activity
20102026
most citedThe first six months of the Advanced LIGO's and Advanced Virgo's third observing run with GRANDMA

76 citations · 288 across the 32 of their papers we have counts for

collaborators
Showing astro-ph.HEShow all

16 papers · 1 filter

astro-ph.HE2026

Fast Optical Variability of the TeV Blazar PKS 1725+123 Observed by SVOM-VT and Insights from Multi-wavelength Follow-up Observations

Shuo-Yu Liu, Yu-Wei Yu, Ji-Shun Lian +29

PKS 1725+123 is a flat-spectrum radio quasar (FSRQ) with a redshift of . The detection of this object in the TeV band was reported by the MAGIC telescopes and H.E.S.S. in…

astro-ph.HE2026

Early results from the SVOM Observatory Science program

A. Coleiro, L. Tao, F. Cangemi +44

We present the organisation and early results from the Observatory Science program of the Space-based multi-band astronomical Variable Objects Monitor (SVOM), based on data collect…

astro-ph.HE2026

SVOM/VT: Overview of data processing and GRB identifications with X-band data

Hua-Li Li, Yu-Lei Qiu, Li-Ping Xin +16

VT (the Visible Telescope) is an optical telescope onboard the SVOM (Space-based Multi-band Astronomical Variable Objects Monitor) mission, specifically designed to detect optical…

astro-ph.HE2026

SVOM/VT: Preliminary Calibration Analysis

Zhu-Heng Yao, Yu-Lei Qiu, Jin-Song Deng +9

We present the in-orbit calibration of the Visible Telescope (VT), one of the key instruments aboard the Space Variable Objects Monitor (SVOM) mission for gamma-ray burst (GRB) stu…

astro-ph.HE2026

SVOM/VT: Instrument Overview, Science Objectives, and First-Year Performance

Yu-Lei Qiu, Li-Ping Xin, Jin-Song Deng +22

The 44-cm Visible Telescope (VT) aboard the Space-based Variable Objects Monitor (SVOM) is a dual-band (400-650 nm and 650-1000 nm) instrument designed to detect and characterize t…

astro-ph.HE2026

Detection of Oscillations in a Type I X-Ray Burst of 4U 0614+091 with SVOM/ECLAIRs

Sébastien Le Stum, Floriane Cangemi, Alexis Coleiro +29

On 2025 January 10, a thermonuclear (Type I) X-ray burst from the neutron star low-mass X-ray binary \textit{4U~0614+091} was detected with the ECLAIRs instrument on board the \tex…

astro-ph.HE2026

Minutes-long soft X-ray prompt emission from a compact object merger

An Li, Chen-Wei Wang, Niccolò Passaleva +75

Compact object mergers are multi-messenger sources and known progenitors of some gamma-ray bursts, bright flashes of high-energy radiation powered by a central engine, either an ac…

astro-ph.HE2024

Simultaneous Multiband Photometry of the Early Optical Afterglow of GRB 240825A with Mephisto

Yehao Cheng, Yu Pan, Yuan-Pei Yang +19

Gamma-ray bursts (GRBs) are the most luminous transients in the universe. The interaction of the relativistic jet with the circumburst medium produces an afterglow and generates mu…

astro-ph.HE2023★ 17 cited

Prompt-to-afterglow transition of optical emission in a long gamma-ray burst consistent with a fireball

Liping Xin, Xuhui Han, Huali Li +19

Long gamma-ray bursts (GRBs), which signify the end-life collapsing of very massive stars, are produced by extremely relativistic jets colliding into circumstellar medium. Huge ene…

astro-ph.HE2022★ 8 cited

Photometric and Spectroscopic Observations of GRB 210104A: Bright Reverse shock Emission and Dense Circumburst Environment

Lu-Lu Zhang, Li-Ping Xin, Jing Wang +6

Early afterglow observations of gamma-ray bursts (GRBs) are valuable for exploring the properties of their jets and ambient medium. We report our photometric and spectroscopic obse…

astro-ph.HE2020★ 12 cited

Distribution of Si II 6355 Velocities of Type Ia Supernovae and Implications for Asymmetric Explosions

Keto D. Zhang, WeiKang Zheng, Thomas de Jaeger +7

The ejecta velocity is a very important parameter in studying the structure and properties of Type Ia supernovae (SNe Ia). It is also a candidate key parameter in improving the uti…

astro-ph.HE2019★ 76 cited

The first six months of the Advanced LIGO's and Advanced Virgo's third observing run with GRANDMA

S. Antier, S. Agayeva, V. Aivazyan +74

We present the Global Rapid Advanced Network Devoted to the Multi-messenger Addicts (GRANDMA). The network consists of 21 telescopes with both photometric and spectroscopic facilit…

astro-ph.HE2018★ 5 cited

Photometric and Spectroscopic Observations of GRB 140629A

Li-Ping Xin, Shu-Qing Zhong, En-Wei Liang +8

We present our optical photometric and spectroscopical observations of GRB 140629A. A redshift of is measured through the metal absorption lines in our spectrosco…

astro-ph.HE2016★ 13 cited

Variations of in subpulse drifting pulsars

R. Yuen, D. B. Melrose, M. A. Samsuddin +2

We develop a model for subpulse separation period, , taking into account both the apparent motion of the visible point as a function of pulsar phase, , and the possibility…

astro-ph.HE2015★ 3 cited

Optical light curve of GRB 121011A: a textbook for the onset of GRB afterglow in a mixture of ISM and wind-type medium

Li-Ping Xin, Jian-Yan Wei, Yu-Lei Qiu +3

We reported the optical observations of GRB 121011A by 0.8-m TNT telescope at Xinglong observatory, China. The light curve of optical afterglow shows a smooth and featureless bump…

astro-ph.HE2010★ 54 cited

Probing the Nature of High-z Short GRB 090426 with Its Early Optical and X-ray Afterglows

Liping Xin, Enwei Liang, Jianyan Wei +13

GRB 090426 is a short duration burst detected by Swift ( s in the observer frame, and s in the burst frame at ). Its host galaxy propert…