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Spectroscopic Redshift Measurements for Galaxy Clusters from the Planck Survey and Observations of These Clusters in the SRG/eROSITA Survey

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Abstract

We present the results of our spectroscopic redshift measurements for galaxy clusters detected previously from Planck all-sky survey data as well as Sloan Digital Sky Survey and WISE all-sky survey data. The redshifts have been measured for 23 clusters, including four galaxy clusters from the second Planck catalogue of Sunyaev–Zeldovich sources. The main spectroscopic observations were carried out during 2019–early 2020 at the 1.6-m AZT-33IK telescope of the Sayan Observatory and the 1.5-m Russian–Turkish telescope (RTT-150). Some of the data have been obtained previously at the 3.5-m Calar Alto telescope. Out of the 23 clusters in this sample, 14 objects are located in the half of the sky where the rights to the data from the eROSITA sky survey onboard the SRG orbital X-ray observatory belong to the Russian side. All these clusters were detected with the eROSITA telescope in the course of the sky survey during 2020. On the whole, we have measured the spectroscopic redshifts for 220 galaxy clusters within our program of optical identifications of galaxy clusters from the Planck catalogue during several years. Many of them have already been detected in the SRG/eROSITA survey; a significant fraction of these objects are among the most massive galaxy clusters of the eROSITA sky survey and will most likely enter into cosmological samples of clusters from this survey.

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Notes

  1. http://hea.iki.rssi.ru/rtt150/ru/index.php?page=tfosc.

  2. http://iraf.noao.edu/.

  3. https://www.eso.org/sci/observing/tools/standards.html.

  4. http://ckp-rf.ru/ckp/3056/.

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ACKNOWLEDGMENTS

This work was supported by RSF grant no. 18-12-00520. We thank TÜBITAK, the Space Research Institute of the Russian Academy of Sciences, the Kazan Federal University, and the Academy of Sciences of Tatarstan for supporting the observations at the Russian–Turkish 1.5-m telescope (RTT-150). The measurements with the AZT-33IK telescope were performed within the basic financing of the FNI II.16 program and were obtained using the equipment of the Angara sharing center.Footnote 4 In this study we used observational data from the eROSITA telescope onboard the SRG observatory. The SRG observatory was built by Roskosmos in the interests of the Russian Academy of Sciences represented by its Space Research Institute (IKI) within the framework of the Russian Federal Space Program, with the participation of the Deutsches Zentrum für Luft- und Raumfahrt (DLR). The SRG/eROSITA X-ray telescope was built by a consortium of German Institutes led by MPE, and supported by DLR. The SRG spacecraft was designed, built, launched, and is operated by the Lavochkin Association and its subcontractors. The science data are downlinked via the Deep Space Network Antennae in Bear Lakes, Ussurijsk, and Baykonur, funded by Roskosmos. The eROSITA data used in this work were processed using the eSASS software system developed by the German eROSITA consortium and the proprietary data reduction and analysis software developed by the Russian eROSITA Consortium.

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Authors and Affiliations

  1. Space Research Institute, 117997, Moscow, ul. Profsoyuznaya 84/32, Russia

    I. A. Zaznobin, R. A. Burenin, G. A. Khorunzhev, A. R. Lyapin, N. S. Lyskova, P. S. Medvedev, M. R. Gilfanov & R. A. Sunyaev

  2. Kazan Federal University, 420000, Kazan, ul. Kremlevskaya 18, Russia

    I. F. Bikmaev & I. M. Khamitov

  3. Academy of Sciences of Tatarstan, Kazan, ul. Baumana, 20, Russia

    I. F. Bikmaev

  4. TÜBITAK National Observatory, Antalya, Turkey

    I. M. Khamitov

  5. Institute of Solar–Terrestrial Physics, Russian Academy of Sciences, Siberian Branch, 664033, Irkutsk, P.O. Box 291, Russia

    M. V. Eselevich

  6. Max Planck Institut für Astrophysik, D-85741, Garching, Karl-Schwarzschild-Str. 1, Postfach 1317, Germany

    M. R. Gilfanov & R. A. Sunyaev

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  1. I. A. Zaznobin
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  2. R. A. Burenin
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  3. I. F. Bikmaev
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  4. I. M. Khamitov
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  7. M. V. Eselevich
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  8. N. S. Lyskova
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  11. R. A. Sunyaev
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Correspondence to I. A. Zaznobin.

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Translated by V. Astakhov

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Zaznobin, I.A., Burenin, R.A., Bikmaev, I.F. et al. Spectroscopic Redshift Measurements for Galaxy Clusters from the Planck Survey and Observations of These Clusters in the SRG/eROSITA Survey. Astron. Lett. 47, 61–70 (2021). https://doi.org/10.1134/S1063773721020055

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