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The current grid of lightcurves used to train Bu2019lm (last updated to include the ultrasat filter) contains a different SDSS magnitude naming convention (e.g. sdss__u) than the sncosmo filters (e.g. sdssu).
Additionally, the Bu2019lm.pkl file on gitlab currently only contains the ultrasat filter key. Updating the file on gitlab without inducing downstream errors will require a new grid of lightcurves that has SDSS magnitudes in the sncosmo filter format.
This could be a useful test case for the model grid update workflow (#302).
The text was updated successfully, but these errors were encountered:
The current grid of lightcurves used to train
Bu2019lm
(last updated to include theultrasat
filter) contains a different SDSS magnitude naming convention (e.g.sdss__u
) than the sncosmo filters (e.g.sdssu
).Additionally, the
Bu2019lm.pkl
file on gitlab currently only contains theultrasat
filter key. Updating the file on gitlab without inducing downstream errors will require a new grid of lightcurves that has SDSS magnitudes in the sncosmo filter format.This could be a useful test case for the model grid update workflow (#302).
The text was updated successfully, but these errors were encountered: