- 22 Dec, 2018 1 commit
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Rodrigo González-Castillo authored
# Conflicts: # pcigale_plots/__init__.py
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- 21 Dec, 2018 4 commits
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Rodrigo González-Castillo authored
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Rodrigo González-Castillo authored
Now it is possible to choose the folder that contains the output files (the "out" folder). It is expected that the default configuration file pcigale.ini be sibling of the "out" folder.
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Rodrigo González-Castillo authored
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Rodrigo González-Castillo authored
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- 14 Dec, 2018 5 commits
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Rodrigo González-Castillo authored
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Rodrigo González-Castillo authored
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Rodrigo González-Castillo authored
BEST_RESULTS and MOCK_RESULTS now are available in the command line options (optional)
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Rodrigo González-Castillo authored
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Rodrigo González-Castillo authored
Minor optimization in logo reading in workers. Fix logo position. Adding logging.
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- 05 Dec, 2018 1 commit
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Médéric Boquien authored
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- 29 Nov, 2018 1 commit
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Médéric Boquien authored
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- 28 Nov, 2018 2 commits
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Médéric Boquien authored
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Médéric Boquien authored
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- 08 Nov, 2018 2 commits
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Médéric Boquien authored
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Médéric Boquien authored
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- 07 Nov, 2018 4 commits
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Médéric Boquien authored
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Médéric Boquien authored
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Yannick Roehlly authored
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- 06 Nov, 2018 8 commits
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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
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Médéric Boquien authored
Add pseudo filters to measure Halpha, Hbeta, and OIII. Beware that the fluxes will be affected by any underlying absorption line. Also make sure that the continuum part of the filter is not significantly affected by emission lines. It is recommended to adapt the filter depending on the actual resolution of the spectral observations.
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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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- 22 Oct, 2018 3 commits
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Médéric Boquien authored
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Médéric Boquien authored
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Médéric Boquien authored
Add the sfhdelayedbq module implementing a delayed SFH with a burst/quench. It is described in detail in Ciesla et al. (2017).
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- 19 Oct, 2018 4 commits
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Médéric Boquien authored
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Médéric Boquien authored
Make sure that the best fit can be computed when the redshift is estimated rather than given as an input.
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Médéric Boquien authored
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Médéric Boquien authored
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- 19 Sep, 2018 3 commits
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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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- 18 Sep, 2018 2 commits
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Médéric Boquien authored
Add the possibility of computing emission lines through special filters when underlying absorption lines are not subtracted.
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Médéric Boquien authored
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