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dc.date.accessioned | 2019-01-22T20:53:53Z | |
dc.date.available | 2019-01-22T20:53:53Z | |
dc.date.issued | 2018 | |
dc.identifier.uri | https://dspace.kpfu.ru/xmlui/handle/net/149321 | |
dc.description.abstract | © 2018 O. Malkov et al. Information 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. | |
dc.subject | Extinction | |
dc.subject | Photometry | |
dc.subject | Supernovae | |
dc.subject | Surveys | |
dc.title | Interstellar extinction from photometric surveys: Application to four high-latitude areas | |
dc.type | Article | |
dc.relation.ispartofseries-issue | 1 | |
dc.relation.ispartofseries-volume | 27 | |
dc.collection | Публикации сотрудников КФУ | |
dc.relation.startpage | 62 | |
dc.source.id | SCOPUS-2018-27-1-SID85045889303 |