In-orbit calibration status of the Insight-HXMT
Xiaobo Li, Liming Song, Xufang Li, Ying Tan, Yanji Yang

TL;DR
The paper reports on the calibration status of China's Insight-HXMT X-ray satellite, detailing in-orbit calibration methods, accuracy, and adjustments for precise timing and spectral measurements.
Contribution
It provides the first comprehensive report on in-orbit calibration procedures and results for the Insight-HXMT satellite, including effective area adjustments and timing accuracy.
Findings
Calibration using radioactive sources and celestial objects
Achieved ~100 microsecond timing accuracy
Modified effective area with empirical adjustments
Abstract
As China's first X-ray astronomical satellite, Insight-HXMT (Hard X-ray Modulation Telescope) successfully launched on Jun 15, 2017. It performs timing and spectral studies of bright sources to determine their physical parameters. HXMT carries three main payloads onboard: the High Energy X-ray telescope (HE, 20-250 keV, NaI(Tl)/CsI(Na)), the Medium Energy X-ray Telescope (ME, 5-30 keV, Si-Pin) and the Low Energy X-ray telescope (LE, 1-15 keV, SCD). In orbit, we have used the radioactive sources, activated lines, the fluorescence line, and Cas A to calibrate the gain and energy resolution of the payloads. The Crab pulsar was adopted as the primary effective area calibrator and an empirical function was found to modify the simulated effective areas. The absolute timing accuracy of HXMT is about 100us from the TOA of Crab Pulsar.
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
Taxonomy
TopicsAstrophysical Phenomena and Observations · Pulsars and Gravitational Waves Research · Particle Detector Development and Performance
