- 14 Feb, 2014 4 commits
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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 3 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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Yannick Roehlly authored
Extend the Calzetti-Leitherer with the Leitherer formula below 91.2 nm. Maybe we should made the attenuation even stronger there. Stop cutting the Maraston 2005 SSP below 91.2 nm.
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- 12 Feb, 2014 2 commits
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Yannick Roehlly authored
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Yannick Roehlly authored
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- 11 Feb, 2014 2 commits
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Yannick Roehlly authored
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Yannick Roehlly authored
Move the igmattenuation module and its LSST dependencies inside the psum analysis module. Remove the redshift_module and redshift_configuration parts of the configuration file.
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- 02 Feb, 2014 1 commit
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Yannick Roehlly authored
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- 31 Jan, 2014 1 commit
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Yannick Roehlly authored
Making glob() available in session/configuration.py allows users of savefluxes and sfhfromfile to use something like filename = "eval glob('sfh*.fits')" sfr_column = 2 to take the star formation history from several files.
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- 30 Jan, 2014 2 commits
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Yannick Roehlly authored
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Yannick Roehlly authored
Create two custom exceptions. When one tries to insert something in the database that is already inside, a DatabaseInserError is raised. When one asks for something in the database that is not present, a DatabaseLookupError is raised indicating what was not found.
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- 29 Jan, 2014 3 commits
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Yannick Roehlly authored
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Yannick Roehlly authored
Now the redshift is an attribute of the SED. The SED.compute_fnu() no longuer takes redshift and apply_redshift arguments as the SED is supposed to be redshifted. The SED.lambda_fnu() method was converted to the SED.fnu property returning th Fν flux density at each wavelength of the wavelength grid.
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Yannick Roehlly authored
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- 21 Jan, 2014 1 commit
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Yannick Roehlly authored
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- 15 Jan, 2014 1 commit
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Yannick Roehlly authored
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- 13 Jan, 2014 1 commit
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Yannick Roehlly authored
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- 11 Jan, 2014 5 commits
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Yannick Roehlly authored
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Yannick Roehlly authored
Remove the author email addresses from the source files and add a AUTHORS.rst file with the addresses and current affiliation to make it easier to update the information. Also, give copyright to the University of Cambridge and the University of Crete for code developed by authors working there.
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Yannick Roehlly authored
Export the bugs-everywhere content to HTML in bugs directory to allow an easy read-only view of bug list.
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Yannick Roehlly authored
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BURGARELLA Denis authored
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- 10 Jan, 2014 1 commit
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Yannick Roehlly authored
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- 27 Dec, 2013 1 commit
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Yannick Roehlly authored
It will make the documentation clearer.
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- 26 Dec, 2013 4 commits
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Yannick Roehlly authored
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Yannick Roehlly authored
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Yannick Roehlly authored
For the creation and analysis modules, move the contents of the common.py files to the __init__.py.
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Yannick Roehlly authored
Move the SED creation modules to pcigale.creation_modules to be more consistent with the analysis module location.
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- 09 Dec, 2013 3 commits
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Yannick Roehlly authored
The quasar contributions must contain the name of the attenuation used because using several attenuations will lead to a key error when adding the second quasar contribution.
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Yannick Roehlly authored
Class name should be CamelCased, arguments and variable inside functions should be lower case. There's no need to put my name in authors when I did not do anything. Use the new post-fixed key names for contributions.
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Laure Ciesla authored
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- 03 Dec, 2013 1 commit
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Yannick Roehlly authored
Manage the bugs / todo with bugs-everywhere [1]. It's less readable but can export fancy HTML lists. [1] http://www.bugseverywhere.org/
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- 29 Nov, 2013 3 commits
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Yannick Roehlly authored
astropy v0.3 cosmology methods now returns quantities. We keep only the value to avoid problems in numpy computations.
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Yannick Roehlly authored
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Yannick Roehlly authored
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- 26 Nov, 2013 1 commit
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Médéric Boquien authored
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