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This PR tests what happens if you have independent main sequence parameters for quenched and main sequence galaxies.

The fits improve considerably. I think this, coupled with independent frac_quench parameters for centrals and satellites will proabably yield a great, final model.

These plots for SMDPL should be compared to #46.

smhm_logsm
pdf_mstar
pdf_ssfr_centrals
pdf_ssfr_satellites

…ers for mainseq and qseq galaxies. Offdiagonals of covariances are set to zero, too
@alexalar
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And here similarly for TNG, to be compared to #47.

Here fits don't improve so much, again, like it happened in #48.

smhm_logsm
pdf_mstar
pdf_ssfr_centrals
pdf_ssfr_satellites

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2 participants