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The Highest-Energy Photons Seen by the Energetic Gamma Ray Experiment Telescope (EGRET) on the Compton Gamma Ray Observatory

机译:高能γ射线实验观察到的最高能光子  康普顿伽马射线天文台的望远镜(EGRET)

摘要

During its nine-year lifetime, the Energetic Gamma Ray Experiment Telescope(EGRET) on the Compton Gamma Ray Observatory (CGRO) detected 1506 cosmicphotons with measured energy E>10 GeV. Of this number, 187 are found within 1degree of sources that are listed in the Third EGRET Catalog and were includedin determining the detection likelihood, flux, and spectra of those sources. Inparticular, five detected EGRET pulsars are found to have events above 10 GeV,and together they account for 37 events. A pulsar not included in the ThirdEGRET Catalog has 2 events, both with the same phase and in one peak of thelower-energy gamma-ray light-curve. Most of the remaining 1319 events appear tobe diffuse Galactic and extragalactic radiation based on the similarity of thetheir spatial and energy distributions with the diffuse model and in the E>100,MeV emission. No significant time clustering which would suggest a burst wasdetected.
机译:在康普顿伽玛射线天文台(CGRO)上的高能伽玛射线实验望远镜(EGRET)在其九年生命中,检测到1506个宇宙光子,其能量E> 10 GeV。在此数量中,在第三个EGRET目录中列出的1度源中发现187个,并包括在确定这些源的检测可能性,通量和光谱中。特别是,发现了五个探测到的EGRET脉冲星具有超过10 GeV的事件,它们共同构成了37个事件。 ThirdEGRET Catalog中未包括的脉冲星有2个事件,具有相同的相位,并且在较低能量的伽马射线光曲线的一个峰值中。剩余的1319个事件中,大多数事件似乎是弥散的银河和银河外辐射,这是由于它们的空间和能量分布与弥散模型的相似性以及E> 100,MeV发射所致。没有明显的时间聚类,这表明未检测到爆发。

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