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The stored MAP spectrum in .h5 file seems to have slightly different properties compared to the one that can be reproduced by the max_theta values.
In the screenshot, the cyan photometry and blue …
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I am fitting an SED and although my fit looks good the parameters are oddly distributed (especially tage) and MCMC results look odd. I keep in general the initial parameters and priors as default exce…
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It seems to me that the `--neutrino-mass-loss-BH-formation` option is not working properly. This was first noted by Jakob Stegmann. Following a quick check on his data I agreed with his take. I then p…
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A nice feature for the next snewpy release would be a simplified interface to instantiate models. The use case is programmatically instantiating models using just the model name string plus class-spec…
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I recently had another look at f3 and wondered about conceivable extensions and applications.
### Is it possible to calibrate the C5, C16, C18 FFIs in the same way as the Kepler prime mission?
As…
gully updated
4 years ago
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**Describe the bug**
The radii of in particular massive single stars fluctuate multiple orders of magnitude in later evolution. This causes the maximum stellar radii of stars above 20 solar mass to b…
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This is related to #116.
* I think it needs to say where to get the example data. I found it here: https://github.com/OttoStruve/muler_example_data/tree/main/IGRINS/01_IGRINS_test_data
And mention…
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I am using a Mac 10.12.6, gcc 7.1.0 (but also tried with v6.3.0), and I am finding a problem when running the first instruction in prospector tutorial:
python prospector.py --param_file=demo_params…
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**Describe the bug**
Massless remnant formed in PISN has finite mass
**Label the issue**
Please label the 'severity' and 'urgency' of this issue. You can choose:
`urgency_moderate` - This is a m…
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This tutorial could use some polishing:
https://gollum-astro.readthedocs.io/en/latest/tutorials/best_fit_for_fixed_template.html
0. Some weird formatting in the first paragraph here, where you wan…