- 24 May, 2015 1 commit
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Médéric Boquien authored
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- 22 May, 2015 3 commits
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Médéric Boquien authored
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Médéric Boquien authored
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Médéric Boquien authored
Homogeneize the attenuation modules with the latest changes regarding the way we handle filters in compute_fnu(). Also make sure we do not request the key from the filter list as it is not a dictionary anymore.
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- 21 May, 2015 2 commits
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Médéric Boquien authored
Implement a cache for the computation of the optimal grid when merging two grids. As the best_grid() function takes numpy arrays as arguments, it makes caching difficult as they are not hashable. To solve the problem we define a helper function to do the memoisation based on the size, min, and max values of each of the input arrays.
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Médéric Boquien authored
Implement a cache for the filters to compute the fluxes. Rather than passing the transmission table as an argument to compute_fnu(), which makes caching difficult and/or slow to compute the hash, we rather pass the filter name. Then the SED object fetches the filter from the database and resamples it on the optimal wavelength grid. The result is stored in cache to avoid carrying out this operation repeatedly.
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- 20 May, 2015 9 commits
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Médéric Boquien authored
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Médéric Boquien authored
Implement the nebular lines over 9 points in wavelength rather than 19. It barely changes anything to the results and it speeds up the computation by 20%.
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Médéric Boquien authored
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Médéric Boquien authored
Plot only to λ=50 cm as the models do not extend much further and there is very rarely any observation beyond λ=21 cm.
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Médéric Boquien authored
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Médéric Boquien authored
As there should never be an sfh.age in sed.info when we add it, remove the option to force an update. Better to stop as it shows there is something wrong going on.
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Médéric Boquien authored
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Médéric Boquien authored
Display the model fluxes on top of the spectrum. Otherwise the dots can be partially masked by the spectrum.
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Médéric Boquien authored
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- 19 May, 2015 4 commits
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Médéric Boquien authored
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Médéric Boquien authored
Chnage the nebular_lines_width parameter to lines_width. Given that we prefix with the module type (here nebular) for output parameters, nebular was just redundant.
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Médéric Boquien authored
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Médéric Boquien authored
Correct two issues that caused plots to display an offset spectrum when redshifts were given with more than 2 decimals. First round the redshift to two decimals. Then, rather than recomputing the luminosity distance, let's just take the one from the best models file.
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- 28 Apr, 2015 5 commits
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Yannick Roehlly authored
Corrections to release v0.5 - Inclusion of the pcigale-plots data. - Better information in setup.py
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Yannick Roehlly authored
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Yannick Roehlly authored
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Yannick Roehlly authored
Note that include_package_data is not necessary.
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Yannick Roehlly authored
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- 24 Apr, 2015 7 commits
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BURGARELLA Denis authored
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BURGARELLA Denis authored
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BURGARELLA Denis authored
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BURGARELLA Denis authored
Update CIGALE to clean anything related to 'average_sfr' and replace it by 'sfr10Myrs' and 'sfr100Myrs'
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BURGARELLA Denis authored
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BURGARELLA Denis authored
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BURGARELLA Denis authored
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- 06 Apr, 2015 2 commits
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BURGARELLA Denis authored
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BURGARELLA Denis authored
change agn_fritz2006_therm to agn.fritz2006_therm to test if we need to plot the AGN emission (correction of bug)
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- 02 Apr, 2015 7 commits
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Yannick Roehlly authored
Release v0.5
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Yannick Roehlly authored
Denis added some corrections for the plots.
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BURGARELLA Denis authored
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BURGARELLA Denis authored
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Yannick Roehlly authored
Release version 0.4
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Yannick Roehlly authored
Release of version 0.4.
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Yannick Roehlly authored
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