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researcher

E. Capote

88 papers hereh-index 357k citations106 works total

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

author position
  • first author2
  • middle author19
  • last author1

Across the 22 of 88 papers where every author was matched, so the position is known.

fields
  • gr-qc47
  • astro-ph.HE25
  • astro-ph.CO7
  • astro-ph.IM7
  • physics.ins-det1
  • quant-ph1
same name
  • E. Capote — 4 papers
  • E. Capote — 1 paper
  • E. Capote — 1 paper
  • E. Capote — 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
20202026
most citedGWTC-3: Compact Binary Coalescences Observed by LIGO and Virgo During the Second Part of the Third Observing Run

1.8k citations · 5.4k across the 86 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.