dc.contributor.author |
Khamitov I. |
|
dc.contributor.author |
Bikmaev I. |
|
dc.contributor.author |
Aslan Z. |
|
dc.contributor.author |
Sakhibullin N. |
|
dc.contributor.author |
Vlasyuk V. |
|
dc.contributor.author |
Zheleznyak A. |
|
dc.contributor.author |
Zakharov A. |
|
dc.date.accessioned |
2018-09-18T20:15:29Z |
|
dc.date.available |
2018-09-18T20:15:29Z |
|
dc.date.issued |
2006 |
|
dc.identifier.issn |
1063-7737 |
|
dc.identifier.uri |
https://dspace.kpfu.ru/xmlui/handle/net/138043 |
|
dc.description.abstract |
We present the R c-band light curves for components A and B of the gravitationally lensed quasar SBS 1520+530 obtained during 2001-2005 with the 1.5-m Russian-Turkish Telescope (RTT-150) at the TUBITAK National Observatory (Turkey). Based on an analysis of the data for the period 2001-2002, we have estimated the time delay of the brightness fluctuations between components A and B of the quasar to be 128 days. This time delay agrees with its previously published values for the periods 1999-2001 and 2003-2004. Using all of the published data on the brightnesses of components A and B of SBS 1520+530 for the 6-year period, we have found at least two microlensing events. One event has the pattern of a long-term linear trend; the duration of the other event is several hundred days. © Pleiades Publishing, Inc., 2006. |
|
dc.relation.ispartofseries |
Astronomy Letters |
|
dc.subject |
Active galactic nuclei |
|
dc.subject |
Microlensing |
|
dc.subject |
Photometry |
|
dc.subject |
Quasars and radio galaxies |
|
dc.subject |
Time delay |
|
dc.title |
Analysis of optical light curves for the components of the gravitationally lensed quasar SBS 1520+530 based on observations with the 1.5-m RTT-150 telescope in 2001-2005 |
|
dc.type |
Article |
|
dc.relation.ispartofseries-issue |
8 |
|
dc.relation.ispartofseries-volume |
32 |
|
dc.collection |
Публикации сотрудников КФУ |
|
dc.relation.startpage |
514 |
|
dc.source.id |
SCOPUS10637737-2006-32-8-SID33746725890 |
|