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 |
|