Creating and Using Large Grids of Pre-calculated Model Atmospheres for Rapid Analysis of Stellar Spectra

@inproceedings{Zsarg2019CreatingAU,
  title={Creating and Using Large Grids of Pre-calculated Model Atmospheres for Rapid Analysis of Stellar Spectra},
  author={Janos Zsarg{\'o} and Celia R. Fierro-Santill{\'a}n and Jaime Klapp and Anabel Arrieta and Lorena Arias and Jurij Mendoza Valencia and Leonardo Di G. Sigalotti},
  booktitle={ISUM},
  year={2019}
}
Aims. We present a database of 43 340 atmospheric models (∼80 000 models at the conclusion of the project) for stars with stellar masses between 9 and 120 M⊙, covering the region of the OB main-sequence and Wolf-Rayet stars in the Hertzsprung-Russell diagram. Methods. The models were calculated using the ABACUS I supercomputer and the stellar atmosphere code CMFGEN. Results. The parameter space has six dimensions: the effective temperature Teff, the luminosity L, the metallicity Z, and three… 
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