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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/7758
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dc.contributor.authorMalkov, O-
dc.contributor.authorKarpov, S-
dc.contributor.authorKovaleva, D-
dc.contributor.authorMurthy, J-
dc.contributor.authorSichevsky, S-
dc.contributor.authorSytov, A-
dc.contributor.authorZhao, G-
dc.contributor.authorZhukov, A-
dc.contributor.authorZakharo, A-
dc.date.accessioned2021-06-29T12:07:41Z-
dc.date.available2021-06-29T12:07:41Z-
dc.date.issued2020-12-
dc.identifier.citationCommunications of the Byurakan Astrophysical Observatory, Vol. 67, No. 2, pp. 272-280en_US
dc.identifier.issn2579-2276-
dc.identifier.urihttp://hdl.handle.net/2248/7758-
dc.description.abstractThe parameterization of stars is a well known problem and used for various purposes in astronomy. We have shown that multicolor photometric data from large modern surveys can be used for parameterization of stars. With sufficiently good quality photometry, one may compute a 3D extinction map by comparing catalogued multicolor photometry with photometry derived from the secondary estimators such as the distance modulus and the interstellar extinction law with suitable calibration tables for absolute magnitudes with reasonable spectral types, extinctions and distances.en_US
dc.language.isoenen_US
dc.publisherNAS RA Byurakan Astrophysical Observatoryen_US
dc.relation.urihttps://doi.org/10.52526/25792776-2020.67.2-272-
dc.rights© NAS RA Byurakan Astrophysical Observatory-
dc.subjectSky surveysen_US
dc.subjectPhotometryen_US
dc.subjectCross-matchingen_US
dc.subjectInterstellar extinctionen_US
dc.titleStellar and interstellar parameters from large photometric surveysen_US
dc.typeArticleen_US
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