- Implementation of the auto-detection of lines in the input flux file so they are automatically added to the list of bands in `pcigale.ini`. (Médéric Boquien)
- The `dl2007` and `dl2014` modules now provide \<U\>. (Médéric Boquien)
- Saving the χ² is now a bit more fine-grained. It is possible to save none, all, only the properties, or only the fluxes. (Médéric Boquien)
- The database now includes the JWST MIRI and NIRCam filters. (Médéric Boquien)
### Changed
- Python 3.6 is now the minimum required version. (Médéric Boquien)
- The logo has now been moved to the lower-right corner of the figure so that it does not overlap with any information and it has been updated for a less pixelated version. (Médéric Boquien & Rodrigo González Castillo)
# Includes Nominal transmission of the JWST OTE is not included. Source: http://svo2.cab.inta-csic.es/svo/theory/fps3/index.php?mode=browse&gname=JWST&gname2=MIRI
# Includes Nominal transmission of the JWST OTE is not included. Source: http://svo2.cab.inta-csic.es/svo/theory/fps3/index.php?mode=browse&gname=JWST&gname2=MIRI