329 citations · 723 across the 14 of their papers we have counts for
14 papers
Flare Quasi-Periodic Pulsation Associated with Recurrent Jets
Dong Li, Fanpeng Shi, Haisheng Zhao +6
Quasi-periodic pulsations (QPPs), which carry time features and plasma characteristics of flare emissions, are frequently observed in light curves of solar/stellar flares. In this…
The removal method and generation mechanism of spikes in Insight-HXMT/HE telescope
Baiyang Wu, Yifei Zhang, Xiaobo Li +5
Spikes are some obvious sharp increases that appear on the raw light curves of High Energy X-ray telescope(HE) onboard Insight-HXMT, which could have influences on the data product…
Detection of flare multi-periodic pulsations in mid-ultraviolet Balmer continuum, Ly-alpha, hard X-ray, and radio emissions simultaneously
Dong Li, Mingyu Ge, Marie Dominique +7
Quasi-periodic pulsations (QPPs), which usually appear as temporal pulsations of the total flux, are frequently detected in the light curves of solar/stellar flares. In this study,…
Insight-HXMT observations of jet-like corona in a black hole X-ray binary MAXI J1820+070
Bei You, Yuoli Tuo, Chengzhe Li +123
A black hole X-ray binary produces hard X-ray radiation from its corona and disk when the accreting matter heats up. During an outburst, the disk and corona co-evolves with each ot…
Comparison of simulated backgrounds with in-orbit observations for HE, ME and LE onboard Insight-HXMT
Juan Zhang, Xiaobo Li, Mingyu Ge +10
Insight-HXMT, the first X-ray astronomical satellite in China, aims to reveal new sources in the Galaxy and to study fundamental physics of X-ray binaries from 1\,keV to 250\,keV.…
Discovery of oscillations above 200 keV in a black hole X-ray binary with Insight-HXMT
Xiang Ma, Lian Tao, Shuang-Nan Zhang +119
Low-frequency quasi-periodic oscillations (LFQPOs) are commonly found in black hole X-ray binaries, and their origin is still under debate. The properties of LFQPOs at high energie…
Background Model for the High-Energy Telescope of Insight-HXMT
Jin-Yuan Liao, Shu Zhang, Xue-Feng Lu +20
Accurate background estimation is essential for spectral and temporal analysis in astrophysics. In this work, we construct the in-orbit background model for the High-Energy Telesco…
Background Model for the Low-Energy Telescope of Insight-HXMT
Jin-Yuan Liao, Shu Zhang, Yong Chen +16
With more than 150 blank sky observations at high Galactic latitude, we make a systematic study to the background of the Low Energy Telescope (LE) of the Hard X-ray Modulation Tele…
In-flight calibration of the Insight-Hard X-ray Modulation Telescope
Xiaobo Li, Xufang Li, Ying Tan +19
We present the calibration of the Insight-Hard X-ray Modulation Telescope (Insight-HXMT) X-ray satellite, which can be used to perform timing and spectral studies of bright X-ray s…
The Background Model of the Medium Energy X-ray telescope of Insight-HXMT
Cheng-Cheng Guo, Jin-Yuan Liao, Shu Zhang +26
The Medium Energy X-ray Telescope (ME) is one of the main payloads of the Hard X-ray Modulation Telescope (dubbed as Insight-HXMT). The background of Insight-HXMT/ME is mainly caus…
Overview to the Hard X-ray Modulation Telescope (Insight-HXMT) Satellite
ShuangNan Zhang, TiPei Li, FangJun Lu +127
As China's first X-ray astronomical satellite, the Hard X-ray Modulation Telescope (HXMT), which was dubbed as Insight-HXMT after the launch on June 15, 2017, is a wide-band (1-250…
Studies on the time response distribution of Insigh}-HXMT/LE
Xiao-Fan Zhao, Yu-Xuan Zhu, Da-Wei Han +105
The Hard X-ray Modulation Telescope (HXMT) named Insight is China's first X-ray astronomical satellite. The Low Energy X-ray Telescope (LE) is one of its main payloads onboard. The…
Insight-HXMT observations of Swift J0243.6+6124 during its 2017-2018 outburst
Yue Zhang, Mingyu Ge, Liming Song +107
The recently discovered neutron star transient Swift J0243.6+6124 has been monitored by {\it the Hard X-ray Modulation Telescope} ({\it Insight-\rm HXMT). Based on the obtained dat…
Insight-HXMT observations of the first binary neutron star merger GW170817
TiPei Li, ShaoLin Xiong, ShuangNan Zhang +107
Finding the electromagnetic (EM) counterpart of binary compact star merger, especially the binary neutron star (BNS) merger, is critically important for gravitational wave (GW) ast…