Pith. sign in

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

1 Pith paper cite this work. Polarity classification is still indexing.

1 Pith paper citing it
abstract

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, where NaI(Tl) serves as the primary detector covering 20--250\,keV, and CsI(Na) is used as an active shield detector to suppress the background of NaI(Tl) and also serves as an all-sky gamma-ray burst monitor covering 0.2--3\,MeV. In this paper, we review the in-orbit performance of HE in the first 5 years since \textit{Insight}-HXMT was launched on June 15, 2017. Methods: The major performances we concern include the gain and energy resolution of NaI(Tl) and CsI(Na) detectors, the performance of pulse-shape-discriminator (PSD) and system dead-time. In this work, we investigate these performances mainly using the data of blank-sky observations and the data when the telescope in earth occultation. Results: The overall performance of HE/NaI(Tl) is very stable in the first 5 years, whereas the gain of HE/CsI(Na) shows a continuously increasing trend and should be calibrated regularly. Conclusion: In general, HE is still in good health and well-calibrated status after five-year's operation. The in-orbit performance of HE has no significant deviation from expectation. HE is expected to be in operation healthily for another several years of extended mission life.

fields

astro-ph.HE 1

years

2025 1

verdicts

CONDITIONAL 1

representative citing papers

Insight-HXMT observations of the extremely bright GRB 221009A

astro-ph.HE · 2025-04-26 · conditional · novelty 6.0

Insight-HXMT's ME and LE telescopes, detecting secondary particles rather than direct gamma rays, recovered the main burst light curve of GRB 221009A and measured a minimum variability timescale of 0.10 s.

citing papers explorer

Showing 1 of 1 citing paper.

  • Insight-HXMT observations of the extremely bright GRB 221009A astro-ph.HE · 2025-04-26 · conditional · none · ref 32 · internal anchor

    Insight-HXMT's ME and LE telescopes, detecting secondary particles rather than direct gamma rays, recovered the main burst light curve of GRB 221009A and measured a minimum variability timescale of 0.10 s.