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The Chandra Source Catalog Release 2 Master Match Pipeline

机译:Chandra Source Catalog版本2主匹配管道

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The Chandra Source Catalog (CSC) is a catalog of pointed and serendipitous sources observed by the Chandra X-Ray Observatory since its 1999 launch. An overview of the first release of the CSC is given by Evans et al. (2010). The second release of the CSC will feature additional sources detected in observations released publicly since the CSC first release, as well as additional fainter sources found by combining observations whose pointings differ by no more than one arcminute into "detect stacks". Algorithm improvements are expected to further increase the number of fainter sources detected, with a goal of identifying sources down to approximately five net counts on-axis. The CSC Release 2 master match pipeline is tasked with matching observations of the same celestial sources from multiple detect stacks to identify "master sources" on the sky, and identifying the detections in all stack observations that contribute to those master sources. The problem of matching photons from sources in multiple detections to form master sources is conceptually similar to multi-catalog crossmatch problems. The core algorithm that will be used in the master pipeline is based on the Bayesian probability approach outlined by Heinis et al. (2009) and takes into account the position errors in assigning match probabilities. Additional pipeline features will include the ability to incorporate the effect of Chandra's spatially variable Point Spread Function (PSF) to allow matching of multiple compact sources detected on-axis in some stacks with single off-axis detections (with significantly larger PSF) from other stacks. Although the match from an off-axis source may be ambiguous as to which onaxis compact source the detected photons belong, knowledge of this type of match is still useful when calculating certain source properties. The algorithm will also be extended to match Convex Hull Sources (CHS), which are areas of extended emission identified in the CSC by a larger polygonal region
机译:Chandra Source目录(CSC)是自1999年推出以来被Chandra X射线天文台观察到的尖锐和午集来源的目录。 CSC的第一个释放的概述由Evans等人给出。 (2010)。 CSC的第二个释放将特征在于CSC第一释放以来公开释放的观察中检测到的额外源,以及通过组合观察结果的额外较微弱的来源,其指向不超过一个Arcminute进入“检测堆栈”。预计算法改进将进一步增加所检测到的微弱源的数量,其目标是将源识别到轴上大约五个净计数。 CSC版本2主匹配流水线是任务的,具有来自多个检测堆栈的相同天体源的匹配观察,以识别天空中的“主源”,并识别所有堆栈观测的检测,这为这些主源有贡献。在多种检测中匹配来自源的光子的问题在概念上类似于多目录交叉匹配问题。将在主水管道中使用的核心算法基于Heinis等人概述的贝叶斯概率方法。 (2009)并考虑了分配匹配概率的位置错误。额外的管道特征包括结合Chandra的空间可变点扩展功能(PSF)的效果(PSF)以允许在某些堆叠中匹配的多个紧凑源与来自其他堆叠的单个离轴检测(具有明显更大的PSF)的堆叠。虽然来自轴源源的匹配可能是模糊的,但是当检测到的光子属于哪个Onaxis紧凑源,但是在计算某些源属性时仍然有用。该算法还将扩展以匹配凸壳源(CHS),该耦合源(CHS)是通过更大的多边形区域在CSC中识别的扩展发射区域

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