="smalllink" href="{{ pathto("user_manual/index") }}">{%trans%}User Manual{%endtrans%}</a></li> | 41 | <li><a class="smalllink" href="{{ pathto("user_manual/index") }}">{%trans%}User Manual{%endtrans%}</a></li> |
| 26 | <li><a class="smalllink" href="{{ pathto("develop") }}">{%trans%}Developing GammaLib{%endtrans%}</a></li> | 42 | <li><a class="smalllink" href="{{ pathto("develop") }}">{%trans%}Developing GammaLib{%endtrans%}</a></li> |
| 27 | <li><a class="smalllink" href="{{ pathto("coding/index") }}">{%trans%}Coding conventions{%endtrans%}</a></li> | 43 | <li><a class="smalllink" href="{{ pathto("coding/index") }}">{%trans%}Coding conventions{%endtrans%}</a></li> |
| 28 | -<li><a class="smalllink" href="doxygen/index.html">{%trans%}Code documentation{%endtrans%}</a></li> | 44 | +<li><a class="smalllink" href="doxygen/index.html">{%trans%}Code documentation (Doxygen){%endtrans%}</a></li> |
| 29 | </ul> | 45 | </ul> |
| 30 | 46 | ||
| 31 | <h2 style="margin-bottom: 0">{%trans%}Links{%endtrans%}</h2> | 47 | <h2 style="margin-bottom: 0">{%trans%}Links{%endtrans%}</h2> |
doc/source/contents.rst
doc/source/home.rst deleted
| 1 | -Home | ||
| 2 | -==== | ||
| 3 | - | ||
| 4 | -GammaLib is a self-contained, instrument independent, open source, | ||
| 5 | -multi-platform C++ library that implements all code required for | ||
| 6 | -high-level science analysis of astronomical gamma-ray data. GammaLib is | ||
| 7 | -also wrapped into a Python module. | ||
| 8 | - | ||
| 9 | -GammaLib does not rely on any third-party software, except of HEASARC's | ||
| 10 | -cfitsio library that is used to implement the FITS interface. Large | ||
| 11 | -parts of the code treat gamma-ray observations in an abstract | ||
| 12 | -representation, and do neither depend on the characteristics of the | ||
| 13 | -employed instrument, nor on the particular formats in which data and | ||
| 14 | -instrument response functions are delivered. Instrument specific | ||
| 15 | -aspects are implemented as isolated and well defined modules that | ||
| 16 | -interact with the rest of the library through a common interface. This | ||
| 17 | -philosophy also enables the joint analysis of data from different | ||
| 18 | -instruments, providing a framework that allows for consistent | ||
| 19 | -broad-band spectral fitting or imaging. So far, GammaLib supports | ||
| 20 | -analysis of COMPTEL, Fermi-LAT, and Cherenkov telescope data (H.E.S.S., MAGIC, CTA). | ||
| 21 | - | ||
| 22 | -GammaLib is free software distributed under the | ||
| 23 | -`GNU GPL license version 3 <http://www.gnu.org/licenses/gpl.html>`_ | ||
| 24 | \ No newline at end of file | 0 | \ No newline at end of file |