Insight-HXMT measurements of the diffuse X-ray background

R. Huang,W. Cui, J. Y. Liao,S. Zhang,S. F. Wang, J. Jin, X. F. Lu, C. C. Guo, Y. You,G. Li,J. Zhang

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY(2022)

引用 2|浏览35
暂无评分
摘要
We present an X-ray spectrum of the diffuse X-ray background (DXRB) between 1.5 and 120 keV, as measured with the Low-Energy Detector (LE) and the High-Energy Detector (HE) aboard the Insight-HXMT satellite, based on 'blank-sky' observations. LE covers a nominal energy range of 1-15 keV and HE 20-250 keV, but calibration issues and data quality narrowed the energy range for this work. The LE background was directly measured with 'blind' detector modules, while the HE background was derived from Earth-occultation data. With the LE data alone, the measured DXRB spectrum can be well-described by a power law; fitting the LE and HE data jointly, however, a spectral cut-off must be introduced in the model to account for the measurements above 30 keV. Modelling the combined spectrum with a cut-off power law, the best-fitting photon index is 1.40, normalization 9.57 ph cm(-2) s(-1) keV(-1) sr(-1) (at 1 keV), and cut-off energy 55 keV after correcting for the effects of the Earth albedo and atmospheric emission (which are significant in the HE band). Based on the best-fitting cut-off power law, we derived the spectral energy distribution (SED) of the DXRB. The shape of the SED is in general agreement with the published measurements, but the overall normalization is lower by varying amounts, except for the HEAO-1 result, with which our result is in good agreement.
更多
查看译文
关键词
instrumentation: detectors, X-rays: diffuse background, X-rays: general
AI 理解论文
溯源树
样例
生成溯源树,研究论文发展脉络
Chat Paper
正在生成论文摘要