dc.contributor.author |
Malkov, O |
|
dc.contributor.author |
Karpov, S |
|
dc.contributor.author |
Kilpio, E |
|
dc.contributor.author |
Sichevsky, S |
|
dc.contributor.author |
Chulkov, D |
|
dc.contributor.author |
Dluzhnevskaya, O |
|
dc.contributor.author |
Kovaleva, D |
|
dc.contributor.author |
Kniazev, A |
|
dc.contributor.author |
Mickaelian, A |
|
dc.contributor.author |
Mironov, A |
|
dc.contributor.author |
Murthy, J |
|
dc.contributor.author |
Sytov, A |
|
dc.contributor.author |
Zhao, G |
|
dc.contributor.author |
Zhukov, A |
|
dc.date.accessioned |
2020-11-11T01:18:12Z |
|
dc.date.available |
2020-11-11T01:18:12Z |
|
dc.date.issued |
2018-04 |
|
dc.identifier.citation |
Open Astronomy, Vol. 27, No. 1, pp. 62-69 |
en_US |
dc.identifier.issn |
2543-6376 |
|
dc.identifier.uri |
http://prints.iiap.res.in/handle/2248/6847 |
|
dc.description |
Open Access © Walter de Gruyter GmbH; https://doi.org/10.1515/astro-2018-0002 |
en_US |
dc.description.abstract |
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. |
en_US |
dc.language.iso |
en |
en_US |
dc.publisher |
De Gruyter |
en_US |
dc.subject |
Extinction |
en_US |
dc.subject |
Supernovae |
en_US |
dc.subject |
Photometry |
en_US |
dc.subject |
Surveys |
en_US |
dc.title |
Interstellar extinction from photometric surveys: application to four high-latitude areas |
en_US |
dc.type |
Article |
en_US |