Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/7288
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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.date.accessioned2018-06-13T05:28:40Z-
dc.date.available2018-06-13T05:28:40Z-
dc.date.issued2018-02-
dc.identifier.citationOpen Astronomy, Vol. 27, No. 1, pp. 62-69en_US
dc.identifier.issn2543-6376-
dc.identifier.urihttp://hdl.handle.net/2248/7288-
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.language.isoenen_US
dc.publisherDe Gruyteren_US
dc.relation.urihttps://doi.org/10.1515/astro-2018-0002-
dc.rights© Walter de Gruyter GmbH-
dc.subjectExtinctionen_US
dc.subjectSurveysen_US
dc.subjectPhotometryen_US
dc.subjectSupernovaeen_US
dc.titleInterstellar extinction from photometric surveys: application to four high-latitude areasen_US
dc.typeArticleen_US
Appears in Collections:IIAP Publications

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