- 19 Nov, 2015 3 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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- 18 Nov, 2015 4 commits
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Médéric Boquien authored
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Médéric Boquien authored
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BURGARELLA Denis authored
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BURGARELLA Denis authored
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- 17 Nov, 2015 1 commit
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Médéric Boquien authored
Simplify and streamline the production of mock plots. Now just output one plot per file and do so in parallel. Also output in log when it seems to make sense.
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- 10 Nov, 2015 1 commit
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Médéric Boquien authored
When the flux file contains a mix of spaces and tabulations as column separators, pcigale discards the header and takes the first data line as the header. Now pcigale properly handles such a combination. Bug reported by Paola Santini.
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- 06 Nov, 2015 3 commits
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Yannick Roehlly authored
Actually raise an exception indicating to the users to change their parameters if the quenching age happens to be superior to the galaxy age. Fixes #2
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Yannick Roehlly authored
A dummy parameter was used in param because a parameterless module is not possible. Now that we have the list of filters, we can remove it.
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Yannick Roehlly authored
Using the param module, if the list of filters is empty, no flux will be computed and the module won't complain about '' missing filter. Also, switch the default value for this list of filters to the empty string, because None means that there is no default value which makes the module not usable without the list for filters parameters. Closes #5
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- 05 Nov, 2015 1 commit
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Yannick Roehlly authored
The luminosity table is also used when plotting Fluxes to access the various components.
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- 04 Nov, 2015 7 commits
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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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Médéric Boquien authored
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Médéric Boquien authored
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Médéric Boquien authored
Ensure that the Lyman continuum emission is properly absorbed by the gas in the nebular module. This means that without that module, the Lyman continuum is left untouched. As this may be an issue for people used to running without the nebular module (assuming that the flux in individual bands in small), add an option to only absorb the Lyman continuum while discarding any nebular emission.
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Médéric Boquien authored
Implement a simple verification of the list of modules to warn the user if some mandatory modules are missing.
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- 02 Nov, 2015 2 commits
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Médéric Boquien authored
Remove the radio component from the dale2014 model so that it can be used with the more flexible radio module, courtesy Daniel Dale
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Médéric Boquien authored
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- 01 Nov, 2015 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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- 26 Oct, 2015 1 commit
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Médéric Boquien authored
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- 25 Oct, 2015 1 commit
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Médéric Boquien authored
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- 23 Oct, 2015 2 commits
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BURGARELLA Denis authored
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BURGARELLA Denis authored
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- 22 Oct, 2015 1 commit
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BURGARELLA Denis authored
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- 17 Oct, 2015 1 commit
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Médéric Boquien authored
Handle the case where we do not know the redshift to estimate the physical parameters by taking all models at all redshifts. This means that in effect pcigale can also act as a photo-z code now on.
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- 16 Oct, 2015 5 commits
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Médéric Boquien authored
Now that we leave the models with NaN fluxes, the scaling factors and χ² may be NaN too. Handle this case.
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Médéric Boquien authored
The galaxy_mass parameter confuses a lot of people. Change its name to sfh.integrated because it is actually the integral of the SFR.
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Médéric Boquien authored
Add an _init_code() to sfh2exp to avoid repeating twice the same operations. Even though that should not be a common occurrence, it is cleaner by separating the computation of the data and the actual processing of the SED object.
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Médéric Boquien authored
The SSPs in the database are always built on a time grid with 1 Myr time steps. No need to drag around a constant for this as it will stay that way for the forseeable future.
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Médéric Boquien authored
By construction the SFH in cigale is a comb. Every 1 Myr stars are formed. All at the same time. In effect star formation is not continuous. This means that we should not use trapz to integrate the SFR or use an analytic relation. Rather we just sum, which is correct for the discrete nature of the SFH.
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- 15 Oct, 2015 1 commit
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Yannick Roehlly authored
Rename the SED info dictionary key for the AGN faction added by dale2014 module from agn.fracAGN to agn.fracAGN_dale2014 to avoid conflict with fritz2006 module.
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- 14 Oct, 2015 1 commit
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Médéric Boquien authored
Avoid multiply the array by a scalar once rather than twice. It makes the computation quite a bit faster.
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- 13 Oct, 2015 1 commit
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Médéric Boquien authored
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- 12 Oct, 2015 1 commit
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Médéric Boquien authored
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