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researcher

W. Kang

25 papers hereh-index 14438 citations77 works total

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

author position
  • first author2
  • middle author21
  • last author1

Across the 24 of 25 papers where every author was matched, so the position is known.

fields
  • astro-ph.SR10
  • astro-ph.GA7
  • astro-ph.EP5
  • astro-ph.CO1
  • astro-ph.HE1
  • astro-ph.IM1
same name
  • W. Kang — 152 papers, h 44
  • W. Kang — 81 papers, h 7
  • W. Kang — 55 papers, h 26
  • W. Kang — 30 papers, h 28
  • W. Kang — 21 papers, h 41
  • W. Kang — 17 papers, h 13

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
20112023
most citedAbundances of Refractory Elements for G-type Stars with Extrasolar Planets

54 citations · 431 across the 23 of their papers we have counts for

collaborators
Showing 2023Show all

3 papers · 1 filter

astro-ph.GA2023

The Seoul National University AGN Monitoring Project IV: Hα reverberation mapping of 6 AGNs and the Hα Size-Luminosity Relation

Hojin Cho, Jong-Hak Woo, Shu Wang +29

The broad line region (BLR) size-luminosity relation has paramount importance for estimating the mass of black holes in active galactic nuclei (AGNs). Traditionally, the size of th…

astro-ph.IM2023★ 11 cited

The Capella Program: Toward A Space-only High-frequency Radio VLBI Network Formed by Small Satellites in Low Earth Orbits

Sascha Trippe, Taehyun Jung, Jung-Won Lee +11

Very long baseline radio interferometry (VLBI) with ground-based observatories is limited by the size of Earth, the geographic distribution of antennas, and the transparency of the…

astro-ph.SR2023★ 11 cited

The Early Light Curve of a Type Ia Supernova 2021hpr in NGC 3147: Progenitor Constraints with the Companion Interaction Model

Gu Lim, Myungshin Im, Gregory S. H. Paek +19

The progenitor system of Type Ia supernovae (SNe Ia) is expected to be a close binary system of a carbon/oxygen white dwarf (WD) and a non-degenerate star or another WD. Here, we p…

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