- 14 Dec, 2018 3 commits
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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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- 08 Nov, 2018 1 commit
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Médéric Boquien authored
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- 07 Nov, 2018 1 commit
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Yannick Roehlly authored
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- 06 Nov, 2018 7 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
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 9 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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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
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Médéric Boquien authored
Have the nebular module compute and store the intrinsic line luminosities. That way they can be fitted as any flux.
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Médéric Boquien authored
Store the name of the individual lines in the database in order so they can easily be identified and retrieved.
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- 27 Jun, 2018 1 commit
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Médéric Boquien authored
Clarify a bit the description of the redshifting module as we do not always just fit a single galaxy
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- 09 May, 2018 7 commits
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Médéric Boquien authored
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Médéric Boquien authored
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Médéric Boquien authored
Completely change the SED cache. Now we rely on the fact that for a given set of modules we only need to store only one model in cache. If there is a cache miss, it means we can discard this one model. In turn the cache key simply becomes the number of modules used, making it easier and faster to access. To check whether the stored module corresponds to the requested one, we store both the model parameters and the SED in a tuple.
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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
Avoid making a copy when storing the redshifted SED. This SED will never be modified. This is done by copying what is returned by get_sed rather than having get_sed return directly a copy.
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- 02 May, 2018 1 commit
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Médéric Boquien authored
Do display the model counter twice when the numbers of models is a multiple of the printing frequency.
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