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researcher

A. Moiseev

4 papers hereh-index 17 citations9 works total

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

author position
  • middle author2
  • last author1

Across the 3 of 4 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA3
  • astro-ph.HE1
same name
  • A. Moiseev — 69 papers, h 21
  • A. Moiseev — 47 papers, h 91
  • A. Moiseev — 10 papers, h 10
  • A. Moiseev — 7 papers, h 13
  • A. Moiseev — 3 papers, h 6
  • A. Moiseev — 3 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
20242026
most citedThe most distant HI galaxies discovered by the 500 m dish FAST

16 citations · 16 across the 2 of their papers we have counts for

collaborators

4 papers

astro-ph.HE2026

New galaxy cluster in the Zone of Avoidance SRGe CL0512.7+3712. Discovery and multi-wavelength characterization

Ildar Khabibullin, Eugene Churazov, Natalya Lyskova +9

The census of massive clusters of galaxies in the local Universe is almost complete, thanks to their prominent observational signatures at X-ray, optical, and sub-mm wavelengths. N…

astro-ph.GA2025

Green Bean galaxies and the fading echoes of AGN activity

A. Arshinova, K. Sanderson, A. Moiseev

Green Bean is a rare type of galaxy which represents a short-lived phase in the life cycle of active galactic nuclei (AGN), characterised by large-scale, powerful ionised clouds in…

astro-ph.GA2025

Chemodynamic evidence of pristine gas accretion in the void galaxy VGS 12

Evgeniya Egorova, Kathryn Kreckel, Oleg Egorov +5

Accretion of metal-poor gas is expected to be an important channel of gas replenishment in galaxy evolution studies. However, observational evidence of this process is still relati…

astro-ph.GA2024★ 16 cited

The most distant HI galaxies discovered by the 500 m dish FAST

Hongwei Xi, Bo Peng, Lister Staveley-Smith +20

Neutral hydrogen (HI) is the primary component of the cool interstellar medium (ISM) and is the reservoir of fuel for star formation. Owing to the sensitivity of existing radio tel…

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