Each folder corresponds, roughly, to a section in the paper.
Takes all the data from several papers and writes it down to a single table (using astropy Tables).
The main output files are:
data_corrected_MW_ext.dat: emission line fluxes corrected by the Milky Way extinction
galaxy_properties.dat: mass, SFR, Te and others from the literature for this sample
Here we calculate the electron temperature and correct for dust in Te_and_Dereddening.ipynb and then use this to calculate the direct metallicity in TeMetallicity.ipynb
The main output files are:
data_Te.dat: with the electron temperature and attenuation for each galaxy
data_dered.dat: dust corrected emission line fluxes
Comparison of the metallicity derived using the direct method and the strong line calibrations.