High-energy sources before INTEGRAL INTEGRAL reference catalog ?
High-energy sources before INTEGRAL INTEGRAL reference catalog ?
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DOI：
10.1051/0004-6361:20031336
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发表时间：
2003-09
影响因子：
6.5
通讯作者：
K. Ebisawa;G. Bourban;A. Bodaghee;N. Mowlavi;T. Courvoisier
中科院分区：
文献类型：
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作者：
K. Ebisawa;G. Bourban;A. Bodaghee;N. Mowlavi;T. Courvoisier
我们描述了INTEGRAL参考目录，该目录在INTEGRAL发射之前对以前已知的明亮X射线和伽马射线源进行了分类。这些源是，或已经至少有一次，比1米蟹超过3千电子伏，预计将被检测到的积分。该目录用于INTEGRAL快速查看分析，以发现新的源或显著变化的源。我们编制了几个已出版的X射线和伽马射线目录，并调查了最近的出版物，寻找新的来源。因此，在我们的INTEGRAL参考目录中有1122个源。除了源的位置，我们显示了一个近似的光谱模型和每个源的预期通量，基于此，我们得到预期的积分计数率。假设默认的仪器性能和至少10 5 s的曝光时间的任何一部分的天空，我们预计，INTEGRAL将检测至少700源低于10 keV和400源以上的20 keV的使命寿命。
We describe the INTEGRAL reference catalog which classifies previously known bright X-ray and gamma-ray sources before the launch of INTEGRAL. These sources are, or have been at least once, brighter than 1m Crab above 3 keV, and are expected to be detected by INTEGRAL. This catalog is being used in the INTEGRALQuick Look Analysisto discover new sources or significantly variable sources. We compiled several published X-ray and gamma-ray catalogs, and surveyed recent publications for new sources. Consequently, there are 1122 sources in our INTEGRAL reference catalog. In addition to the source positions, we show an approximate spectral model and expected flux for each source, based on which we derive expected INTEGRAL counting rates. Assuming the default instrument performances and at least10 5 s exposure time for any part of the sky, we expect that INTEGRAL will detect at least700 sources below 10 keV and400 sources above 20 keV over the mission life.