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Should this be left in or kept as as a separately maintained branch? It depends on how flexible the current on-the-fly magnitude calculations are. For example, could the current code be used to calculate the rest frame B band luminosity at z=0.5? If not, then probably best to keep it separate. This will involve removing it from the develop branch.
The text was updated successfully, but these errors were encountered:
I agree, however, this is working towards a public release of the code. Having everything in there named as general "magnitudes" might make many people think that the code can be used to produce any magnitudes (ie not just restricted to high redshift and/or UV). The question is then - how general is this magnitude code? Can it be used to generate K-band mags at z=0, for example?
Should this be left in or kept as as a separately maintained branch? It depends on how flexible the current on-the-fly magnitude calculations are. For example, could the current code be used to calculate the rest frame B band luminosity at z=0.5? If not, then probably best to keep it separate. This will involve removing it from the
develop
branch.The text was updated successfully, but these errors were encountered: