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K. Matsuoka

43 papers hereh-index 211.5k citations71 works total

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

author position
  • first author8
  • middle author24
  • last author6

Across the 38 of 43 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA30
  • astro-ph.CO10
  • astro-ph.HE3
same name
  • K. Matsuoka — 59 papers, h 20
  • K. Matsuoka — 31 papers, h 6
  • K. Matsuoka — 13 papers, h 15
  • K. Matsuoka — 12 papers
  • K. Matsuoka — 3 papers, h 6
  • K. Matsuoka — 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
20092024
most citedA statistical relation between the X-ray spectral index and Eddington ratio of active galactic nuclei in deep surveys

214 citations · 1.6k across the 43 of their papers we have counts for

collaborators
Showing 2016Show all

3 papers · 1 filter

astro-ph.GA2016★ 105 cited

The Complete Infrared View of Active Galactic Nuclei from the 70-month Swift/BAT Catalog

Kohei Ichikawa, Claudio Ricci, Yoshihiro Ueda +5

We systematically investigate the near- (NIR) to far-infrared (FIR) photometric properties of a nearly complete sample of local active galactic nuclei (AGN) detected in the Swift/B…

astro-ph.GA2016★ 15 cited

Near-infrared spectroscopy of nearby Seyfert galaxies: Is there evidence for the shock excitation in narrow-line regions?

Koki Terao, Tohru Nagao, Tetsuya Hashimoto +5

One of the unsettled, important problems in active galactic nuclei (AGNs) is the major ionization mechanism of gas clouds in their narrow-line regions (NLRs). In order to investiga…

astro-ph.GA2016★ 12 cited

Revisiting the Completeness and the Luminosity Function in High-Redshift Low-Luminosity Quasar Surveys

Mana Niida, Tohru Nagao, Hiroyuki Ikeda +4

Recent studies have derived quasar luminosity functions (QLFs) at various redshifts. However, the faint side of the QLF at high redshifts is still too uncertain. An accurate estima…

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