Gothard Obs. Synthetic Stellar Phot. Database
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https://b2find.eudat.eu/dataset/65a9da3c-cdf5-5659-b7d5-5ac2da6c524c
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To determine stellar luminosities and radii, it is necessary to know the total bolometric fluxes emitted by the stars, or equivalently the bolometric corrections (BCs) as...
