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Yongjun Chen

43 papers hereh-index 193.4k citations69 works total

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

author position
  • middle author23
  • last author2

Across the 25 of 43 papers where every author was matched, so the position is known.

fields
  • astro-ph.HE21
  • astro-ph.GA17
  • astro-ph.IM2
  • gr-qc2
  • astro-ph.CO1
same name
  • Yongjun Chen — 7 papers, h 6
  • Yongjun Chen — 7 papers, h 2
  • Yongjun Chen — 2 papers, h 5

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
20102026
most citedFirst M87 Event Horizon Telescope Results. II. Array and Instrumentation

1.1k citations · 5.3k across the 43 of their papers we have counts for

collaborators
Showing 2022Show all

4 papers · 1 filter

astro-ph.GA2022★ 4 cited

Radio continuum and OH line emission of high-z OH megamaser galaxies

Zhongzu Wu, Yu. V. Sotnikova, Bo Zhang +8

We present the study of arcsecond scale radio continuum and OH line emission of a sample of known OH megamaser galaxies with z≥ 0.15 using archival Very Large Array (VLA) dat…

astro-ph.HE2022★ 5 cited

The radio structure of the γ-ray narrow-line Seyfert 1 galaxy SDSS J211852.96−073227.5

Xi Shao, Minfeng Gu, Yongjun Chen +4

The γ-ray narrow-line Seyfert 1 (NLS1) galaxies can be considered to be the third class of γ-ray active galactic nuclei possessing relativistic jets. In this paper, we present…

astro-ph.HE2022★ 69 cited

The Photon Ring in M87*

Avery E. Broderick, Dominic W. Pesce, Paul Tiede +48

We report measurements of the gravitationally lensed secondary image -- the first in an infinite series of so-called "photon rings" -- around the supermassive black hole M87* via s…

astro-ph.GA2022★ 8 cited

Radio properties of the OH megamaser galaxy IIZw 096

Hong Wu, Zhongzu Wu, Yu. Sotnikova +9

Based on the two epochs EVN archive data from OH line observations of IIZw 096, we confirm that the high-resolution OH emission in this source mainly comes from two spots (OH1 and…

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