Показать сокращенную информацию
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 |