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Do we want to moe to [`dust_extiction`](https://dust-extinction.readthedocs.io/en/stable/index.html)?
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We could use the dust_extinction package that has been recently developed and is now an astropy affiliated package. I was the lead of this development. This would provide the same plus additional du…
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Show how to use the dust_extinction package to unextinguish (deredden) a spectrum.
Use observed ultraviolet spectra from a FITS binary table file -> use astropy.io.fits.
Include photometry from Si…
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In the physics model grid creation, there are a number of places where two choices are present, those where the dust extinction model include f_A and those where it does not. It would be simpler if t…
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Define ACTRIS variable names for at least:
- dust optical depth at 550nm (instantaneous)
- dust load (instantaneous)
- surface dust concentration (instantaneous)
- surface dust extinction (instant…
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TRILEGAL star properties may be obtained from Astro Data Lab. See available quantities at https://datalab.noirlab.edu/query.php?name=lsst_sim.simdr2. As compared to the information available to skyCa…
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There's a generalization of the CCM89 dust extinction model in the Appendix of Conroy+10 that varies the bump strength to allow for modeling attenuation in galaxies. A possible addition for this pack…
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Dear friends,
I would just kindly suggest to add explicit models for the SMC and the LMC. More or less as in the analogous python package dust_extinction (https://dust-extinction.readthedocs.io/en/…
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The functionality for dealing with the EUV parts of the SEDs in the BEAST has not been maintained well. We need to update/add back those functionalities.
@karllark will include dust physic models …
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It would be very illustrative and pedagogical to create a widget showing side by side a picture of the dust/star geometry, clumpiness of dust distribution, (others?) and the corresponding attenuation …