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Simon L. Morris

D-Index & Metrics

Physics

D-Index
78
Citations
22034
World Ranking
3170
National Ranking
280

Simon L. Morris 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 Simon L. Morris 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: 328 publications — 23rd percentile

23% of scientists in this discipline score the same or lower.

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

Simon L. Morris 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 Simon L. Morris 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: 78 D-Index — 15th percentile

15% of scientists in this discipline score the same or lower.

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

Overview

Simon L. Morris is affiliated with Durham University in the United Kingdom and has contributed to research primarily within the fields of Physics and Astronomy. Their research spans subfields including Astronomy and Astrophysics, Atomic and Molecular Physics, and Optics, Nuclear and High Energy Physics, Instrumentation, and Electrical and Electronic Engineering.

The main topics explored in their work cover a variety of areas such as:

  • Galaxies: Formation, Evolution, Phenomena
  • Stellar, planetary, and galactic studies
  • Adaptive optics and wavefront sensing
  • Astronomy and Astrophysical Research
  • Astrophysics and Cosmic Phenomena
  • Astrophysical Phenomena and Observations
  • Gamma-ray bursts and supernovae

Simon L. Morris has appeared as an author on a number of scientific papers published in key venues. Recent publications include:

  • "Into the Ly α jungle: exploring the circumgalactic medium of galaxies at z ∼ 4−5 with MUSE" (2020) in Monthly Notices of the Royal Astronomical Society
  • "The MUSE Ultra Deep Field (MUDF). III. Hubble Space Telescope WFC3 Grism Spectroscopy and Imaging" (2023) in The Astrophysical Journal Supplement Series
  • "Using realistic host galaxy metallicities to improve the GRB X-ray equivalent total hydrogen column density and constrain the intergalactic medium density" (2020) in Monthly Notices of the Royal Astronomical Society
  • "Quasar Sightline and Galaxy Evolution (QSAGE) survey - II. Galaxy overdensities around UV luminous quasars at z = 1-2" (2020) in Monthly Notices of the Royal Astronomical Society
  • "The relationship between gas and galaxies at z < 1 using the Q0107 quasar triplet" (2021) in Monthly Notices of the Royal Astronomical Society

The venues where Simon L. Morris most frequently publishes are:

  • Monthly Notices of the Royal Astronomical Society
  • arXiv (Cornell University)
  • The Astrophysical Journal Supplement Series
  • Ground-based and Airborne Instrumentation for Astronomy IX
  • Experimental Astronomy

Collaborations have included working with co-authors such as:

  • Michele Fumagalli
  • Sebastiano Cantalupo
  • Nicolás Tejos
  • Tony Dalton
  • Alexander Beckett

Best Publications

  • Comparisons of the Emission-Line and Continuum Properties of Broad Absorption Line and Normal Quasi-stellar Objects

    Ray J. Weymann;Simon L. Morris;Craig B. Foltz;Paul C. Hewett

  • The Einstein Observatory Extended Medium-Sensitivity Survey. II - The optical identifications

    John T. Stocke;Simon L. Morris;I. M. Gioia;T. Maccacaro

  • Differential Galaxy Evolution in Cluster and Field Galaxies at z ≈ 0.3

    Michael L. Balogh;Simon L. Morris;Simon L. Morris;H. K. C. Yee;H. K. C. Yee;R. G. Carlberg;R. G. Carlberg

  • The Origin of Star Formation Gradients in Rich Galaxy Clusters

    Michael L. Balogh;Michael L. Balogh;Julio F. Navarro;Julio F. Navarro;Simon L. Morris

  • A High Signal-to-Noise Ratio Composite Quasar Spectrum

    Paul J. Francis;Paul C. Hewett;Craig B. Foltz;Frederic H. Chaffee

  • The Einstein Observatory Extended Medium-Sensitivity Survey. I - X-ray data and analysis

    I. M. Gioia;T. Maccacaro;R. E. Schild;A. Wolter

  • Galaxy cluster virial masses and Omega

    R. G. Carlberg;H. K. C. Yee;E. Ellingson;R. Abraham

  • The Extended Medium Sensitivity Survey Distant Cluster Sample: X-Ray Data and Interpretation of the Luminosity Evolution

    J. P. Henry;I. M. Gioia;T. Maccacaro;S. L. Morris

  • Steps toward determination of the size and structure of the broad-line region in active galactic nuclei. II - An intensive study of NGC 5548 at optical wavelengths

    B. M. Peterson;B. M. Peterson;T. J. Balonek;E. S. Barker;J. Bechtold

  • A Population of Faint Extended Line Emitters and the Host Galaxies of Optically Thick QSO Absorption Systems

    Michael Rauch;Martin Haehnelt;Andrew Bunker;George Becker

  • The average mass profile of galaxy clusters

    R. G. Carlberg;R. G. Carlberg;H. K. C. Yee;H. K. C. Yee;E. Ellingson;E. Ellingson;S. L. Morris;S. L. Morris

  • The Extended Medium Sensitivity Survey distant cluster sample : X-ray cosmological evolution

    I. M. Gioia;J. P. Henry;T. Maccacaro;S. L. Morris

  • The CNOC2 Field Galaxy Luminosity Function. I. A Description of Luminosity Function Evolution

    Huan Lin;H. K. C. Yee;H. K. C. Yee;R. G. Carlberg;R. G. Carlberg;Simon L. Morris;Simon L. Morris

  • The Dependence of Cluster Galaxy Star Formation Rates on the Global Environment

    Mike L. Balogh;David Schade;David Schade;Simon L. Morris;Simon L. Morris;H. K. C. Yee;H. K. C. Yee

  • Star Formation in Cluster Galaxies at 0.2<z<0.55

    Mike L. Balogh;Simon L. Morris;Simon L. Morris;H. K. C. Yee;H. K. C. Yee;R. G. Carlberg;R. G. Carlberg

  • A Population of Faint Extended Line Emitters and the Host Galaxies of Optically Thick QSO Absorption Systems

    Michael Rauch;Martin Haehnelt;Andrew Bunker;George Becker

  • Dynamically close galaxy pairs and merger rate evolution in the cnoc2 redshift survey

    D. R. Patton;C. J. Pritchet;C. J. Pritchet;R. G. Carlberg;R. G. Carlberg;R. O. Marzke;R. O. Marzke

  • Multiwavelength Observations of Short-Timescale Variability in NGC 4151. IV. Analysis of Multiwavelength Continuum Variability

    RA Edelson;T Alexander;DM Crenshaw;S Kaspi

  • Galaxy Evolution in Abell 2390

    R. G. Abraham;R. G. Abraham;Tammy A. Smecker-Hane;Tammy A. Smecker-Hane;Tammy A. Smecker-Hane;J. B. Hutchings;R. G. Carlberg;R. G. Carlberg

  • Steps toward Determination of the Size and Structure of the Broad-Line Region in Active Galactic Nuclei. XI. Intensive Monitoring of the Ultraviolet Spectrum of NGC 7469

    I. Wanders;I. Wanders;B. M. Peterson;D. Alloin;T. R. Ayres

Frequent Co-Authors

Raymond G. Carlberg
Raymond G. Carlberg University of Toronto
Patrick B. Hall
Patrick B. Hall York University
Chris Evans
Chris Evans UK Astronomy Technology Centre
John T. Stocke
John T. Stocke University of Colorado Boulder
J. B. Hutchings
J. B. Hutchings National Research Council Canada
Tom Theuns
Tom Theuns Durham University
Richard G. Bower
Richard G. Bower Durham University
Roberto Abraham
Roberto Abraham University of Toronto
Tim Morris
Tim Morris University of Oxford
Lex Kaper
Lex Kaper University of Amsterdam

External Links

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Publications: 88

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