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Guanlin Li

Machine Intelligence and Translation Lab, Harbin Institute of Technology

10 papers hereh-index 8174 citations21 works total

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • first author4
  • middle author6

Across the 10 of 10 papers where every author was matched, so the position is known.

fields
  • astro-ph.SR4
  • cs.CL3
  • astro-ph.IM1
  • cs.CR1
  • cs.LG1
affiliations
  • Machine Intelligence and Translation Lab, Harbin Institute of Technology
Homepage
same name
  • Guanlin Li — 15 papers, h 7
  • Guanlin Li — 8 papers, h 4
  • Guanlin Li — 2 papers
  • Guanlin Li — 2 papers, h 4
  • GuanLin Li — 1 paper
  • Guanlin Li — 1 paper, h 1

Either other researchers who publish under this name, or the same person where the external sources have not merged their records.

identity via Semantic Scholar / OpenAlex

activity
20202023
most citedPhotometric observations of flares on AD Leo from GWAC-F30 and TESS

12 citations · 41 across the 10 of their papers we have counts for

collaborators
Showing 2023Show all

3 papers · 1 filter

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★ 12 cited

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.SR2023★ 4 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…

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Not affiliated with arXiv. Researcher data from Semantic Scholar (ODC-BY) and OpenAlex.