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This'll be a question for @katiebreivik.
I'm currently evolving every binary in COSMIC for 13.7 billion years - **this is not correct** given that they each have different birth times. We should ac…
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Maybe, user wants to manually set the opacity source table. It's controlled by `kap_file_prefix` for higher temperature, hydrogen-rich conditions, `kap_lowT_prefix` for low temperatures. Also there i…
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I've yet to see a clear example in screenshots or videos, but I'm assuming it is possible to provide replacement textures with PBR information.
If so, could this process (how they should be provide…
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Hi! Could you please help with the following?
I have a simple scene in Blender with one camera, one cube, and one rectangular emitter (see attached). The cube has metallicity = 1 and specular = 0,…
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@will-waalkes identified some deeply weird behavior. Sometimes, the first time `get_phoenix_photons` gets called with `wavelength=`, it seems not to be loading the correct resolution background librar…
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Hello,
In the Spatially-Resolved Mass-Metallicity Relation solution, in the Compute Stellar Mass Surface Density section, the CSV file for reading in the Firefly data for stellar mass doesn't exist…
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Hi.
1. I see that the best-fit parameters are saved in acb/*spectral_fits.csv files. Is there any existing way to export the norm obtained from the spectral fitting as a fits image? Probably like …
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__getitem__ for PHOENIXGrid is indexing in an odd fashion which causes the returned spectrum to miss teff, logg, and metallicity attributes.
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Hi, I am new to MESA, so please bear with me if this question looks too stupid.
I've been using MESA to simulate the evolution Pre-Main Sequence stars. In my project, I need to set up an initial rot…
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It would be very helpful to have the MIST grid extended to cover the oldest clusters, so essentially all the way to age of the Universe, instead of ending at 10 billion years. Would that be possible?
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