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Xiaofeng Li

4 papers hereh-index 349 citations9 works total

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

author position
  • first author2
  • middle author1
  • last author1

Across the 4 of 4 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA2
  • astro-ph.HE2
same name
  • Xiaofeng Li — 8 papers, h 3
  • Xiaofeng Li — 6 papers, h 8
  • Xiaofeng Li — 4 papers, h 17
  • Xiaofeng Li — 4 papers, h 5
  • Xiaofeng Li — 3 papers, h 33
  • Xiaofeng Li — 2 papers

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
20182023
most citedImaging and variability studies of CTA~102 during the 2016 January γ-ray flare

21 citations · 35 across the 4 of their papers we have counts for

collaborators

4 papers

astro-ph.HE2023

Toward Microarcsecond Astrometry for the Innermost Wobbling Jet of the BL Lacertae Object OJ 287

Xiaopeng Cheng, Jun Yang, Guang-Yao Zhao +3

The BL Lacertae object OJ 287 is a very unusual quasar producing a wobbling radio jet and some double-peaked optical outbursts with a possible period of about 12 yr for more than o…

astro-ph.GA2020★ 14 cited

The parsec-scale jet of the neutrino-emitting blazar TXS~0506+056

Xiaofeng Li, Tao An, Prashanth Mohan +1

Recently the IceCube collaboration detected very high energy (VHE) neutrinos and associated them with the blazar \txs{}, raising a possible association of VHE neutrinos with this a…

astro-ph.GA2019

Features of Structure and Absorption in the Jet-Launching Region of M87

Wei Zhao, Xiaoyu Hong, Tao An +3

M87 is one of the best available source for studying the AGN jet-launching region. To enrich our knowledge of this region, with quasi-simultaneous observations using VLBA at 22, 43…

astro-ph.HE2018★ 21 cited

Imaging and variability studies of CTA~102 during the 2016 January γ-ray flare

Xiaofeng Li, P. Mohan, T. An +6

The γ-ray bright blazar CTA 102 is studied using imaging (new 15 GHz and archival 43 GHz Very Long Baseline Array, VLBA data) and time variable optical flux density, polarization…

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