Chandra Orion Ultradeep Project: Observations and Source Lists
Chandra Orion Ultradeep Project: Observations and Source Lists
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钱德拉猎户座超深项目：观测和来源清单
DOI：
10.1086/432092
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发表时间：
2004
期刊：
影响因子：
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通讯作者：
E. Feigelson
中科院分区：
文献类型：
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作者：
K. Getman;E. Flaccomio;P. Broos;N. Grosso;M. Tsujimoto;L. Townsley;G. Garmire;J. Kastner;J. Li;F. Harnden;Jr.;S. Wolk;S. Murray;C. Lada;August Muench;M. McCaughrean;G. Meeus;F. Damiani;G. Micela;S. Sciortino;J. Bally;L. Hillenbrand;W. Herbst;T. Preibisch;E. Feigelson
我们提出了一个描述的数据简化方法和派生目录的1600多个X射线点源从异常深2003年1月钱德拉X射线天文台（钱德拉）的猎户座星云星团和嵌入式人口周围OMC-1的观测。这次观测是由钱德拉的先进CCD成像光谱仪（ACIS）获得的，并被昵称为钱德拉猎户座超深项目（COUP）。COUP观测在13.2天的连续时间内进行了838 ks的曝光，提供了X射线天文学历史上获得的关于正常恒星X射线发射的最统一和最全面的数据集。
We present a description of the data reduction methods and the derived catalog of more than 1600 X-ray point sources from the exceptionally deep 2003 January Chandra X-Ray Observatory (Chandra) observation of the Orion Nebula Cluster and embedded populations around OMC-1. The observation was obtained with Chandra's Advanced CCD Imaging Spectrometer (ACIS) and has been nicknamed the Chandra Orion Ultradeep Project (COUP). With an 838 ks exposure made over a continuous period of 13.2 days, the COUP observation provides the most uniform and comprehensive data set on the X-ray emission of normal stars ever obtained in the history of X-ray astronomy.