This paper extends synthetic photometry to components of binary star systems. The paper demonstrates accurate recovery of single star photometric properties for four photometric standards, Vega, Sirius, GD153, and HD209458, ranging over the HR diagram, when their model synthetic spectra are placed in fictitious binary systems and subjected to synthetic photometry processing. Techniques for photometric distance determination have been validated for all four photometric standards.
|Original language||English (US)|
|State||Published - Sep 2013|
- methods: numerical
- stars: individual (Sirius, Vega, GD153, HD209458)
ASJC Scopus subject areas
- Astronomy and Astrophysics
- Space and Planetary Science
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Spectra of Vega, Sirius, GD153, and HD209458
Linnell, A. P. (Creator), Destefano, P. (Contributor) & Hubeny, I. (Creator), Centre de Donnees Strasbourg (CDS), 2014
DOI: 10.26093/cds/vizier.51460068, https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/146/68