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Building Release 2 of the Chandra Source Catalog

机译:建立Chandra源目录的第2版

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The second major release of the Chandra Source Catalog builds on the first catalog release by stacking subsets of overlapping observations, using a permissive source detection approach to identify source candidates and enable point detections down to ~ 5 net counts on-axis, and evaluating the reality of the candidate detections by applying a Sherpa-based maximum-likelihood estimator.?The catalog provides a detailed set of properties for each X-ray source, including source position, extent, multi-band aperture photometry, spectral fits and hardness ratios, and temporal variability measures. In addition, the catalog provides per-field and per-source data products such as images, photon event lists, spectra, light curves, and extended source polygons. We highlight the differences between the first and second catalog releases, and discuss the decisions that drove the changes. We present the newly developed techniques that were required to build release 2 of the catalog, and identify algorithms that have been updated. Finally, we briefly discuss lessons learned.
机译:钱德拉源目录的第二主隔离建立在通过堆叠的重叠观察的子集,使用许可源检测方法来识别源的候选,并启用点检测下降到轴〜5净计数和评估所述现实第一目录释放通过应用基于夏尔巴-最大似然estimator.?The目录提供了详细的集合对于每个X射线源的特性,包括源位置,范围,多频带孔径测光,光谱拟合和硬度比的候选检测,和时间变化措施。此外,目录还提供每场和每个源数据产品,例如图像,光子事件列表,光谱,光曲线和扩展源多边形。我们突出了第一和第二目录版本之间的差异,并讨论了推动变化的决策。我们提出了建立目录版本所需的新开发的技术,并识别已更新的算法。最后,我们简要介绍了学习的经验教训。

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