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**Describe the changes**
- Add "Alpha2 CVn stars" as Use For in http://astrothesaurus.org/uat/27
- Relate Protoplanetary nebulae http://astrothesaurus.org/uat/1301 and Post-asymptotic giant branch
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Hello,
First of all thanks for the grate code you have created.
So I just installed BASE-9 from the repository and run test with the default parameters from the base9.yml file and it worked well.…
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I wonder whether everyone is on the same page re. selecting white dwarfs. Two things have happened 'recently':
- Boris has stated a preference for targeting white dwarfs based on a pre-selected cat…
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Need to get the new ones so that they can be added to the BEAST library download.
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Может кто-то помочь? Или у кого-то мб что-то подобное было?
У меня почему-то некоторые источники отображаются в формате "первый автор, название, остальное", а некоторые начинаются с названия сразу.…
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Add in functionality to deal with MAP isochrone fitting for observed data. This will focus on generating isochrones as a function of age and metallicity and comparing them to observed objects. The goa…
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A while back there was an implementation of the self-consistent field (SCF) initialization for binary white dwarfs in the `wdmerger` repo, in `prob.cpp`. This should be recovered from the git histor…
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The online Codex on EDSM shows for DQ Type Star:
https://www.edsm.net/en/codex/discoveries/idR/9/region/Inner+Scutum-Centaurus+Arm/details/idD/11190/nameD/White+Dwarf+Star/idC/10000/nameC/Astronomica…
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I'm working on visualizations of ASTs. To start, using the SMIDGE catalog, here is a comparison between the two methods of selecting ASTs. Both methods are applied after discarding SEDs that are not…
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Currently star temperature is defined by the star's class. Actually a lot of stars have nonstandard values (white dwarfs, neutron stars, etc), so for them it's good to have a temperature parameter in …