World's Best Scientists 2026 revealed!

D-Index & Metrics

Physics

D-Index
122
Citations
55837
World Ranking
755
National Ranking
67

Keith Horne 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 Keith Horne 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: 874 publications — 88th percentile

88% of scientists in this discipline score the same or lower.

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

Keith Horne 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 Keith Horne 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: 122 D-Index — 80th percentile

80% of scientists in this discipline score the same or lower.

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

Research.com Recognitions

  • 1998 - Fellow of the Royal Society of Edinburgh

Overview

Keith Horne is affiliated with the University of St Andrews in the United Kingdom and specializes in the field of Physics and Astronomy. Their research spans various subfields, primarily focusing on Astronomy and Astrophysics, with additional work in Instrumentation, Nuclear and High Energy Physics, Atomic and Molecular Physics, and Optics, as well as Computational Mechanics.

Their work covers a broad range of main topics including Astrophysical Phenomena and Observations, Stellar, Planetary, and Galactic Studies, Astronomy and Astrophysical Research, Galaxies: Formation, Evolution, and Phenomena, Astro and Planetary Science, Gamma-ray Bursts and Supernovae, and Astrophysics and Star Formation Studies.

Keith Horne has collaborated frequently with several researchers, highlighting an extensive network of coauthors. Among these frequent collaborators are Karen A. Collins, Jon M. Jenkins, Edward M. Cackett, Richard P. Schwarz, and M. R. Goad, each contributing to multiple joint publications.

The scientist's work has appeared across a variety of publication venues. The most common outlets include arXiv (Cornell University), The Astrophysical Journal, The Astronomical Journal, Monthly Notices of the Royal Astronomical Society, and Astronomy and Astrophysics.

Recent notable publications include:

  • Intensive disc-reverberation mapping of Fairall 9: first year of Swift and LCO monitoring, 2020, Monthly Notices of the Royal Astronomical Society
  • The tidal disruption event AT 2018hyz - I. Double-peaked emission lines and a flat Balmer decrement, 2020, Monthly Notices of the Royal Astronomical Society
  • The Sloan Digital Sky Survey Reverberation Mapping Project: The Hβ Radius-Luminosity Relation, 2020, The Astrophysical Journal
  • The Sloan Digital Sky Survey Reverberation Mapping Project: Key Results, 2024, The Astrophysical Journal Supplement Series
  • Paper by K. C. Sahu, 2022, Warwick Research Archive Portal (University of Warwick)

Keith Horne was awarded the title of Fellow of the Royal Society of Edinburgh in 1998, recognizing their contributions to their field.

Best Publications

  • AN OPTIMAL EXTRACTION ALGORITHM FOR CCD SPECTROSCOPY.

    K. Horne

  • The WASP project and the superWASP cameras

    Don Pollacco;I. Skillen;A. Collier Cameron;D. J. Christian

  • Echoes in X‐ray binaries

    K. O'Brien;K. O'Brien;Keith Horne;R. I. Hynes;R. I. Hynes;W. Chen

  • Discovery of a cool planet of 5.5 Earth masses through gravitational microlensing

    J.-P. Beaulieu;D. P. Bennett;P. Fouqué;A. Williams

  • One or more bound planets per Milky Way star from microlensing observations

    A. Cassan;A. Cassan;D. Kubas;D. Kubas;J.-P. Beaulieu;J.-P. Beaulieu;M. Dominik;M. Dominik

  • Images of accretion discs – II. Doppler tomography

    T. R. Marsh;Keith Horne

  • No supernovae associated with two long-duration gamma ray bursts

    Johan P. U. Fynbo;Darach Watson;Christina C. Thöne;Jesper Sollerman

  • No supernovae from two nearby long gamma ray bursts

    Johan P. U. Fynbo;Darach Watson;Christina C. Thoene;Jesper Sollerman

  • Harps-N: the new planet hunter at TNG

    Rosario Cosentino;Christophe Lovis;Francesco Pepe;Andrew Collier Cameron

  • On Uncertainties in Cross‐Correlation Lags and the Reality of Wavelength‐dependent Continuum Lags in Active Galactic Nuclei

    Bradley M. Peterson;Ignaz Wanders;Keith Horne;Stefan Collier

  • Discovery of a Jupiter/Saturn Analog with Gravitational Microlensing

    B. S. Gaudi;D. P. Bennett;A. Udalski;A. Gould

  • Ultraviolet variability of NGC 5548 : dynamics of the continuum production region and geometry of the broad-line region

    J. H. Krolik;Keith Horne;T. R. Kallman;M. A. Malkan

  • WASP-12b: The hottest transiting planet yet discovered

    L. Hebb;A. Collier-Cameron;B. Loeillet;D. Pollacco

  • The Radial Velocity Curve and Peculiar TiO Distribution of the Red Secondary Star in Z Chamaeleontis

    Richard A. Wade;Keith Horne

  • Images of accretion discs – I. The eclipse mapping method

    Keith Horne

  • WASP-12b: the hottest transiting extrasolar planet yet discovered

    L. Hebb;A. Collier-Cameron;B. Loeillet;Don Pollacco

  • Emission line formation in accretion discs

    Keith Horne;T. R. Marsh

  • Microlens OGLE-2005-BLG-169 Implies Cool Neptune-Like Planets are Common

    A. Gould;A. Udalski;D. An;D. P. Bennett

  • A systematic search for changing-look quasars in SDSS

    Chelsea L. MacLeod;Nicholas P. Ross;Andy Lawrence;Mike Goad

  • Efficient identification of exoplanetary transit candidates from SuperWASP light curves

    A. Collier Cameron;D. M. Wilson;Richard G. West;L. Hebb

Frequent Co-Authors

David P. Bennett
David P. Bennett Goddard Space Flight Center
Iain A. Steele
Iain A. Steele Liverpool John Moores University
Igor Soszyński
Igor Soszyński University of Warsaw
Michał K. Szymański
Michał K. Szymański University of Warsaw
Grzegorz Pietrzyński
Grzegorz Pietrzyński Polish Academy of Sciences
Andrzej Udalski
Andrzej Udalski University of Warsaw
Andrew Gould
Andrew Gould The Ohio State University
Fumio Abe
Fumio Abe Nagoya University
Yoshitaka Itow
Yoshitaka Itow Nagoya University
Richard W. Pogge
Richard W. Pogge The Ohio State University

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