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researcher

D. Davis

109 papers hereh-index 6933.6k citations152 works total

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

author position
  • first author4
  • middle author16
  • last author1

Across the 21 of 109 papers where every author was matched, so the position is known.

fields
  • gr-qc54
  • astro-ph.HE35
  • astro-ph.IM7
  • astro-ph.CO6
  • physics.ins-det5
  • quant-ph2
same name
  • D. Davis — 50 papers, h 18
  • D. Davis — 33 papers, h 28
  • D. Davis — 25 papers, h 13
  • D. Davis — 16 papers, h 11
  • D. Davis — 5 papers
  • D. Davis — 4 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
20132026
most citedGravitational Waves and Gamma-rays from a Binary Neutron Star Merger: GW170817 and GRB 170817A

3.6k citations · 32.9k across the 109 of their papers we have counts for

collaborators
Showing 2016 · gr-qcShow all

3 papers · 2 filters

gr-qc2016★ 312 cited

Upper Limits on the Stochastic Gravitational-Wave Background from Advanced LIGO's First Observing Run

The LIGO Scientific Collaboration, the Virgo Collaboration, B. P. Abbott +992

A wide variety of astrophysical and cosmological sources are expected to contribute to a stochastic gravitational-wave background. Following the observations of GW150914 and GW1512…

gr-qc2016★ 102 cited

All-sky search for short gravitational-wave bursts in the first Advanced LIGO run

The LIGO Scientific Collaboration, the Virgo Collaboration, B. P. Abbott +986

We present the results from an all-sky search for short-duration gravitational waves in the data of the first run of the Advanced LIGO detectors between September 2015 and January…

gr-qc2016★ 138 cited

Effects of waveform model systematics on the interpretation of GW150914

The LIGO Scientific Collaboration, the Virgo Collaboration, B. P. Abbott +999

Parameter estimates of GW150914 were obtained using Bayesian inference, based on three semi-analytic waveform models for binary black hole coalescences. These waveform models diffe…

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