- 17 Sep, 2013 1 commit
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Yannick Roehlly authored
So that the configuration files and the serialized data have a logical order.
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- 16 Sep, 2013 10 commits
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Yannick Roehlly authored
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Yannick Roehlly authored
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Yannick Roehlly authored
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Yannick Roehlly authored
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Yannick Roehlly authored
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Yannick Roehlly authored
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Yannick Roehlly authored
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Yannick Roehlly authored
Use sphinx with astropy _templates (it would be great to make pcigale an affilated package). Make the skeleton of the documentation. Start to write pcigale script usage.
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Yannick Roehlly authored
We follow the astropy version number scheme VERSION-RELEASE.
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Médéric Boquien authored
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- 26 Aug, 2013 1 commit
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Yannick Roehlly authored
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- 23 Aug, 2013 1 commit
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Yannick Roehlly authored
Take the Maraston 2005 models from the right page (see Readme.rst). The one we were using come from an old (but still alive) page and the Kroupa half solar metallicity SSP had a problem that was corrected around 2011. Also, we keep all the unused SSP in the "not_in_base" folder.
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- 30 Jul, 2013 1 commit
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Yannick Roehlly authored
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- 24 Jul, 2013 1 commit
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Yannick Roehlly authored
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- 11 Jul, 2013 1 commit
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Yannick Roehlly authored
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- 09 Jul, 2013 6 commits
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Yannick Roehlly authored
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Yannick Roehlly authored
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Yannick Roehlly authored
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Yannick Roehlly authored
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Yannick Roehlly authored
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Yannick Roehlly authored
In Maraston 2005 module, use Z value for metallicity (instead of log10[Z/H]) and homogenise IMF name with BC03 ones.
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- 08 Jul, 2013 2 commits
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Yannick Roehlly authored
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Médéric Boquien authored
PEP8-fication of the code and correction of various typos and spelling mistakes.
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- 06 Jul, 2013 1 commit
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Yannick Roehlly authored
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- 05 Jul, 2013 2 commits
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Yannick Roehlly authored
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Yannick Roehlly authored
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- 02 Jul, 2013 4 commits
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Yannick Roehlly authored
If the SED is redshifted, apply the redshift before checking the boundaries.
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Yannick Roehlly authored
Prepare to make it possible to get the flux in a filter without taking into account the contribution from the spectral lines.
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Yannick Roehlly authored
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Yannick Roehlly authored
Store the spectral lines in the SED as a three axis numpy array and add a method to add new sets of lines.
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- 01 Jul, 2013 4 commits
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Médéric Boquien authored
Add the necessary structures and methods to add and retrieve them from the database.
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Médéric Boquien authored
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Yannick authored
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Yannick Roehlly authored
The redshifting also lower the fluxes (that's different from the cosmological dimming). Also, simplify some methods.
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- 30 Jun, 2013 1 commit
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Yannick Roehlly authored
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- 29 Jun, 2013 1 commit
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Yannick Roehlly authored
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- 28 Jun, 2013 3 commits
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Yannick Roehlly authored
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Médéric Boquien authored
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Yannick authored
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