activity
20172026
most citedOverview to the Hard X-ray Modulation Telescope (Insight-HXMT) Satellite

329 citations · 1.2k across the 64 of their papers we have counts for

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12 papers · 1 filter

astro-ph.HE2026★ 1 cited

Search for the Highest-energy Quasiperiodic Oscillation in the Black Hole X-Ray Binary Candidate Swift J1727.8-1613

Xiang Ma, Qing-Cang Shui, Ming-Yu Ge +8

We report the first detection of a low-frequency quasiperiodic oscillation (QPO) extending above 250 keV in the black hole X-ray binary candidate Swift J1727.8-1613 using Insight-H…

astro-ph.HE2026

An Insight-HXMT View of the Evolution of the Type-C Quasiperiodic Oscillation during the Flaring State of Swift J1727.8-1613

Min Wei, Xiang Ma, Liang Zhang +16

We present a detailed analysis of the evolution of type-C quasiperiodic oscillations (QPOs) observed during the flaring state of the recently discovered black hole X-ray binary Swi…

astro-ph.HE2026

Unveiling hidden millihertz quasi-periodic oscillations in 1A 0535+262

Zihan Yang, Ruican Ma, Mariano Méndez +9

Be/X-ray binary pulsars show transient outbursts and complex timing behaviour, including millihertz quasi-periodic oscillations (QPOs), whose physical origin and energy dependence…

astro-ph.IM2026

The trigger and localization system of SVOM-GRM

Jiang He, Jian-Chao Sun, Yue Huang +20

The Space multi-band Variable Object Monitor (SVOM) is an astronomical satellite jointly developed by China and France, primarily focused on the detection of gamma-ray bursts (GRBs…

astro-ph.HE2026

The GRB joint scientific analysis pipeline of the ECLAIRs and GRM instruments on board SVOM

F. Piron, F. Daigne, T. Maiolino +35

The study of the prompt high-energy emission of Gamma-Ray Bursts (GRBs) with SVOM relies on the observations performed by ECLAIRs (4-150 keV) and the Gamma-Ray Monitor (GRM, 0.015-…

astro-ph.IM2026

The Gamma-Ray Monitor onboard the SVOM satellite

Jian-Chao Sun, Yong-Wei Dong, Jiang He +21

The Gamma-Ray Monitor (GRM) is a key scientific payload onboard the Space-based Multi-band Variable Object Monitor (SVOM) satellite, designed specifically for the detection and stu…

astro-ph.HE2026

Study on the detector energy response of SVOM/GRM

Xiao-Yun Zhao, Jiang He, Shi-Jie Zheng +32

The SVOM mission is specifically designed to for the detection and localization of Gamma-Ray Bursts (GRBs) and subsequent follow-up observations. Among the four telescopes installe…

astro-ph.HE2026

Comprehensive Measurement of Spectral Evolution in a GRB Flare: High Time-Resolution Insights into the "Double-Tracking" Phenomenon

Zheng-Hang Yu, Wen-Jun Tan, Chen-Wei Wang +41

The spectral evolution characteristics of the prompt emission in gamma-ray bursts (GRBs) have been extensively studied, but detailed investigations of spectral evolution in a GRB f…

astro-ph.EP2026

High-resolution spectroscopic atmospheric studies of 5 hot Jupiters across the edge of the Neptune desert

Zewen Jiang, Wei Wang, Shumei Jia +6

Hot Jupiters (HJs), especially the Ultra-Hot Jupiters (UHJs), are ideal targets for robust atmospheric characterization, thanks to their high equilibrium temperatures and large atm…

astro-ph.IM2026

A New Method for Identifying Contaminating Sources and Locating Target Sources through the Cross-Arm Features of Micro Pore Optics

Yiming Huang, Lian Tao, Jin-Yuan Liao +15

The Pathfinder of the Type-A satellites in the Chasing All Transients Constellation Hunters (CATCH) space mission is equipped with Micro-Pore Optics (MPOs) and four single-pixel Si…

astro-ph.HE2026★ 1 cited

X-ray and radio observations of the AMXP MAXI J1957+032 covering the 2022-2025 outbursts

Zhaosheng Li, Lucien Kuiper, Yuanyue Pan +12

We presented a comprehensive multi-epoch timing and multiwavelength analysis of the accreting millisecond X-ray pulsar MAXI J1957+032, covering two major outbursts in 2022 and 2025…

astro-ph.HE2026★ 1 cited

Characteristics of the High-frequency Humps in the Black hole X-ray Binary Swift J1727.8--1613

Ze-Xi Li, Liang Zhang, Lian Tao +13

We present a detailed timing analysis of the two high-frequency humps observed in the power density spectrum of Swift J1727.8--1613 up to 100 keV, using data from the Hard X-ray Mo…