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Separate MS params and Satellite specific quenching #51
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…rameters for qseq and mseq galaxies, without offdiagonal covariance elements, and with separate quenching parameters for centrals and satellites.
… to maximize the number of haloes that can be fit at once
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Here are the results for SMDPL. To be compared with:
This is the best version so far, and for the first time we get good sSFR distribution for low mass galaxies at z=0, for both centrals and satellites. The loss function value is also clearly the lowest (20% better) than previous best results. |
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Similarly, here are the results for TNG. To be compared with:
The improvements in this case are not so significant. The sSFR of satellites for low mass galaxies at z=0 also get better, but the other differences remain. |
…py so that mc_diffstarpop_tpeak_sepms_satfrac is used instead of mc_diffstarpop_tpeak
…s.py still fails because u_lgmu_lo_mh_hi parameter has zero gradient
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@alexalar I fixed some bugs in the last few commits. The reason the current PR checks fail is because the |
… the best fit params to SMDPL no merging data








This PR combines the model updates from #49 and #48, adding separate main sequence parameters for mseq and qseq galaxies, and also adding an independent
frac_quenchsigmoid function for centrals and satellites.