Optical Identifications of High-Redshift Galaxy Clusters from the Planck Sunyaev–Zeldovich Survey
- Авторы: Burenin R.A.1, Bikmaev I.F.2,3, Khamitov I.M.2,4, Zaznobin I.A.1, Khorunzhev G.A.1, Eselevich M.V.5, Afanasiev V.L.6, Dodonov S.N.6, Rubiño-Martín J.7, Aghanim N.8, Sunyaev R.A.1,9
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Учреждения:
- Space Research Institute
- Kazan Federal University
- Academy of Sciences of Tatarstan
- Observatory of Scientific and Technological Research Council of Turkey
- Institute of Solar–Terrestrial Physics, Russian Academy of Sciences
- Special Astrophysical Observatory, Russian Academy of Sciences
- Instituto de Astrofísica de Canarias
- Institut d´ Astrophysique Spatiale
- Max Planck Institut für Astrophysik
- Выпуск: Том 44, № 5 (2018)
- Страницы: 297-308
- Раздел: Article
- URL: https://ogarev-online.ru/1063-7737/article/view/190585
- DOI: https://doi.org/10.1134/S1063773718050018
- ID: 190585
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Аннотация
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.
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Об авторах
R. Burenin
Space Research Institute
Автор, ответственный за переписку.
Email: rodion@hea.iki.rssi.ru
Россия, ul. Profsoyuznaya 84/32, Moscow, 117997
I. Bikmaev
Kazan Federal University; Academy of Sciences of Tatarstan
Email: rodion@hea.iki.rssi.ru
Россия, ul. Kremlevskaya 18, Kazan, 420000; ul. Baumana 20, Kazan
I. Khamitov
Kazan Federal University; Observatory of Scientific and Technological Research Council of Turkey
Email: rodion@hea.iki.rssi.ru
Россия, ul. Kremlevskaya 18, Kazan, 420000; Antalya
I. Zaznobin
Space Research Institute
Email: rodion@hea.iki.rssi.ru
Россия, ul. Profsoyuznaya 84/32, Moscow, 117997
G. Khorunzhev
Space Research Institute
Email: rodion@hea.iki.rssi.ru
Россия, ul. Profsoyuznaya 84/32, Moscow, 117997
M. Eselevich
Institute of Solar–Terrestrial Physics, Russian Academy of Sciences
Email: rodion@hea.iki.rssi.ru
Россия, Irkutsk, 664033
V. Afanasiev
Special Astrophysical Observatory, Russian Academy of Sciences
Email: rodion@hea.iki.rssi.ru
Россия, Karachai-Cherkessian Republic, 369167
S. Dodonov
Special Astrophysical Observatory, Russian Academy of Sciences
Email: rodion@hea.iki.rssi.ru
Россия, Karachai-Cherkessian Republic, 369167
J.-A. Rubiño-Martín
Instituto de Astrofísica de Canarias
Email: rodion@hea.iki.rssi.ru
Испания, Tenerife
N. Aghanim
Institut d´ Astrophysique Spatiale
Email: rodion@hea.iki.rssi.ru
Франция, Orsay
R. Sunyaev
Space Research Institute; Max Planck Institut für Astrophysik
Email: rodion@hea.iki.rssi.ru
Россия, ul. Profsoyuznaya 84/32, Moscow, 117997; Karl-Schwarzschild-Str. 1, Postfach 1317, Garching, D-85741
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