GitLab

Allow different AGN accretion disks. We allow either the regular SKIRTOR model or the model of Schertmann (2005). In either case we also allow for a modification of the UV-optical-near-infrared slope through an extra parameter delta.

Simplify the fritz2006 module by merging the disk and the scatter component into a single disk component, following what is done for the skirtor2016 model. Some variables have also been renamed for consistency between the two AGN modules.

SED plots could not be generated for runs without a dust attenuation module as pcigale-plots sed assumed there would be one. This case is now handled.

An input redshift of integer type caused pcigale-plot sed to crash because it could not be formatted as a float. It is now explicitly converted to a float for safety.

Make sure the save_chi2 parameter is correctly acknowledged in pcigale-plots pdf. Otherwise this leads to a crash as it tries to build the PDF of parameters for which the corresponding chi2 files were not saved.

Make sure the save_chi2 parameter is correctly acknowledged in pcigale-plots pdf. Otherwise this leads to a crash as it tries to build the PDF of parameters for which the corresponding chi2 files were not saved.

Use the Einstein summation convention to avoid the creation of temporary arrays when computing the likelihood-weighted means and standard deviations. This speeds up the evaluation of the physical properties and ultimately pdf_analysis can run more than 25% faster when evaluating a large number of physical properties with more than a million models.

Add a test to ensure that we are always in a situation where we can generate a valid pcigale.ini.spec file, otherwise raise en exception.

Close #22

Handle the units for properties in log. Note that currently they cannot be saved properly in FITS files due to the format limit.

Switch the implementation to a suggestion made by Yannick. The speed is similar for small catalogues but it is substantially faster for large catalogues.

Handle the case where some bands do not have a best fit (e.g., in case the flux was not calculated because no object has a flux and the user did not add this band to the "band" parameter in pdf_analysis).

Ensure the figure is properly created and minimise the disturbance caused by the logo by placing it in the lower left corner.