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Earth occultation imaging of the low energy gamma-ray sky with GBM

机译:GBM对低能伽玛射线天空的地球掩星成像

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Aims. The Earth Occultation Technique (EOT) has been applied to Fermi’s Gamma-ray Burst Monitor (GBM) to perform all-sky monitoring for a predetermined catalog of hard X-ray/soft γ-ray sources. In order to search for sources not in the catalog, thus completing the catalog and reducing a source of systematic error in EOT, an imaging method has been developed – Imaging with a Differential filter using the Earth Occultation Method (IDEOM). Methods. IDEOM is a tomographic imaging method that takes advantage of the orbital precession of the Fermi satellite. Using IDEOM, all-sky reconstructions have been generated for ~4 years of GBM data in the 12–50 keV, 50–100 keV and 100–300 keV energy bands in search of sources otherwise unmodeled by the GBM occultation analysis. Results. IDEOM analysis resulted in the detection of 57 sources in the 12–50 keV energy band, 23 sources in the 50–100 keV energy band, and 7 sources in the 100–300 keV energy band. Seventeen sources were not present in the original GBM-EOT catalog and have now been added. We also present the first joined averaged spectra for four persistent sources detected by GBM using EOT and by the Large Area Telescope (LAT) on Fermi: NGC 1275, 3C 273, Cen A, and the Crab.
机译:目的地球掩星技术(EOT)已应用于费米的伽马射线爆破监测仪(GBM),以对预定的硬X射线/软γ射线源目录进行全天候监测。为了搜索不在目录中的源,从而完成目录并减少EOT中的系统误差,已开发出一种成像方法-使用地球掩星法(IDEOM)使用微分滤波器成像。方法。 IDEOM是一种层析成像方法,它利用了费米卫星的轨道进动。使用IDEOM,已经在12–50 keV,50–100 keV和100–300 keV的能带中生成了大约4年的GBM数据的全天候重建,以寻找GBM掩埋分析无法建模的来源。结果。 IDEOM分析导致检测到12–50 keV能量带中的57个源,50–100 keV能量带中的23个源和100–300 keV能量带中的7个源。原始GBM-EOT目录中没有十七个来源,现在已添加。我们还介绍了GBM使用EOT和费米大面积望远镜(LAT)探测到的四个持久源的首次联合平均光谱:NGC 1275、3C 273,Cen A和Crab。

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