- 16 Sep, 2013 3 commits
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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 6 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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Yannick Roehlly authored
The process method was used to complete and check the parameter dictionary before launching the _process one defined in each module. Now that the parameters are dealed with at instantiation, this separation is no more useful. Also, modify the attenuation modules to read the filter in the database at instantiation.
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Yannick Roehlly authored
In order to speed-up module re-use, get the module needs (ssp, filters...) out of pcigale database at module instantiation instead of doing this everytime "process" is called. To do that: - we must give the module parameters (and proceed with their checking) at module instantiation. - we must add the possibility for each module to have its own initialisation code. In addition, to create the configuration file, we must be able to load the modules without any parameter to query them for their parameter list. The bc03, dh2002 and m2005 modules were changed to use this new behavior.
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Médéric Boquien authored
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- 27 Jun, 2013 3 commits
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Yannick Roehlly authored
To avoid problems that might occur when, for instance, using an integer instead of a float, we now cast the module parameters to their expected type. This will also have the advantage to raise an error when a parameter can't be interpreted with its expected type. Also, use integer for age parameters as we are now using Myr as unit.
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Yannick Roehlly authored
Thanks to Médéric Boquien. The normalisation factor must take into account the error associated with each filter flux.
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Yannick Roehlly authored
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- 25 Jun, 2013 1 commit
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Yannick Roehlly authored
Thanks to Médéric Boquien.
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- 17 Jun, 2013 1 commit
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Yannick Roehlly authored
It's a dictionnary to hold the spectral lines associated with the SED. We use a disctionnary to be able to differentiate several sets of lines (e.g. lines from old and young populations). TODO: Complete the code to add the line contributions to the integrated flux.
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