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researcher

A. L. Miller

59 papers here

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

fields
  • gr-qc28
  • astro-ph.HE24
  • astro-ph.CO4
  • astro-ph.IM3
ORCID 0000-0002-4890-7627
same name
  • A. L. Miller — 5 papers, h 5
  • A. L. Miller — 3 papers, h 4
  • A. L. Miller — 3 papers, h 1
  • A. L. Miller — 2 papers
  • A. L. Miller — 1 paper
  • A. L. Miller — 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
20142025
most citedGW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral

9.8k citations · 29.6k across the 59 of their papers we have counts for

collaborators
Showing 2025Show all

3 papers · 1 filter

gr-qc2025

Search for planetary-mass ultra-compact binaries using data from the first part of the LIGO--Virgo--KAGRA fourth observing run

The LIGO Scientific Collaboration, the Virgo Collaboration, the KAGRA Collaboration +1765

We present a search for gravitational waves from inspiraling, planetary-mass ultra-compact binaries using data from the first part of the fourth observing run of LIGO, Virgo and KA…

gr-qc2025★ 5 cited

GW230814: investigation of a loud gravitational-wave signal observed with a single detector

The LIGO Scientific Collaboration, The Virgo Collaboration, The Kagra Collaboration +1783

GW230814, detected by the LIGO Livingston observatory with a signal-to-noise ratio of 42.4, represents the loudest gravitational-wave signal in the GWTC-4.0 catalog. Its source is…

astro-ph.HE2025★ 17 cited

Search for continuous gravitational waves from known pulsars in the first part of the fourth LIGO-Virgo-KAGRA observing run

The LIGO Scientific Collaboration, the Virgo Collaboration, the KAGRA Collaboration +1816

Continuous gravitational waves (CWs) emission from neutron stars carries information about their internal structure and equation of state, and it can provide tests of General Relat…

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