Показать сокращенную информацию
dc.contributor.author | Vorobyev V. | |
dc.contributor.author | Burenin R. | |
dc.contributor.author | Bikmaev I. | |
dc.contributor.author | Khamitov I. | |
dc.contributor.author | Dodonov S. | |
dc.contributor.author | Zhuchkov R. | |
dc.contributor.author | Irtuganov E. | |
dc.contributor.author | Mescheryakov A. | |
dc.contributor.author | Melnikov S. | |
dc.contributor.author | Semena A. | |
dc.contributor.author | Tkachenko A. | |
dc.contributor.author | Aghanim N. | |
dc.contributor.author | Sunyaev R. | |
dc.date.accessioned | 2018-09-19T20:51:32Z | |
dc.date.available | 2018-09-19T20:51:32Z | |
dc.date.issued | 2016 | |
dc.identifier.issn | 1063-7737 | |
dc.identifier.uri | https://dspace.kpfu.ru/xmlui/handle/net/143350 | |
dc.description.abstract | © 2015, Pleiades Publishing, Inc.We present the results of spectroscopic redshift measurements for the galaxy clusters from the first all-sky Planck catalogue that have been mostly identified based on the optical observations performed previously by our team (Planck Collaboration 2015a). Data on 13 galaxy clusters at redshifts from z ≈ 0.2 to z ≈ 0.8, including the improved identification and redshift measurement for the cluster PSZ1 G141.73+14.22 at z = 0.828, are provided. We have performed the measurements based on data from the Russian–Turkish 1.5-m telescope (RTT-150), the 2.2-m Calar Alto Observatory telescope, and the 6-m SAO RAS telescope (Bolshoy Teleskop Azimutalnyi, BTA). | |
dc.relation.ispartofseries | Astronomy Letters | |
dc.subject | galaxies | |
dc.subject | galaxy clusters | |
dc.title | Additional spectroscopic redshift measurements for galaxy clusters from the first Planck catalogue | |
dc.type | Article | |
dc.relation.ispartofseries-issue | 2 | |
dc.relation.ispartofseries-volume | 42 | |
dc.collection | Публикации сотрудников КФУ | |
dc.relation.startpage | 63 | |
dc.source.id | SCOPUS10637737-2016-42-2-SID84958793773 |