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dc.contributor.authorKarpov, S-
dc.contributor.authorKilpio, E-
dc.contributor.authorSichevsky, S-
dc.contributor.authorChulkov, D-
dc.contributor.authorDluzhnevskaya, O-
dc.contributor.authorKovaleva, D-
dc.contributor.authorKniazev, A-
dc.contributor.authorMickaelian, A-
dc.contributor.authorMironov, A-
dc.contributor.authorMurthy, J-
dc.contributor.authorSytov, A-
dc.contributor.authorZhao, G-
dc.contributor.authorZhukov, A-
dc.identifier.citationOpen Astronomy, Vol. 27, No. 1, pp. 62-69en_US
dc.descriptionOpen Accessen_US
dc.description.abstractInformation on interstellar extinction and dust properties may be obtained from modern large photometric surveys data. Virtual Observatory facilities allow users to make a fast and correct cross-identification of objects from various surveys. It yields a multicolor photometry data on detected objects and makes it possible to estimate stellar parameters and calculate interstellar extinction. A 3D extinction map then can be constructed. The method was applied to 2MASS, SDSS, GALEX and UKIDSS surveys. Results for several high-latitude areas are obtained, compared with independent sources and discussed here.en_US
dc.publisherDe Gruyteren_US
dc.rights© Walter de Gruyter GmbH-
dc.titleInterstellar extinction from photometric surveys: application to four high-latitude areasen_US
Appears in Collections:IIAP Publications

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