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researcher

I. W. Harry

86 papers here

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

author position
  • middle author3

Across the 3 of 86 papers where every author was matched, so the position is known.

fields
  • gr-qc46
  • astro-ph.HE27
  • astro-ph.CO6
  • astro-ph.IM5
  • astro-ph2
ORCID 0000-0002-5304-9372
same name
  • I. W. Harry — 5 papers
  • I. W. Harry — 3 papers
  • I. W. Harry — 2 papers
  • I. W. Harry — 2 papers
  • I. W. Harry — 1 paper
  • I. W. Harry — 1 paper

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
20032026
most citedGW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral

9.8k citations · 37.2k across the 86 of their papers we have counts for

collaborators
Showing 2019Show all

3 papers · 1 filter

astro-ph.HE2019★ 127 cited

Search for Eccentric Binary Black Hole Mergers with Advanced LIGO and Advanced Virgo during their First and Second Observing Runs

The LIGO Scientific Collaboration, the Virgo Collaboration, B. P. Abbott +1183

When formed through dynamical interactions, stellar-mass binary black holes may retain eccentric orbits (e>0.1 at 10 Hz) detectable by ground-based gravitational-wave detectors.…

gr-qc2019★ 98 cited

All-sky search for short gravitational-wave bursts in the second Advanced LIGO and Advanced Virgo run

The LIGO Scientific Collaboration, the Virgo Collaboration, B. P. Abbott +1186

We present the results of a search for short-duration gravitational-wave transients in the data from the second observing run of Advanced LIGO and Advanced Virgo. We search for gra…

astro-ph.HE2019★ 149 cited

All-sky search for continuous gravitational waves from isolated neutron stars using Advanced LIGO O2 data

The LIGO Scientific Collaboration, the Virgo Collaboration, B. P. Abbott +1130

We present results of an all-sky search for continuous gravitational waves (CWs), which can be produced by fast-spinning neutron stars with an asymmetry around their rotation axis,…

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