- Read object redshift from the Beagle output file, so that pyp_beagle correctly deals with redshifts when provided in the prior catalogue; correctly plots masked regions read from the 'MARGINAL SED MASK' extension - Correctly identify object ID from Beagle output file name - Cosmetics improvements to the marginal photometry plot
0.6.4
- Introduced option to overplot on a photometric SED the maximum-a-posteriori (MAP) spectrum - Exploiting the *args and **kwargs appraoches to simplify the passing of command-line arguments to the different classes
0.6.3
- Bug fix: file names of spectra and object IDs were not correctly matched
0.6.2
- Correctly dealing with lines not observed (i.e. negative fluxes and errors in the observed catalogue)
0.6.1
- Implemented option to print the values of observed and model fluxes on the plot - Removed unused function - Changed parser variable name - Cosmetics: added dotted lines linking symbols in the plot to the line labels on the x-axis
0.6.0
- Merge branch 'feature/spectral_indices' into develop - Added SpectralIndices module - Finished integration of module to plot spectral indices (integrated line fluxes and EWs) - Added option to print values of line fluxes in the output image - Started integrating the new 'SpectralIndices' class in the main module - Started implementing the new module to post-process fitting to spectral indices / integrated fluxes / EWs - Using the new class 'ObservedCatalogue' - Added new module containing a generic 'observed catalogue' - Changed mail address - Removed support for python 2.6