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researcher

I. Katkov

50 papers hereh-index 14601 citations69 works total

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

author position
  • sole author1
  • first author12
  • middle author22
  • last author13

Across the 48 of 50 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA39
  • astro-ph.CO6
  • astro-ph.IM4
  • astro-ph.HE1
same name
  • I. Katkov — 94 papers
  • I. Katkov — 92 papers, h 121
  • I. Katkov — 30 papers, h 5
  • I. Katkov — 21 papers
  • I. Katkov — 21 papers
  • I. Katkov — 20 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
20102026
most citedA Population of Bona Fide Intermediate Mass Black Holes Identified as Low Luminosity Active Galactic Nuclei

157 citations · 771 across the 50 of their papers we have counts for

collaborators
Showing 2018 · astro-ph.GAShow all

3 papers · 2 filters

astro-ph.GA2018★ 27 cited

A Malin 1 'cousin' with counter-rotation: internal dynamics and stellar content of the giant low surface brightness galaxy UGC 1922

Anna S. Saburova, Igor V. Chilingarian, Ivan Yu. Katkov +5

The formation scenario for giant low surface brightness (gLSB) galaxies with discs as large as 100 kpc still remains unclear. These stellar systems are rare and very hard to observ…

astro-ph.GA2018★ 12 cited

The imprint of the thick stellar disc in the mid-plane of three early-type edge-on galaxies in the Fornax cluster

Ivan Yu. Katkov, Alexei Yu. Kniazev, Anastasia V. Kasparova +1

Galactic stellar discs, such as that of the Milky Way, have usually a complex structure consisting of a thin and a thick component. The study of galactic disc substructures and the…

astro-ph.GA2018★ 157 cited

A Population of Bona Fide Intermediate Mass Black Holes Identified as Low Luminosity Active Galactic Nuclei

Igor V. Chilingarian, Ivan Yu. Katkov, Ivan Yu. Zolotukhin +4

Nearly every massive galaxy harbors a supermassive black hole (SMBH) in its nucleus. SMBH masses are millions to billions M⊙​, and they correlate with properties of spheroi…

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