diff --git a/doc/source/_static/logo-cyfronet.png b/doc/source/_static/logo-cyfronet.png new file mode 100644 index 0000000..69573f8 --- /dev/null +++ b/doc/source/_static/logo-cyfronet.png diff --git a/doc/source/_static/logo-desy.png b/doc/source/_static/logo-desy.png new file mode 100644 index 0000000..28929fc --- /dev/null +++ b/doc/source/_static/logo-desy.png diff --git a/doc/source/_static/logo-ecap.jpg b/doc/source/_static/logo-ecap.jpg new file mode 100644 index 0000000..80f8114 --- /dev/null +++ b/doc/source/_static/logo-ecap.jpg diff --git a/doc/source/_static/logo-irap.png b/doc/source/_static/logo-irap.png new file mode 100644 index 0000000..a6d04e4 --- /dev/null +++ b/doc/source/_static/logo-irap.png diff --git a/doc/source/_static/logo-lapp.png b/doc/source/_static/logo-lapp.png new file mode 100644 index 0000000..dd25bea --- /dev/null +++ b/doc/source/_static/logo-lapp.png diff --git a/doc/source/_static/logo-lupm.png b/doc/source/_static/logo-lupm.png new file mode 100644 index 0000000..8ce26ee --- /dev/null +++ b/doc/source/_static/logo-lupm.png diff --git a/doc/source/_static/logo-mpik.png b/doc/source/_static/logo-mpik.png new file mode 100644 index 0000000..58605dc --- /dev/null +++ b/doc/source/_static/logo-mpik.png diff --git a/doc/source/_templates/index.html b/doc/source/_templates/index.html index 1ee65ce..96b2666 100755 --- a/doc/source/_templates/index.html +++ b/doc/source/_templates/index.html @@ -16,14 +16,35 @@ is supported as well. {%endtrans%}
{%trans%} ctools are based on GammaLib, a versatile toolbox for the scientific analysis of astronomical gamma-ray data. Besides CTA, GammaLib supports the analysis of H.E.S.S., MAGIC, VERITAS, -Fermi/LAT, COMPTEL and INTEGRAL/SPI data. GammaLib supports in particular the +Fermi/LAT, CGRO/COMPTEL and INTEGRAL/SPI data. GammaLib supports in particular the combination of data from different instruments in a true joint multi-wavelength analysis that consistently handles the response of each instrument. An interface -to virtual observatory ressources does also exist. +to virtual observatory resources does also exist. {%endtrans%}
-{%trans%} ctools are developed by a team of enthousiastic gamma-ray -astronomers with support from engineers. We regularily organise +
{%trans%} ctools are developed by a community of enthousiastic gamma-ray +astronomers with support from engineers. The lead institute is
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As of today there have been contributions by the following institutions:
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We regularily organise coding sprints where key developers but also newcomers meet to discuss the developments and next steps, and advance with the coding of the software. diff --git a/doc/source/about.rst b/doc/source/about.rst index d67ecd3..bd73d07 100755 --- a/doc/source/about.rst +++ b/doc/source/about.rst @@ -16,11 +16,11 @@ Creation of shell or Python scripts and pipelines is supported as well. ctools are based on GammaLib, a versatile toolbox for the scientific analysis of astronomical gamma-ray data. Besides CTA, GammaLib supports the analysis of H.E.S.S., MAGIC, VERITAS, -Fermi/LAT, COMPTEL and INTEGRAL/SPI data. +Fermi/LAT, CGRO/COMPTEL and INTEGRAL/SPI data. GammaLib supports in particular the combination of data from different instruments in a true joint multi-wavelength analysis that consistently handles the response of each instrument. -An interface to virtual observatory ressources does also exist. +An interface to virtual observatory resources does also exist. ctools are developed by a team of enthousiastic gamma-ray astronomers with support from engineers. We regularily organise