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D-Index & Metrics

Physics

D-Index
71
Citations
28758
World Ranking
3613
National Ranking
1690

E. Ochsner publication distribution in Physics in 2026

The chart shows the distribution of publications by all Research.com ranked scientists in the field of Physics in 2026. The highlighted bar marks where E. Ochsner sits on this spectrum.

103–122 publications: 7 scientists 123–142 publications: 10 scientists 143–162 publications: 31 scientists 163–182 publications: 35 scientists 183–202 publications: 53 scientists 203–222 publications: 81 scientists 223–242 publications: 85 scientists 243–262 publications: 112 scientists 263–282 publications: 114 scientists 283–302 publications: 126 scientists 303–322 publications: 136 scientists 323–342 publications: 162 scientists 343–362 publications: 155 scientists 363–382 publications: 156 scientists 383–402 publications: 134 scientists 403–422 publications: 145 scientists 423–442 publications: 147 scientists 443–462 publications: 131 scientists 463–482 publications: 131 scientists 483–502 publications: 116 scientists 503–522 publications: 106 scientists 523–542 publications: 103 scientists 543–562 publications: 87 scientists 563–582 publications: 84 scientists 583–602 publications: 94 scientists 603–622 publications: 70 scientists 623–642 publications: 76 scientists 643–662 publications: 60 scientists 663–682 publications: 54 scientists 683–702 publications: 60 scientists 703–722 publications: 48 scientists 723–742 publications: 64 scientists 743–762 publications: 48 scientists 763–782 publications: 37 scientists 783–802 publications: 43 scientists 803–822 publications: 34 scientists 823–842 publications: 36 scientists 843–862 publications: 32 scientists 863–882 publications: 32 scientists 883–902 publications: 31 scientists 903–922 publications: 25 scientists 923–942 publications: 15 scientists 943–962 publications: 24 scientists 963–982 publications: 13 scientists 983–1,002 publications: 21 scientists 1,003–1,022 publications: 21 scientists 1,023–1,042 publications: 16 scientists 1,043–1,062 publications: 9 scientists 1,063–1,082 publications: 19 scientists 1,083–1,102 publications: 11 scientists 1,103–1,122 publications: 17 scientists 1,123–1,142 publications: 11 scientists 1,143–1,162 publications: 7 scientists 1,163–1,182 publications: 4 scientists 1,183–1,202 publications: 10 scientists 1,203–1,222 publications: 8 scientists 1,223–1,242 publications: 16 scientists 1,243–1,262 publications: 4 scientists 1,263–1,282 publications: 10 scientists 1,283–1,302 publications: 5 scientists 1,303–1,322 publications: 7 scientists 1,323–1,342 publications: 4 scientists 1,343–1,362 publications: 8 scientists 1,363–1,382 publications: 6 scientists 1,383–1,402 publications: 7 scientists 1,403–1,422 publications: 3 scientists 1,423–1,442 publications: 4 scientists 1,443–1,462 publications: 4 scientists 1,463–1,468 publications: 3 scientists 1,469+ publications: 100 scientists
103 publications 1,469+

This scientist: 104 publications — 1st percentile

1% of scientists in this discipline score the same or lower.

The last bar groups every scientist with 1,469 publications or more.

E. Ochsner D-index placement in Physics in 2026

The chart shows the D-index (discipline H-index) distribution of Physics scientists ranked by Research.com in 2026. The highlighted bar marks where E. Ochsner sits on this spectrum.

70–71 D-Index: 76 scientists 72–73 D-Index: 110 scientists 74–75 D-Index: 143 scientists 76–77 D-Index: 153 scientists 78–79 D-Index: 144 scientists 80–81 D-Index: 167 scientists 82–83 D-Index: 167 scientists 84–85 D-Index: 166 scientists 86–87 D-Index: 132 scientists 88–89 D-Index: 155 scientists 90–91 D-Index: 134 scientists 92–93 D-Index: 137 scientists 94–95 D-Index: 102 scientists 96–97 D-Index: 112 scientists 98–99 D-Index: 110 scientists 100–101 D-Index: 116 scientists 102–103 D-Index: 97 scientists 104–105 D-Index: 103 scientists 106–107 D-Index: 87 scientists 108–109 D-Index: 90 scientists 110–111 D-Index: 67 scientists 112–113 D-Index: 78 scientists 114–115 D-Index: 75 scientists 116–117 D-Index: 67 scientists 118–119 D-Index: 69 scientists 120–121 D-Index: 60 scientists 122–123 D-Index: 59 scientists 124–125 D-Index: 53 scientists 126–127 D-Index: 42 scientists 128–129 D-Index: 41 scientists 130–131 D-Index: 33 scientists 132–133 D-Index: 32 scientists 134–135 D-Index: 45 scientists 136–137 D-Index: 19 scientists 138–139 D-Index: 24 scientists 140–141 D-Index: 28 scientists 142–143 D-Index: 31 scientists 144–145 D-Index: 22 scientists 146–147 D-Index: 20 scientists 148–149 D-Index: 12 scientists 150–151 D-Index: 16 scientists 152–153 D-Index: 24 scientists 154–155 D-Index: 23 scientists 156–157 D-Index: 15 scientists 158–159 D-Index: 15 scientists 160–161 D-Index: 11 scientists 162–163 D-Index: 17 scientists 164–165 D-Index: 12 scientists 166–167 D-Index: 11 scientists 168–169 D-Index: 9 scientists 170–171 D-Index: 9 scientists 172–173 D-Index: 11 scientists 174–175 D-Index: 4 scientists 176–177 D-Index: 8 scientists 178–179 D-Index: 5 scientists 180–181 D-Index: 3 scientists 182–183 D-Index: 4 scientists 184 D-Index: 4 scientists 185+ D-Index: 99 scientists
70 D-Index 185+

This scientist: 71 D-Index — 2nd percentile

2% of scientists in this discipline score the same or lower.

The last bar groups every scientist with 185 D-Index or more.

Overview

E. Ochsner is affiliated with Amazon Web Services in the United States. Their professional focus involves work related to cloud computing technologies and associated infrastructure, as indicated by the primary affiliation with a leading cloud service provider.

No published papers, co-authors, or specific publication venues have been listed, which suggests that the individual's contributions might be more oriented toward industry practice or internal projects rather than extensive academic publishing.

There is no available data on fields of study, subfields, or main research topics. This absence indicates that their scientific output or publicly documented research scope may currently be limited or non-disclosed.

Similarly, there are no recorded awards or recognized distinctions attributed to E. Ochsner at this time.

This profile reflects the current public record based on available data, focusing on their professional role and presence within the technology sector at Amazon Web Services.

Best Publications

  • GW170104: Observation of a 50-Solar-Mass Binary Black Hole Coalescence at Redshift 0.2

    B. P. Abbott;R. Abbott;T. D. Abbott;F. Acernese

  • Prospects for Observing and Localizing Gravitational-Wave Transients with Advanced LIGO, Advanced Virgo and KAGRA

    B. P. Abbott;R. Abbott;T. D. Abbott;M. R. Abernathy

  • Binary Black Hole Mergers in the First Advanced LIGO Observing Run

    B. P. Abbott;R. Abbott

  • Predictions for the Rates of Compact Binary Coalescences Observable by Ground-based Gravitational-wave Detectors

    J. Abadie;B. P. Abbott

  • Characterization of the LIGO detectors during their sixth science run

    J. Aasi;J. Abadie;B. P. Abbott;R. Abbott

  • A gravitational wave observatory operating beyond the quantum shot-noise limit

    J. Abadie;B. P. Abbott;R. Abbott;T. D. Abbott

  • Prospects for Observing and Localizing Gravitational-Wave Transients with Advanced LIGO, Advanced Virgo and KAGRA

    B. P. Abbott

  • ASTROPHYSICAL IMPLICATIONS OF THE BINARY BLACK HOLE MERGER GW150914

    B. P. Abbott;R. Abbott;T. D. Abbott;M. R. Abernathy

  • Directional Limits on Persistent Gravitational Waves from Advanced LIGO’s First Observing Run

    B. P. Abbott;R. Abbott;T. D. Abbott;M. R. Abernathy

  • Exploring the Sensitivity of Next Generation Gravitational Wave Detectors

    B. P. Abbott;R. Abbott;T. D. Abbott;M. R. Abernathy

  • Comparison of post-Newtonian templates for compact binary inspiral signals in gravitational-wave detectors

    Alessandra Buonanno;Alessandra Buonanno;Bala Iyer;Bala Iyer;Evan Ochsner;Yi Pan

  • GW150914: First results from the search for binary black hole coalescence with Advanced LIGO

    B. P. Abbott;R. Abbott;T. D. Abbott;M. R. Abernathy

  • An upper limit on the stochastic gravitational-wave background of cosmological origin

    B. P. Abbott;R. Abbott;F. Acernese;R. Adhikari

  • GW150914: implications for the stochastic gravitational wave background from binary black holes

    B. P. Abbott;R. Abbott;T. D. Abbott;M. R. Abernathy

  • Characterization of transient noise in Advanced LIGO relevant to gravitational wave signal GW150914

    B. P. Abbott;R. Abbott;T. D. Abbott;M. R. Abernathy

  • Higher-order spin effects in the amplitude and phase of gravitational waveforms emitted by inspiraling compact binaries: Ready-to-use gravitational waveforms

    K. G. Arun;K. G. Arun;Alessandra Buonanno;Alessandra Buonanno;Guillaume Faye;Evan Ochsner

  • Localization and broadband follow-up of the gravitational-wave transient GW150914

    B. P. Abbott;R. Abbott;T. D. Abbott;M. R. Abernathy

  • Search for gravitational waves from low mass compact binary coalescence in LIGO's sixth science run and Virgo's science runs 2 and 3

    J. Abadie;B.P. Abbott;R. Abbott;T.D. Abbott

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

    B. P. Abbott;R. Abbott;R. Abbott;T. D. Abbott;M. R. Abernathy

  • Supplement: The Rate of Binary Black Hole Mergers Inferred from Advanced LIGO Observations Surrounding GW150914

    B. P. Abbott;R. Abbott;T. D. Abbott;M. R. Abernathy

Frequent Co-Authors

Bruce Allen
Bruce Allen Max Planck Society
N. A. Robertson
N. A. Robertson California Institute of Technology
Alessandra Buonanno
Alessandra Buonanno Max Planck Institute for Gravitational Physics
Karsten Danzmann
Karsten Danzmann Max Planck Institute for Gravitational Physics
James Whelan
James Whelan La Trobe University
Evan Goetz
Evan Goetz University of British Columbia
Laura Cadonati
Laura Cadonati Georgia Institute of Technology

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