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Planck intermediate results. XXVI. Optical identification and redshifts of Planck clusters with the RTT150 telescope

机译:普朗克中间结果。二十六。使用RTT150望远镜进行光学识别和普朗克星团的红移

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摘要

We present the results of approximately three years of observations of Planck Sunyaev-Zeldovich (SZ) sources with the Russian-Turkish 1.5?m telescope (RTT150), as a part of the optical follow-up programme undertaken by the Planck collaboration. During this time period approximately 20% of all dark and grey clear time available at the telescope was devoted to observations of Planck objects. Some observations of distant clusters were also done at the 6 m Bolshoi Telescope Alt-azimutalnyi (BTA) of the Special Astrophysical Observatory of the Russian Academy of Sciences. In total, deep, direct images of more than one hundred fields were obtained in multiple filters. We identified 47 previously unknown galaxy clusters, 41 of which are included in the Planck catalogue of SZ sources. The redshifts of 65 Planck clusters were measured spectroscopically and 14 more were measured photometrically. We discuss the details of cluster optical identifications and redshift measurements. We also present new spectroscopic redshifts for 39 Planck clusters that were not included in the Planck SZ source catalogue and are published here for the first time.
机译:作为普朗克合作开展的光学后续计划的一部分,我们将用俄土1.5毫米望远镜(RTT150)展示普朗克Sunyaev-Zeldovich(SZ)光源大约三年的观测结果。在这段时间里,望远镜可用的所有暗色和灰色晴朗时间的大约20%专用于对普朗克天体的观测。俄罗斯科学院特别天文台的6 m莫斯科大望远镜Alt-azimutalnyi(BTA)也对远处的星团进行了一些观测。总共,在多个滤镜中获得了一百多个场的深层直接图像。我们确定了47个以前未知的星系团,其中41个被包括在SZ源的普朗克目录中。用光谱法测量了65个普朗克簇的红移,用光度法测量了另外14个。我们讨论了群集光学识别和红移测量的细节。我们还为39个普朗克星团提供了新的光谱红移,这些光谱未包括在普朗克SZ源目录中,并且首次在此处发布。

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