activity
20092025
most citedDesign and Construction of the BESIII Detector

1.2k citations · 1.9k across the 36 of their papers we have counts for

collaborators

36 papers

astro-ph.HE2025★ 4 cited

New insight into the Rapid Burster by Insight-HXMT

Y. P. Chen, S. Zhang, S. N. Zhang +91

We report the timing and spectral analyses upon of the type II X-ray bursts from the Rapid Burster (MXB 1730--335) observed by Insight-HXMT and Swift/XRT. By stacking the long-dura…

astro-ph.HE2023★ 21 cited

The First GECAM Observation Results on Terrestrial Gamma-ray Flashes and Terrestrial Electron Beams

Y. Zhao, J. C. Liu, S. L. Xiong +59

Gravitational-wave high-energy Electromagnetic Counterpart All-sky Monitor (GECAM) is a space-borne instrument dedicated to monitoring high-energy transients, including Terrestrial…

astro-ph.IM2021

The Design and Performance of Charged Particle Detector onboard the GECAM Mission

Y. B. Xu, X. L. Sun, S. Yang +47

The Gravitational Wave highly energetic Electromagnetic Counterpart All-sky Monitor (GECAM) is dedicated to detecting gravitational wave gamma-ray bursts. It is capable of all-sky…

astro-ph.IM2021★ 3 cited

Ground-based calibration and characterization of GRD of GECAM: 8-160 keV

J. J. He, Z. H. An, W. X. Peng +58

As the main detector of the GECAM satellite, the calibration of the energy response and detection efficiency of the GRD detector is the main content of the ground-based calibration…

astro-ph.IM2021★ 4 cited

The SiPM Array Data Acquisition Algorithm Applied to the GECAM Satellite Payload

Y. Q. Liu, K. Gong, X. Q. Li +47

The Gravitational Wave Burst High-energy Electromagnetic Counterpart All-sky Monitor (GECAM), consists of 2 small satellites that each contain 25 LaBr3 (lanthanum bromide doped wit…

astro-ph.IM2021★ 42 cited

The design and performance of GRD onboard the GECAM satellite

Z. H. An, X. L. Sun, D. L. Zhang +48

Background: Each GECAM satellite payload contains 25 gamma-ray detectors (GRDs), which can detect gamma-rays and particles and can roughly localize the Gamma-Ray Bursts (GRBs). GRD…

physics.ins-det2021★ 3 cited

Inflight performance of the GECAM Gamma-ray and Charge particle Detectors

X. Q. Li, X. Y. Wen, S. L. Xiong +56

The GECAM mission consists of two identical microsatellites (GECAM-A and GECAM-B). Each satellite is equipped with 25 gamma-ray detectors (GRD) and 8 charged particle detectors (CP…

hep-ex2021

Dedicated SiPM array for GRD of GECAM

D. L. Zhang, X. L. Sun, Z. H. An +45

The discovery of gravitational waves and gamma-ray bursts heralds the era of multi-messenger astronomy. With the adoption of two small satellites to achieve the all-sky monitoring…

astro-ph.HE2021★ 25 cited

Search for Gamma-Ray Bursts and Gravitational Wave Electromagnetic Counterparts with High Energy X-ray Telescope of \textit{Insight}-HXMT

C. Cai, S. L. Xiong, C. K. Li +96

The High Energy X-ray telescope (HE) on-board the Hard X-ray Modulation Telescope (\textit{Insight}-HXMT) can serve as a wide Field of View (FOV) gamma-ray monitor with high time r…

physics.ins-det2021

Quality assurance test and Failure Analysis of SiPM Arrays of GECAM Satellites

D. L. Zhang, M. Gao, X. L. Sun +45

The Gravitational wave high-energy Electromagnetic Counterpart All-sky Monitor (GECAM) satellite consists of two small satellites. Each GECAM payload contains 25 gamma ray detector…

astro-ph.HE2021

Broadband variability study of MAXI J1631-479 in its Hard-Intermediate State observed with Insight-HXMT

Q. C. Bu, S. N. Zhang, A. Santangelo +10

We report the energy-resolved broadband timing analysis of the black hole X-ray transient MAXI J1631-479 during its 2019 outburst from February 11 to April 9, using data from the I…

astro-ph.HE2021★ 1 cited

Accretion Torque Reversals in GRO J1008-57 Revealed by Insight-HXMT

W. Wang, Y. M. Tang, Y. L. Tuo +92

GRO J1008-57, as a Be/X-ray transient pulsar, is considered to have the highest magnetic field in known neutron star X-ray binary systems. Observational data of the X-ray outbursts…

astro-ph.HE2021★ 9 cited

QPOs and Orbital elements of X-ray binary 4U 0115+63 during the 2017 outburst observed by Insight-HXMT

Y. Z. Ding, W. Wang, P. Zhang +90

In this paper, we presented a detailed timing analysis of a prominent outburst of 4U 0115+63 detected by \textit{Insight}-HXMT in 2017 August. The spin period of the neutron star w…

astro-ph.HE2020★ 8 cited

X-ray reprocessing in accreting pulsar GX 301-2 observed with Insight-HXMT

L. Ji, V. Doroshenko, V. Suleimanov +100

We investigate the absorption and emission features in observations of GX 301-2 detected with Insight-HXMT/LE in 2017-2019. At different orbital phases, we found prominent Fe Kalph…

astro-ph.HE2020★ 17 cited

Insight-HXMT observations of a possible fast transition from jet to wind dominated state during a huge flare of GRS~1915+105

L. D. Kong, S. Zhang, Y. P. Chen +92

We present the analysis of the brightest flare that was recorded in the \emph{Insight}-HMXT data set, in a broad energy range (2200 keV) from the microquasar GRS~1915+105 during…

astro-ph.HE2020★ 36 cited

Physical origin of the nonphysical spin evolution of MAXI J1820+070

J. Guan, L. Tao, J. L. Qu +91

We report on the Insight-HXMT observations of the new black hole X-ray binary MAXI J1820+070 during its 2018 outburst. Detailed spectral analysis via the continuum fitting method s…

astro-ph.HE2020★ 30 cited

A variable ionized disk wind in the black-hole candidate EXO 1846-031

Yanan Wang, Long Ji, Javier A. Garcia +88

After 34 years, the black-hole candidate EXO 1846-031 went into outburst again in 2019. We investigate its spectral properties in the hard intermediate and the soft states with NuS…

astro-ph.HE2020★ 12 cited

Constraining the transient high-energy activity of FRB180916.J0158+65 with Insight-HXMT followup observations

C. Guidorzi, M. Orlandini, F. Frontera +96

A link between magnetars and fast radio burst (FRB) sources has finally been established. In this context, one of the open issues is whether/which sources of extra galactic FRBs ex…

astro-ph.HE2020★ 22 cited

Insight-HXMT firm detection of the highest energy fundamental cyclotron resonance scattering feature in the spectrum of GRO J1008-57

M. Y. Ge, L. Ji, S. N. Zhang +118

We report on the observation of the accreting pulsar GRO J1008-57 performed by Insight-HXMT at the peak of the source's 2017 outburst. Pulsations are detected with a spin period of…

astro-ph.HE2020★ 3 cited

Insight-HXMT insight into switch of the accretion mode: the case of the X-ray pulsar 4U 1901+03

Y. L. Tuo, L. Ji, S. S. Tsygankov +116

We use the In data collected during the 2019 outburst from X-ray pulsar 4U 1901+03 to complement the orbital parameters reported by Fermi/GBM. Using the Insight-HXMT, we examine th…

astro-ph.HE2020★ 34 cited

The evolution of the broadband temporal features observed in the black-hole transient MAXI J1820+070 with Insight-HXMT

Yanan Wang, Long Ji, S. N. Zhang +117

We study the evolution of the temporal properties of MAXI 1820+070 during the 2018 outburst in its hard state from MJD 58190 to 58289 with Insight-HXMT in a broad energy band 1-150…

astro-ph.HE2020★ 19 cited

Discovery of delayed spin-up behavior following two large glitches in the Crab pulsar, and the statistics of such processes

M. Y. Ge, S. N. Zhang, F. J. Lu +130

Glitches correspond to sudden jumps of rotation frequency () and its derivative () of pulsars, the origin of which remains not well understood yet, partly because the jum…

astro-ph.HE2020★ 30 cited

A search for prompt gamma-ray counterparts to fast radio bursts in the Insight-HXMT data

C. Guidorzi, M. Marongiu, R. Martone +118

No robust detection of prompt electromagnetic counterparts to fast radio bursts (FRBs) has yet been obtained, in spite of several multi-wavelength searches carried out so far. Spec…

astro-ph.HE2020★ 13 cited

Switches between accretion structures during flares in 4U 1901+03

L. Ji, L. Ducci, A. Santangelo +120

We report on our analysis of the 2019 outburst of the X-ray accreting pulsar 4U 1901+03 observed with Insight-HXMT and NICER. Both spectra and pulse profiles evolve significantly i…