activity
20042023
most citedVery high energy gamma-ray emission beyond 10 TeV from GRB 221009A

112 citations · 113 across the 2 of their papers we have counts for

collaborators

6 papers

astro-ph.HE2023112 cited

Very high energy gamma-ray emission beyond 10 TeV from GRB 221009A

Zhen Cao, F. Aharonian, Q. An +276

The highest energy gamma-rays from gamma-ray bursts (GRBs) have important implications for their radiation mechanism. Here we report for the first time the detection of gamma-rays…

astro-ph.SR20211 cited

Non-thermal electron energization during the impulsive phase of an X9.3 flare revealed by Insight-HXMT

P. Zhang, W. Wang, Y. Su +8

The X9.3 flare SOL20170906T11:55 was observed by the CsI detector aboard the first Chinese X-ray observatory Hard X-ray Modulation telescope (Insight-HXMT). By using wavelets metho…

astro-ph.IM2021

Calibration of the Air Shower Energy Scale of the Water and Air Cherenkov Techniques in the LHAASO experiment

F. Aharonian, Q. An, Axikegu +246

The Wide Field-of-View Cherenkov Telescope Array (WFCTA) and the Water Cherenkov Detector Arrays (WCDA) of LHAASO are designed to work in combination for measuring the energy spect…

physics.ins-det2020

Construction and On-site Performance of the LHAASO WFCTA Camera

F. Aharonian, Q. An, Axikegu +246

The focal plane camera is the core component of the Wide Field-of-view Cherenkov/fluorescence Telescope Array (WFCTA) of the Large High-Altitude Air Shower Observatory (LHAASO). Be…

astro-ph.HE2020

The observation of the Crab Nebula with LHAASO-KM2A for the performance study

F. Aharonian, Q. An, Axikegu +246

As a sub-array of the Large High Altitude Air Shower Observatory (LHAASO), KM2A is mainly designed to cover a large fraction of the northern sky to hunt for gamma-ray sources at en…

astro-ph2004

A Radio Outburst Nearly Coincident with the Large X-ray Flare from Sgr A* on 2002-10-03

Jun-Hui Zhao, R. M. Herrnstein, G. C. Bower +2

A large radio outburst from Sgr A* was observed during the VLA weekly monitoring program at 2 cm, 1.3 cm and 7 mm, nearly coincident with the brightest X-ray flare detected to date…