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Right now, our default is to do linear interpolation in composition (X,Z) for opacity tables. Even though cubic interpolation returns more realistic opacities, it returns much worse derivatives. Turni…
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Hello,
I'd like to embed fsps into a framework which requires that instances be brought up and down rapidly. In particular, I'd like to get
```python
import fsps
pop = fsps.StellarPopulation()…
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pb.wd_data currently contain the entire atmcof/atmcofplanck files. This is clearly superfluous and needs fixing. The python part in passbands.py that extracts the particular passband info is written b…
aprsa updated
3 years ago
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I am trying to run beagle and getting this error. It occurs with param files that used to work, and using version 0.10.x. I have downloaded 0.18.2 and get the same error. I also get the same error usi…
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The code below produces two very different isochrones, where I expect them to be the same. This is true for the whole range of allowed (age, feh) which does not cause `isochrone()` to fail (that's an…
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People will forget to update both compasConfigDefault.yaml and example_bbh_compas_config.
Lets update the CI to use compasConfigDefault.yaml (default settings) but only over-write the initial condit…
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The stellar grid is currently based on isochrones. This the grid has uniform spacing in age, but non-uniform in mass. Isochrones are best for dealing with ensembles of stars, but not necessarily for…
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I am using BEAGLE to fit both broadband photometry and emission line equivalent width measured from spectra simultaneously. It runs well if equivalent width type `ewType` is set to be `standard` or `l…
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We discuss here the science cases of having an 8-m wide FOV (~1 deg in diameter) telescope with a multi-object spectrograph on following up the dwarf galaxies in Milky Way. And maybe also a comparison…
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This is an issue to track progress on the axion dark matter hack. Our plan is to do some reading tonight on 4 different astrophysical axion constraints:
* Tip of the red giant branch
* Horizontal …