首页> 外文期刊>Astronomy and astrophysics >Characterization of a subsample of the Planck SZ source cluster catalogues using optical SDSS DR12 data
【24h】

Characterization of a subsample of the Planck SZ source cluster catalogues using optical SDSS DR12 data

机译:使用光学SDSS DR12数据表征 Planck SZ源群集目录的子样本

获取原文
           

摘要

Aims . The Planck catalogues of Sunyaev –Zeldovich (SZ) sources, PSZ1 and PSZ2, are the largest catalogues of galaxy clusters selected through their SZ signature in the full sky. In 2013, we started a long-term observational programme at Canary Island observatories with the aim of validating ~500 unconfirmed SZ sources. In this work we present results of the initial pre-screening of possible cluster counterparts using photometric and spectroscopic data of the Sloan Digital Sky Survey DR12. Our main aim is to identify previously unconfirmed PSZ2 cluster candidates and to contribute in the determination of the actual purity and completeness of Planck SZ source sample. Methods . Using the latest version of the PSZ2 catalogue, we selected all sources overlapping with the SDSS DR12 footprint and without redshift information. We validated these cluster fields following optical criteria (mainly distance with respect to the Planck pointing, magnitude of the brightest cluster galaxy, and cluster richness), and combined these criteria with the profiles of the Planck Compton y -maps. This combined procedure allows for a more robust identification of optical counterparts compared to simply cross-matching with existing SDSS cluster catalogues that have been constructed from earlier SDSS data releases. Results . The sample contains new redshifts for 37 Planck galaxy clusters that were not included in the original release of PSZ2 Planck catalogue. We detect three cases as possible multiple counterparts. We show that a combination of all available information (optical images and profile of SZ signal) can provide correct associations between the observed Planck SZ source and the optically identified cluster. We also show that Planck SZ detection is very sensitive even to high- z ( z > 0.5) clusters. In addition, we also present updated spectroscopic information for 34 Planck PSZ1 sources (33 previously photometrically confirmed and 1 new identification).
机译:目的。 Sunyaev – Zeldovich(SZ)源的普朗克目录PSZ1和PSZ2是通过满天的SZ签名选择的最大星系团目录。 2013年,我们在加那利岛天文台启动了一项长期观测计划,目的是验证约500个未经确认的深圳源。在这项工作中,我们介绍了使用Sloan Digital Sky Survey DR12的光度和光谱数据对可能的聚类对应物进行初步预筛选的结果。我们的主要目的是确定以前未确认的PSZ2簇候选物,并有助于确定普朗克SZ源样品的实际纯度和完整性。方法 。使用最新版本的PSZ2目录,我们选择了与SDSS DR12占用空间重叠且没有红移信息的所有来源。我们根据光学标准(主要是相对于普朗克指向的距离,最亮的群集星系的大小和群集丰富度)验证了这些群集场,并将这些标准与普朗克·康普顿y图的轮廓结合在一起。与简单地交叉匹配从早期SDSS数据版本构建的现有SDSS群集目录相比,此组合过程可以更可靠地识别光学对象。结果。该示例包含针对PSZ2 Planck目录原始发行版中未包含的37个Planck星系团的新红移。我们检测到三种可能的情况。我们表明,所有可用信息(光学图像和SZ信号轮廓)的组合可以在观察到的普朗克SZ源和光学识别的簇之间提供正确的关联。我们还表明,即使对于高z(z> 0.5)簇,普朗克SZ检测也非常敏感。此外,我们还为34个普朗克PSZ1光源提供了更新的光谱信息(33个以前用光度法确认和1个新标识)。

著录项

相似文献

  • 外文文献
  • 专利
获取原文

客服邮箱:kefu@zhangqiaokeyan.com

京公网安备:11010802029741号 ICP备案号:京ICP备15016152号-6 六维联合信息科技 (北京) 有限公司©版权所有
  • 客服微信

  • 服务号