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We do not want to just mask when there is a division by zero. That's the wrong thing to do here. There will be a physical reason that there is no HI, and in the real universe we wouldn't be able to measure the HI in those galaxies - so we should cut by that physical reason (e.g. just plot for star forming galaxies in a given mass range).
The data in several cold-gas-fractions plots may have
NaN
values (depending on the run and redshift), which makes the pipeline crash in certain cases.E.g.
sigma_h2_to_neutral_H_fraction_100
Possible solution: always use
mask
whenever there is a change to have division by zero.The text was updated successfully, but these errors were encountered: