Ben Johnson

This is probably another issue with `get_best`, I suspect that the line ```py _, pbest = get_best(hf["sampling"]) ``` is returning something non-standard for pbest. I don't have time at the...

But hopefully I can dig into this in the next week or so.

You can obtain the ratio of the surviving stellar mass to the formed stellar mass from a call to predict, e.g. ```python spec, phot, mfrac = model.predict(parameter_vector, obs=obs, sps=sps) surviving_mass...

Sorry, not in general; the problem is that the ratio of surviving to formed mass is not known until the model is generated (it depends on the stellar age and...

Also to note a future update to prospector will store the ratio of the surviving to formed mass in the output.

some work on this done in c34b65a8dff

Hi @steveschulze, 1. No, sorry. You could create a branch and change https://github.com/bd-j/prospector/blob/master/prospect/sources/constants.py#L4 in your own repo and reinstall. For most cases it should make very very little difference. 2....

Hi Steve, sorry for the delay but (_gestures broadly at everything_) 3. For the nonparametric sfhs you can use `prospect.models.transforms.logsfr_ratios_to_sfrs` and then just read off the SFR of the most...

you could do something like ```python import numpy as np from scipy.special import gamma, gammainc tage, tau, mass = 2.83, 0.51, 10**10.34 # for delay tau this function gives the...

1. In principle yes, but the FSPS fortran source code has fixed wavelength gridding; the change has to be made to FSPS stellar libraries and source code. 2. set `model_params["add_dust_emission"]["init"]...