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researcher

A. Basalaev

34 papers hereh-index 12671 citations40 works total

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

author position
  • middle author14

Across the 14 of 34 papers where every author was matched, so the position is known.

fields
  • gr-qc22
  • astro-ph.HE6
  • astro-ph.CO4
  • astro-ph.IM1
  • physics.ins-det1
same name
  • A. Basalaev — 80 papers, h 59
  • A. Basalaev — 62 papers
  • A. Basalaev — 9 papers
  • A. Basalaev — 5 papers
  • A. Basalaev — 3 papers
  • A. Basalaev — 1 paper, h 1

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 citedGW231123: a Binary Black Hole Merger with Total Mass 190-265 M⊙​

121 citations · 273 across the 33 of their papers we have counts for

collaborators
Showing 2026 · astro-ph.HEShow all

3 papers · 2 filters

astro-ph.HE2026

Sub-Torque-Balance Upper Limits on Continuous Gravitational Waves from Scorpius X-1

The LIGO Scientific Collaboration, the Virgo Collaboration, the KAGRA Collaboration +1836

We present the results of a search for continuous gravitational waves from the low-mass X-ray binary Scorpius X-1 using LIGO data from the first part of the fourth LIGO-Virgo-KAGRA…

astro-ph.HE2026

GWTC-5.0: Population Properties of Merging Compact Binaries

The LIGO Scientific Collaboration, the Virgo Collaboration, the KAGRA Collaboration +1813

We present the population properties of merging compact binaries inferred using 267 mergers from the cumulative Gravitational-Wave Transient Catalog 5.0. As this data set contains…

astro-ph.HE2026

Searches for Binary Mergers with Sub-solar Mass Components in Data from the First Part of LIGO--Virgo--KAGRA's Fourth Observing Run

The LIGO Scientific Collaboration, the Virgo Collaboration, the KAGRA Collaboration +1832

We report on a gravitational wave search for compact binary coalescences involving at least one component with mass between 0.2M⊙​ to 1M⊙​, and ratio of component m…

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