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D-Index & Metrics

Discipline name D-Index World Ranking Current World Ranking National Ranking Current National Ranking Publications Citations
Physics 122 755 715 67 62 874 55837

Keith Horne publications per year

The chart shows the history of publications by Keith Horne between 1979 and 2025, highlighting the no. of papers published in each year and offering an overview of the publication velocity of this scholar. Keith Horne published across 47 years, from 1979 to 2025, averaging 21.2 papers a year. Output peaked at 45 publications in 2023. 78 of the 996 publications appeared in the last two years.

No. of publications
10 20 30 40
Bar chart. Horizontal axis: year, 1979 to 2025. Vertical axis: number of publications, 0 to 45. Peak 45 publications in 2023. 1979: 3 publications 1980: 3 publications 1981: 4 publications 1982: 1 publication 1983: 5 publications 1984: 1 publication 1985: 5 publications 1986: 8 publications 1987: 2 publications 1988: 5 publications 1989: 4 publications 1990: 8 publications 1991: 8 publications 1992: 9 publications 1993: 14 publications 1994: 16 publications 1995: 17 publications 1996: 22 publications 1997: 25 publications 1998: 22 publications 1999: 17 publications 2000: 21 publications 2001: 26 publications 2002: 19 publications 2003: 22 publications 2004: 40 publications 2005: 22 publications 2006: 33 publications 2007: 23 publications 2008: 28 publications 2009: 32 publications 2010: 30 publications 2011: 31 publications 2012: 30 publications 2013: 25 publications 2014: 28 publications 2015: 35 publications 2016: 39 publications 2017: 34 publications 2018: 26 publications 2019: 44 publications 2020: 31 publications 2021: 38 publications 2022: 17 publications 2023: 45 publications 2024: 44 publications 2025: 34 publications
1979 2025

996 publications in total across all disciplines

View publications per year as a table
Keith Horne: publications per year, 1979 to 2025
Year Publications
1979 3
1980 3
1981 4
1982 1
1983 5
1984 1
1985 5
1986 8
1987 2
1988 5
1989 4
1990 8
1991 8
1992 9
1993 14
1994 16
1995 17
1996 22
1997 25
1998 22
1999 17
2000 21
2001 26
2002 19
2003 22
2004 40
2005 22
2006 33
2007 23
2008 28
2009 32
2010 30
2011 31
2012 30
2013 25
2014 28
2015 35
2016 39
2017 34
2018 26
2019 44
2020 31
2021 38
2022 17
2023 45
2024 44
2025 34
Total 996
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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.

No. of scientists
50 100 150
Bar chart with 70 bars. Horizontal axis: publications, 103–122 to 1,469+. Vertical axis: number of scientists, 0 to 162. Most scientists, 162, have 323–342 publications. The last bar groups every scientist with 1,469 publications or more. The highlighted bar, 863–882 publications, is where this scientist sits. 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
103–122 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.

View publications distribution as a table
Number of Physics scientists by publication count, Research.com 2026 ranking edition. Based on 3,678 ranked scientists.
Publications Scientists This scientist
103–122 7
123–142 10
143–162 31
163–182 35
183–202 53
203–222 81
223–242 85
243–262 112
263–282 114
283–302 126
303–322 136
323–342 162
343–362 155
363–382 156
383–402 134
403–422 145
423–442 147
443–462 131
463–482 131
483–502 116
503–522 106
523–542 103
543–562 87
563–582 84
583–602 94
603–622 70
623–642 76
643–662 60
663–682 54
683–702 60
703–722 48
723–742 64
743–762 48
763–782 37
783–802 43
803–822 34
823–842 36
843–862 32
863–882 32 874
883–902 31
903–922 25
923–942 15
943–962 24
963–982 13
983–1,002 21
1,003–1,022 21
1,023–1,042 16
1,043–1,062 9
1,063–1,082 19
1,083–1,102 11
1,103–1,122 17
1,123–1,142 11
1,143–1,162 7
1,163–1,182 4
1,183–1,202 10
1,203–1,222 8
1,223–1,242 16
1,243–1,262 4
1,263–1,282 10
1,283–1,302 5
1,303–1,322 7
1,323–1,342 4
1,343–1,362 8
1,363–1,382 6
1,383–1,402 7
1,403–1,422 3
1,423–1,442 4
1,443–1,462 4
1,463–1,468 3
1,469+ 100
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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.

No. of scientists
50 100 150
Bar chart with 59 bars. Horizontal axis: D-Index, 70–71 to 185+. Vertical axis: number of scientists, 0 to 167. Most scientists, 167, have 80–81 D-Index. The last bar groups every scientist with 185 D-Index or more. The highlighted bar, 122–123 D-Index, is where this scientist sits. 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
70–71 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.

View D-Index distribution as a table
Number of Physics scientists by D-index, Research.com 2026 ranking edition. Based on 3,678 ranked scientists.
D-Index Scientists This scientist
70–71 76
72–73 110
74–75 143
76–77 153
78–79 144
80–81 167
82–83 167
84–85 166
86–87 132
88–89 155
90–91 134
92–93 137
94–95 102
96–97 112
98–99 110
100–101 116
102–103 97
104–105 103
106–107 87
108–109 90
110–111 67
112–113 78
114–115 75
116–117 67
118–119 69
120–121 60
122–123 59 122
124–125 53
126–127 42
128–129 41
130–131 33
132–133 32
134–135 45
136–137 19
138–139 24
140–141 28
142–143 31
144–145 22
146–147 20
148–149 12
150–151 16
152–153 24
154–155 23
156–157 15
158–159 15
160–161 11
162–163 17
164–165 12
166–167 11
168–169 9
170–171 9
172–173 11
174–175 4
176–177 8
178–179 5
180–181 3
182–183 4
184 4
185+ 99
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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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