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arXiv 1609.09244astro-ph.HE
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第二次ROSAT全天巡天源目录

Second ROSAT all-sky survey (2RXS) source catalogue

Th. Boller, M. J. Freyberg, J. Truemper, F. Haberl, W. Voges, K. Nandra

摘要:

我们提出第二个ROSAT全天空巡天源目录,以下简称为2 RXS目录。这是1990年6月至1991年8月期间利用PSPC进行的ROSAT全天空巡天(RASS)观测中获得的第二份公开发布的ROSAT点状源目录,是亮源和暗源目录的扩展和修订版本。我们使用最新版本的RASS处理来生成6.4x6.4度天空区域的重叠X射线图像。为了创建源目录,将基于似然性的检测算法应用于这些源目录,该算法考虑了PSPC视场中的PSF。与1 RXS相比,还实现了背景测定的改进。我们在0.1-2.4 keV的能量带中获得了大约135,000个X射线探测,其可能性阈值为6.5。我们的模拟表明,预期的虚假内容的目录是一个强大的功能的检测可能性,和完整的目录预计将包含约30%的虚假检测。X射线图像和叠加的X射线轮廓线提供了额外的用户产品,以目视评估检测结果,我们进行了自己的目视检查,以标记不确定的检测结果。基于标准化过量方差和最大振幅变异性分析,对X射线光变曲线的日内变异性进行定量。使用三个基本模型,幂律,热等离子体发射模型和黑体发射进行X射线光谱拟合。确定了32个具有扩散排放和嵌入式点源的大型扩展区域,并将其排除在本分析之外。2 RXS目录提供了比eROSITA更深入、更清晰的X射线全天巡天目录。

英文摘要:

We present the second ROSAT all-sky survey source catalogue, hereafter referred to as the 2RXS catalogue. This is the second publicly released ROSAT catalogue of point-like sources obtained from the ROSAT all-sky survey (RASS) observations performed with the PSPC between June 1990 and August 1991, and is an extended and revised version of the bright and faint source catalogues. We used the latest version of the RASS processing to produce overlapping X-ray images of 6.4x6.4 degrees sky regions. To create a source catalogue, a likelihood-based detection algorithm was applied to these, which accounts for the PSF across the PSPC field of view. Improvements in the background determination compared to 1RXS were also implemented. We obtained about 135,000 X-ray detections in the 0.1-2.4 keV energy band down to a likelihood threshold of 6.5. Our simulations show that the expected spurious content of the catalogue is a strong function of detection likelihood, and the full catalogue is expected to contain about 30% spurious detections. X-ray images and overlaid X-ray contour lines provide an additional user product to evaluate the detections visually, and we performed our own visual inspections to flag uncertain detections. Intra-day variability in the X-ray light curves was quantified based on the normalised excess variance and a maximum amplitude variability analysis. X-ray spectral fits were performed using three basic models, a power law, a thermal plasma emission model, and black-body emission. Thirty-two large extended regions with diffuse emission and embedded point sources were identified and excluded from the present analysis. The 2RXS catalogue provides the deepest and cleanest X-ray all-sky survey catalogue in advance of eROSITA.

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