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Astrophysics > Cosmology and Nongalactic Astrophysics

arXiv:1403.0758v1 (astro-ph)
[Submitted on 4 Mar 2014 ]

Title: The 2XMMi/SDSS Galaxy Cluster Survey. III. Clusters associated with spectroscopically targeted luminous red galaxies in SDSS-DR10

Title: 2XMMi/SDSS星系团调查。 III. 与光谱目标明亮红星系相关的星系团在SDSS-DR10中

Authors:A. Takey, A. Schwope, G. Lamer
Abstract: We present a sample of 383 X-ray selected galaxy groups and clusters with spectroscopic redshift measurements (up to z ~ 0.79) from the 2XMMi/SDSS Galaxy Cluster Survey. The X-ray cluster candidates were selected as serendipitously detected sources from the 2XMMi-DR3 catalogue that were located in the footprint of the Sloan Digital Sky Survey (SDSS-DR7). The cluster galaxies with available spectroscopic redshifts were selected from the SDSS-DR10. We developed an algorithm for identifying the cluster candidates that are associated with spectroscopically targeted luminous red galaxies and for constraining the cluster spectroscopic redshift. A cross-correlation of the constructed cluster sample with published optically selected cluster catalogues yielded 264 systems with available redshifts. The present redshift measurements are consistent with the published values. The current cluster sample extends the optically confirmed cluster sample from our cluster survey by 67 objects. Moreover, it provides spectroscopic confirmation for 78 clusters among our published cluster sample, which previously had only photometric redshifts. Of the new cluster sample that comprises 67 systems, 55 objects are newly X-ray discovered clusters and 52 systems are sources newly discovered as galaxy clusters in optical and X-ray wavelengths. Based on the measured redshifts and the fluxes given in the 2XMMi-DR3 catalogue, we estimated the X-ray luminosities and masses of the cluster sample.
Abstract: 我们呈现了一个包含383个X射线选定的星系团和星系簇的样本,并具有光谱红移测量值(最高至z ~ 0.79),来自2XMMi/SDSS星系簇调查。 X射线簇候选体是从2XMMi-DR3目录中偶然检测到的源,这些源位于斯隆数字天空调查(SDSS-DR7)的覆盖范围内。 具有可用光谱红移的簇星系是从SDSS-DR10中选择的。 我们开发了一种算法,用于识别与光谱目标明亮红色星系相关的簇候选体,并限制簇的光谱红移。 将构建的簇样本与已发表的光学选定簇目录进行交叉相关,得到了264个具有可用红移的系统。 目前的红移测量结果与已发表的值一致。 当前的簇样本将我们调查中的光学确认的簇样本扩展了67个对象。 此外,它为我们的已发表簇样本中的78个簇提供了光谱确认,这些簇之前只有测光红移。 在由67个系统组成的新的簇样本中,55个对象是新发现的X射线簇,52个系统是在光学和X射线波长中首次发现的星系簇。 基于测量的红移和2XMMi-DR3目录中给出的通量,我们估计了簇样本的X射线光度和质量。
Comments: A&A in press, 12 pages, 15 figures, 1 table, http://www.aanda.org/index.php?option=com_article&access=doi&doi=10.1051/0004-6361/201322973
Subjects: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
Cite as: arXiv:1403.0758 [astro-ph.CO]
  (or arXiv:1403.0758v1 [astro-ph.CO] for this version)
  https://doi.org/10.48550/arXiv.1403.0758
arXiv-issued DOI via DataCite
Related DOI: https://doi.org/10.1051/0004-6361/201322973
DOI(s) linking to related resources

Submission history

From: Ali Takey [view email]
[v1] Tue, 4 Mar 2014 12:20:05 UTC (1,637 KB)
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