- 20 Feb, 2014 8 commits
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Médéric Boquien authored
Remove the possibility to use the same module several times. Simplification of the code ensues. Now sed.info keys are prefixed with the characteristic of the module (stellar, nebular, etc.).
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Yannick authored
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Médéric Boquien authored
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Yannick Roehlly authored
glob is imported in the pcigale/session/configuration.py to allow its use in the configuration file (with eval). TODO: write a new configuration pattern to add several files with something like "files *.fits".
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Médéric Boquien authored
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Médéric Boquien authored
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Médéric Boquien authored
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Médéric Boquien authored
Implement the nebular continuum emission. This has required some refactoring to have some homogeneous naming.
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- 19 Feb, 2014 14 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
There is maybe a bug triggering the display of the best model figure in a matplotlib interactive window.
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Yannick Roehlly authored
Use a simplified gaussian kernel density estimation for computing the probability density functions.
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Médéric Boquien authored
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Médéric Boquien authored
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Médéric Boquien authored
Update with Inoue's latest models computed with a BC03 stellar continuum. 124 lines are now included from the FUV to the FIR.
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Yannick Roehlly authored
The team will use the projets.lam.fr issue tracker instead.
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Yannick Roehlly authored
Modification to savefluxes to have all the contenct of the sed.info dictionary in the output table. That means that all the SED created with the modules must have the same sed.info keys.
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Yannick Roehlly authored
For a given observation, taking the least chi-square or the least reduced chi-square is the same thing.
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Médéric Boquien authored
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Médéric Boquien authored
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- 18 Feb, 2014 5 commits
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Yannick Roehlly authored
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Yannick Roehlly authored
Start of the rewrite of the psum analysis module in pdf_analysis. The computation is made avoiding loops by using numpy multidimensional arrays.
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Médéric Boquien authored
Use np.max/np.min instead of the built-in functions. This results in a factor ~2 speedup to compute the fluxes.
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Yannick Roehlly authored
Maybe we should change the name.
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Yannick Roehlly authored
To make it easy to save the best models table.
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- 17 Feb, 2014 3 commits
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Yannick Roehlly authored
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Yannick Roehlly authored
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Médéric Boquien authored
Factor 2 speedup to compute the IGM attenuation. This is done by doing some computations only on the part of the SED actually affected by the IGM. This could still be improved.
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- 16 Feb, 2014 1 commit
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Yannick Roehlly authored
Add redshifting and IGM attenuation modules (make psum use them). Remove atpy dependency and use astropy instead. Some modification to make the code Python 3 compatible.
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- 14 Feb, 2014 7 commits
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Yannick Roehlly authored
Correction of a problem spotted by Médéric, basestring does not exists in Python 3.
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Médéric Boquien authored
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Médéric Boquien authored
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Médéric Boquien authored
Make the source code more compatible with Python 3. As far as I understand the documentation, this should be harmless for Python 2.
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Yannick Roehlly authored
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Médéric Boquien authored
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Médéric Boquien authored
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- 13 Feb, 2014 2 commits
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Yannick Roehlly authored
and remove old igmattenuation code.
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Yannick Roehlly authored
Implementation of one module for the redshifting and one for the IGM attenuation. For now, the IGM module only implements the Meskin (2006) attenuation; alternative attenuation law can be added with a parameter in the module to choose which one to apply.
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