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Using a list to keep the information keys that are proportional to the
mass leads to problems when forcing the update of a proportional
information: the key name appears then twice (or more) in the list and
the information is multiplied twice (or more) by the mass.

Note that include_package_data is not necessary.

Update CIGALE to clean anything related to 'average_sfr' and replace it by 'sfr10Myrs' and 'sfr100Myrs'

change agn_fritz2006_therm to agn.fritz2006_therm to test if we need to plot the AGN emission (correction of bug)

Release v0.5

Denis added some corrections for the plots.

Release version 0.4

Release of version 0.4.

Resample the m2005 stellar models at long wavelengths. The reason is that as the sampling is too sparse, the linear interpolation carried out in cigale creates waves that are not only disgracious but that also artificially boost the broadband fluxes flux. Patch based on previous commit that fixed the same issue for the bc03 models.

Resample the bc03 stellar models at long wavelengths. The reason is that as the sampling is too sparse, the linear interpolation carried out in cigale creates waves that are not only disgracious but that also artificially boost the broadband fluxes flux.

Last (?) modification of the Fritz 2006 parameters. The opening angle is in agreement with Fig. 1 in Fritz (2006). The viewing angle is in agreement with Hatziminaoglou (2008) and Fritz (2010) models.

Large revamp of the SED plotting procedure by Denis and I. Among the main changes: 1. option to plot in mJy in observed frame or un luminosity in rest frame 2. different components are now plotted automatically 3. a logo is now diplayed but can be removed with an option.

Commit Denis' change to make sure that pcigale-plots does not crash when pcigale did not find a best fit.

Add a carriage return after we have computed the last model or analysed the last object so that the information does not get erased.

Add the IRAS, SCUBA and VLA filters from Barbara.

Add some filters from Barbara.

The "galaxy_mass" parameter must not be set to 1.0 in the stellar
emission modules because when using CIGALE to generate SED without
normalising the 1.0 is wrong and misleading.

Instead, we compute the real galaxy mass (the integration of the SFH) in
the star formation history modules.