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

17 citations · 22 across the 4 of their papers we have counts for

collaborators

6 papers

astro-ph.SR2023

White-light superflare and long-term activity of the nearby M7 type binary EI~Cnc observed with GWAC system

Hua-Li Li, Jing Wang, Li-Ping Xin +14

Stellar white-light flares are believed to play an essential role on the physical and chemical properties of the atmosphere of the surrounding exoplanets. Here we report an optical…

astro-ph.SR2023

Photometric observations of flares on AD Leo from GWAC-F30 and TESS

Jian-Ying Bai, Jing Wang, Hua-Li Li +4

We observed active M dwarf star AD Leo for 146 hr in photometry by GWAC-F30 and also analyzed 528-hr photometric data of the star from TESS. A total of 9 and 70 flares are detected…

astro-ph.IM2023

Sciences with the 2.5-meter Wide Field Survey Telescope (WFST)

WFST Collaboration, Tinggui Wang, Guilin Liu +60

The Wide Field Survey Telescope (WFST) is a dedicated photometric surveying facility being built jointly by the University of Science and Technology of China and the Purple Mountai…

cs.CV20231 cited

AutoKary2022: A Large-Scale Densely Annotated Dataset for Chromosome Instance Segmentation

Dan You, Pengcheng Xia, Qiuzhu Chen +3

Automated chromosome instance segmentation from metaphase cell microscopic images is critical for the diagnosis of chromosomal disorders (i.e., karyotype analysis). However, it is…

astro-ph.HE202317 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.SR20234 cited

A huge-amplitude white-light superflare on a L0 brown dwarf discovered by GWAC survey

Li-Ping Xin, Hua-li Li, Jing Wang +21

White-light superflares from ultra cool stars are thought to be resulted from magnetic reconnection, but the magnetic dynamics in a fully convective star is not clear yet. In this…