PHOENIX grid T2000-6000 W21500-22200 R40000
- 1. UCLA
- 2. MSU
Description
A test grid made for StarKit code (https://github.com/starkit/starkit) made from Phoenix grid (any use of the code needs to cite Husser et al. 2013 - bibtex code can be found and end of this description). The range of effective temperatures: 2000-6000K, wavelength range 21500-22200 Angstroms, resolution of 40000.
@ARTICLE{2013A&A...553A...6H,
author = {{Husser}, T. -O. and {Wende-von Berg}, S. and {Dreizler}, S. and
{Homeier}, D. and {Reiners}, A. and {Barman}, T. and
{Hauschildt}, P.~H.},
title = "{A new extensive library of PHOENIX stellar atmospheres and synthetic spectra}",
journal = {\aap},
keywords = {stars: atmospheres, convection, stars: late-type, Astrophysics - Solar and Stellar Astrophysics},
year = 2013,
month = May,
volume = {553},
eid = {A6},
pages = {A6},
doi = {10.1051/0004-6361/201219058},
archivePrefix = {arXiv},
eprint = {1303.5632},
primaryClass = {astro-ph.SR},
adsurl = {https://ui.adsabs.harvard.edu/\#abs/2013A&A...553A...6H},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}
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