We present the results of optical identifications and spectroscopic redshift measurements for galaxy clusters from the second Planck catalogue of Sunyaev-Zeldovich sources. We used the data of observations with the 1.5-m Russian-Turkish telescope (RTT150), the 1.6-m Sayan Observatory AZT-33IK telescope, the 3.5-m Calar Alto telescope, and the 6-m SAO RAS telescope (Bolshoi Teleskop Azimutalnyi, BTA). For the observations we selected Sunyaev-Zeldovich sources unidentified with galaxy clusters with known redshifts. The observations have been carried out for three years, as a result of which we obtained direct images in various filters for a set of galaxy clusters and spectra for the brightest red-sequence galaxies of these clusters. For 38 ga...
We present the results of approximately three years of observations of Planck Sunyaev-Zeldovich (SZ)...
We present the results of approximately three years of observations of Planck Sunyaev-Zeldovich (SZ)...
International audienceWe present the results of approximately three years of observations of Planck ...
© 2019, Pleiades Publishing, Inc. We present the results of optical identifications and spectroscopi...
International audienceWe present the results of optical identifications and spectroscopic redshift m...
We present the results of approximately three years of observations of Planck Sunyaev-Zeldovich (SZ)...
We present the results of approximately three years of observations of Planck Sunyaev-Zeldovich (SZ)...
International audienceWe present the results of approximately three years of observations of Planck ...
© 2019, Pleiades Publishing, Inc. We present the results of optical identifications and spectroscopi...
International audienceWe present the results of optical identifications and spectroscopic redshift m...
We present the results of approximately three years of observations of Planck Sunyaev-Zeldovich (SZ)...
We present the results of approximately three years of observations of Planck Sunyaev-Zeldovich (SZ)...
International audienceWe present the results of approximately three years of observations of Planck ...