IQcollaboratory / galpopFM

forward modeling galaxy populations
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SIMBA discrepancies #48

Open changhoonhahn opened 3 years ago

changhoonhahn commented 3 years ago

Compared to EAGLE and TNG, the posteriors from ABC for SIMBA had the opposite correlation with SFR. In fact, the SIMBA posteriors reversed the SFR-to-color relation --- i.e. star-forming galaxies formed the red sequence in the optical color-magnitude diagram.

Here's what happens if we take SIMBA and run the dust model with the EAGLE posteriors. I've marked in red galaxies with high SSFR image

This discrepancy seems to be driven by two factors:

changhoonhahn commented 3 years ago

I recently changed the dust model parameterization from SFR to SSFR (de247a663eba4ce7b87e6d030f70a814ce9adec7, see also #47). Even after the change in parameterization, the posterior for SIMBA reverses the relationship between SFR and color:

image

changhoonhahn commented 3 years ago

Here's an updated plot using the new SSFR parameterization: image Once star-burst galaxies are removed, SIMBA run with EAGLE posteriors have very good agreement with SDSS observations.

changhoonhahn commented 3 years ago

Updates after new SFR=0 prescription*:

Screen Shot 2020-11-09 at 10 19 15 AM

In order to reproduce the observed optical color-magnitude relation, SIMBA's starburst population requires high attenuation and steep slope, which contradicts the observed attenuation-slope relation

*in the new prescription SFR=0 galaxies are assigned SFR=SFR_min

changhoonhahn commented 3 years ago

New text added describing the discrepancy with SIMBA and how that's driven by the starburst population: https://github.com/IQcollaboratory/galpopFM/blob/abfa96ec5cbe9dfa842aa0b672a4bbe748264c8d/doc/paper/results.tex#L60