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dc.date.accessioned | 2019-01-22T20:41:01Z | |
dc.date.available | 2019-01-22T20:41:01Z | |
dc.date.issued | 2018 | |
dc.identifier.issn | 1063-7737 | |
dc.identifier.uri | https://dspace.kpfu.ru/xmlui/handle/net/148274 | |
dc.description.abstract | © 2018, Pleiades Publishing, Inc. We present the results of optical identifications and spectroscopic redshift measurements for galaxy clusters from the second Planck catalogue of Sunyaev–Zeldovich sources (PSZ2) located at high redshifts, z ≈ 0.7−0.9. We used the data of optical observations with the Russian–Turkish 1.5-mtelescope (RTT-150), the Sayan Observatory 1.6-m telescope, the Calar Alto 3.5-m telescope, and the 6-m SAO RAS telescope (BTA). The spectroscopic redshift measurements were obtained for seven galaxy clusters, including one cluster, PSZ2 G126.57+51.61, from the cosmological sample of the PSZ2 catalogue. In the central regions of two clusters, PSZ2 G069.39+68.05 and PSZ2 G087.39−34.58, we detected arcs of strong gravitational lensing of background galaxies, one of which is at redshift z = 4.262. The data presented below roughly double the number of known galaxy clusters in the second Planck catalogue of Sunyaev–Zeldovich sources at high redshifts, z ≈ 0.8. | |
dc.relation.ispartofseries | Astronomy Letters | |
dc.subject | galaxy clusters | |
dc.subject | sky surveys | |
dc.title | Optical Identifications of High-Redshift Galaxy Clusters from the Planck Sunyaev–Zeldovich Survey | |
dc.type | Article | |
dc.relation.ispartofseries-issue | 5 | |
dc.relation.ispartofseries-volume | 44 | |
dc.collection | Публикации сотрудников КФУ | |
dc.relation.startpage | 297 | |
dc.source.id | SCOPUS10637737-2018-44-5-SID85047482406 |