activity
20132023
most citedOverview to the Hard X-ray Modulation Telescope (Insight-HXMT) Satellite

329 citations · 708 across the 25 of their papers we have counts for

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Showing 2023Show all

6 papers · 1 filter

astro-ph.IM2023★ 3 cited

Insight-HXMT on-orbit thermal control status and thermal deformation impact analysis

Aimei Zhang, Yifan Zhang, Jinyuan Liao +23

Purpose: The Hard X-ray Modulation Telescope is China's first X-ray astronomy satellite launched on June 15th, 2017, dubbed Insight-HXMT. Active and passive thermal control measure…

astro-ph.HE2023★ 2 cited

Insight-HXMT Measurements of the Diffuse X-ray Background

Rui Huang, Wei Cui, Jin-Yuan Liao +8

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…

astro-ph.HE2023★ 33 cited

Insight-HXMT and GECAM-C observations of the brightest-of-all-time GRB 221009A

Zheng-Hua An, S. Antier, Xing-Zi Bi +174

GRB 221009A is the brightest gamma-ray burst ever detected since the discovery of this kind of energetic explosions. However, an accurate measurement of the prompt emission propert…

astro-ph.IM2023

Five-year in-orbit background of Insight-HXMT

Jin-Yuan Liao, Shu Zhang, Juan Zhang +24

Purpose: We present the five-year in-orbit background evolution of Insight-HXMT since the launch, as well as the effects of the background model in data analysis. Methods: The back…

astro-ph.IM2023

In-orbit performance of HE onboard Insight-HXMT in the first 5 years

Xu-Fang Li, Cong-Zhan Liu, Yi-Fei Zhang +10

Purpose: The High-Energy X-ray telescope (HE), one of the three main payloads of the \textit{Insight}-HXMT mission, is composed of eighteen NaI(Tl)/CsI(Na) phoswich detectors, wher…

astro-ph.HE2023★ 4 cited

Burst phase distribution of SGR J1935+2154 based on Insight-HXMT

Xuefeng Lu, Liming Song, Mingyu Ge +10

On April 27, 2020, the soft gamma ray repeater SGR J1935+2154 entered its intense outburst episode again. Insight-HXMT carried out about one month observation of the source. A tota…