S. E. Dwyer

71.5k citations
158 papers · 50.8k · 33 hit papers · h-index 71

Impact in

    • Pulsars and Gravitational Waves Research
    • Gamma-ray bursts and supernovae
    • Cosmology and Gravitation Theories
    • Astrophysical Phenomena and Observations
    • Black Holes and Theoretical Physics
    • Astrophysics and Cosmic Phenomena

Papers in

    • Pulsars and Gravitational Waves Research 148
    • Gamma-ray bursts and supernovae 67
    • Astrophysical Phenomena and Observations 39
    • Cosmology and Gravitation Theories 23
    • Geophysics and Gravity Measurements 32

S. E. Dwyer

156 papers receiving 48.9k citations

S. E. Dwyer's Hit Papers

Advanced LIGO detector performance in the fourth observing run 2025 · 51 citations
510+2+5Years since publication4008001.2k

Peers

S. E. Dwyer
Comparison fields: 5 of 150
  • Astronomy and Astrophysics 45.0k
  • Nuclear and High Energy Physics 15.7k
  • Geophysics 5.8k
  • Oceanography 5.0k
  • Atomic and Molecular Physics, and Optics 6.6k
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Chad Hanna United States
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Citations per field
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Citations per year

Countries citing papers authored by S. E. Dwyer

Since Specialization
Citations

This map shows the geographic impact of S. E. Dwyer's research. It shows the number of citations coming from papers published by authors working in each country. You can also color the map by specialization and compare the number of citations received by S. E. Dwyer with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites S. E. Dwyer more than expected).

Fields of papers citing papers by S. E. Dwyer

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

This network shows the impact of papers produced by S. E. Dwyer. Nodes represent research fields, and links connect fields that are likely to share authors. Colored nodes show fields that tend to cite the papers produced by S. E. Dwyer. The network helps show where S. E. Dwyer may publish in the future.

Co-authors

The 25 scholars most cited alongside S. E. Dwyer, linked wherever they have co-authored with each other. Click a name or a connecting line to browse the papers they share.

Border = papers with S. E. Dwyer Line = papers co-authored together S. E. Dwyer links everyone, so they are left out of the graph.

All Works

20 of 20 papers shown

Showing the 20 most-cited of 158 papers — load more, or switch the sort, to bring in the rest.

#Work
1
Observation of Gravitational Waves from a Binary Black Hole Merger
Hit paper breakdown →
20169808
2
GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral
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20176925
3
Advanced LIGO
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20152689
4
GW151226: Observation of Gravitational Waves from a 22-Solar-Mass Binary Black Hole Coalescence
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20162488
5
Gravitational Waves and Gamma-Rays from a Binary Neutron Star Merger: GW170817 and GRB 170817A
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20172443
6
GW170817: Measurements of Neutron Star Radii and Equation of State
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20181847
7
Tests of General Relativity with GW150914
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20161320
8
GW190425: Observation of a Compact Binary Coalescence with Total Mass ∼ 3.4 M ⊙
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20201268
9
GW190521: A Binary Black Hole Merger with a Total Mass of 150 M ⊙
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20201022
10
Characterization of the LIGO detectors during their sixth science run
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2015968
11
Exploring the sensitivity of next generation gravitational wave detectors
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2017920
12
GW170608: Observation of a 19 Solar-mass Binary Black Hole Coalescence
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2017881
13
Prospects for observing and localizing gravitational-wave transients with Advanced LIGO, Advanced Virgo and KAGRA
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2018865
14
Enhanced sensitivity of the LIGO gravitational wave detector by using squeezed states of light
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2013843
15
Properties of the Binary Black Hole Merger GW150914
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2016733
16
Population Properties of Compact Objects from the Second LIGO–Virgo Gravitational-Wave Transient Catalog
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2021730
17
Population of Merging Compact Binaries Inferred Using Gravitational Waves through GWTC-3
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2023729
18
A gravitational wave observatory operating beyond the quantum shot-noise limit
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2011658
19
Tests of general relativity with the binary black hole signals from the LIGO-Virgo catalog GWTC-1
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2019637
20
Binary Black Hole Mergers in the first Advanced LIGO Observing Run
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2016629

About S. E. Dwyer

S. E. Dwyer is a scholar working on Astronomy and Astrophysics, Oceanography, Atomic and Molecular Physics, and Optics, Nuclear and High Energy Physics and Ocean Engineering, having authored 158 papers that have together received 50.8k indexed citations. Recurring topics across this work include Pulsars and Gravitational Waves Research (148 papers), Gamma-ray bursts and supernovae (67 papers), Astrophysical Phenomena and Observations (39 papers), Geophysics and Gravity Measurements (32 papers), Geophysics and Sensor Technology (24 papers), Cosmology and Gravitation Theories (23 papers), Advanced Frequency and Time Standards (23 papers) and Astrophysics and Cosmic Phenomena (16 papers). The work is most often cited by research in Astronomy and Astrophysics (45.0k citations), Nuclear and High Energy Physics (15.7k citations), Geophysics (5.8k citations), Oceanography (5.0k citations) and Atomic and Molecular Physics, and Optics (6.6k citations). S. E. Dwyer has collaborated with scholars based in United States, Germany and France. Frequent co-authors include Daniel Sigg, Lisa Barsotti, N. Mavalvala, S. Ballmer, Matthew Evans, Eric Oelker, Georgia L. Mansell, Lee McCuller, D. A. Shaddock and Michael Stefszky. Their work appears in journals such as Physical review. D, Physical Review Letters, The Astrophysical Journal, The Astrophysical Journal Letters and Classical and Quantum Gravity.

Rankless uses publication and citation data sourced from OpenAlex, an open and comprehensive bibliographic database. While OpenAlex provides broad and valuable coverage of the global research landscape, it—like all bibliographic datasets—has inherent limitations. These include incomplete records, variations in author disambiguation, differences in journal indexing, and delays in data updates. As a result, some metrics and network relationships displayed in Rankless may not fully capture the entirety of a scholar's output or impact.

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