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Optical Identifications of High-Redshift Galaxy Clusters from the Planck Sunyaev-Zeldovich Survey
DOI: 10.1134/S1063773718050018 Bibcode: 2018AstL...44..297B

Aghanim, N.; Bikmaev, I. F.; Khamitov, I. M. +8 more

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,…

2018 Astronomy Letters
Planck 28
An extension of the Planck galaxy cluster catalogue
DOI: 10.1134/S1063773717080035 Bibcode: 2017AstL...43..507B

Burenin, R. A.

We present a catalogue of galaxy clusters detected in the Planck all-sky Compton parameter maps and identified using data from the WISE and SDSS surveys. The catalogue comprises about 3000 clusters in the SDSS fields. We expect the completeness of this catalogue to be high for clusters with masses larger than M 500 ≈ 3 × 1014

2017 Astronomy Letters
Planck 27
Additional spectroscopic redshift measurements for galaxy clusters from the first Planck catalogue
DOI: 10.1134/S1063773716020055 Bibcode: 2016AstL...42...63V

Aghanim, N.; Melnikov, S. S.; Irtuganov, E. N. +10 more

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 ident…

2016 Astronomy Letters
Planck 11
Steep-spectrum sources of the RCR catalog in the millimeter and submillimeter ranges based on Planck data
DOI: 10.1134/S1063773715090066 Bibcode: 2015AstL...41..457V

Verkhodanov, O. V.; Majorova, E. K.; Zhelenkova, O. P. +2 more

We have investigated the regions of cosmic microwave background maps from the Planck experiment in the neighborhoods of radio sources from the RCR catalog. Based on the measurements of sources from the Planck catalog, we have constructed the calibration curves to determine the brightness of objects. For 34 steep-spectrum objects, for the first tim…

2015 Astronomy Letters
Planck 10