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If no Fe II lines (or if Teff from H-line?): Determine logg from an isochrone given the temperature, propagating temperature uncertainties.
User should input the isochrone (age, metallicity) and ADS …
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Mario has called out equation 80 of Hurley. The factor of 0.1 is not going to be a good factor when we integrate with CMC. We instead should make this a flag (yay flags) that can be set by the user.
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My python version is: Python 2.7.11 :: Anaconda 4.0.0 (x86_64)
I am having trouble with latex and pyp-beagle. Do I need a special package? For instance, if in the .json file I use:
"tauv_eff": {
"r…
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When fitting photometry with fixed Ha flux, I got this error:
[ERROR: Parameter `hbaa@6563` does not correspond to any physical parameter ]
[FUNCTION: "change_galaxy_parameters" ]
[MODULE: "par…
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Hi @timothydmorton, I have a suggestion for the [interpolation section](https://isochrones.readthedocs.io/en/latest/modelgrids.html#Background-and-EEPs) of the docs. Could you provide an example of ho…
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While diving into #195, I found some really wonky stuff is going on with the calculation of the AGB core mass in hrdiag.f. This is causing PISN to _never_ happen, since the core masses that are calcul…
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Cosmic does not warn/restrict initial conditions that start the binary evolution in RLOF. These binaries are evolved normally even though they have unrealistic initial conditions.
I found these bi…
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Someone (probably me): start a 2019 production run in the example folder. Everyone can look at the `datamodel` file to converge on a set of parameters (ASTs, grid spacing, etc) that we like. Discuss…
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I used Prospector-alpha model (2018) to fit 151 galaxies from COSMOS. The stellar mass results are quite larger compare to COSMOS results, overall by 0.5 index. I also compare my results to MAGPHYS+A…
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Hi,
It seems that we discovered a bug in the cooling at high redshift (before the reionization). When running a cosmological simulation, the cooling converges to a heating at 1000 K if the initial …