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 |
|