World's Best Scientists 2026 revealed!
Raymond G. Carlberg

Raymond G. Carlberg

D-Index & Metrics

Physics

D-Index
103
Citations
46433
World Ranking
1477
National Ranking
29

Raymond G. Carlberg 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 Raymond G. Carlberg 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: 368 publications — 31st percentile

31% of scientists in this discipline score the same or lower.

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

Raymond G. Carlberg 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 Raymond G. Carlberg 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: 103 D-Index — 60th percentile

60% of scientists in this discipline score the same or lower.

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

Overview

Raymond G. Carlberg is affiliated with the University of Toronto in Canada. Their main field of study is Physics and Astronomy, with a particular focus on subfields including Astronomy and Astrophysics, Instrumentation, and Statistical and Nonlinear Physics.

The scientist's research covers a range of topics primarily centered on stellar, planetary, and galactic studies, as well as broader astronomy and astrophysical research. Other key areas include astrophysics and star formation studies, galaxies' formation, evolution, and phenomena, scientific research and discoveries, radio astronomy observations and technology, and gamma-ray bursts and supernovae.

Frequent publication venues for their work include:

  • Monthly Notices of the Royal Astronomical Society
  • arXiv (Cornell University)
  • Astronomy and Astrophysics

Raymond G. Carlberg has coauthored several papers with researchers such as Anke Arentsen, Else Starkenburg, Nicolas F. Martin, David S. Aguado, and Federico Sestito, each of whom has collaborated with Carlberg on multiple publications.

Notable recent papers by Carlberg include:

  • Euclidpreparation, 2022, Astronomy and Astrophysics
  • The Pristine survey - XVI. The metallicity of 26 stellar streams around the Milky Way detected with the STREAMFINDER in Gaia EDR3, 2022, Monthly Notices of the Royal Astronomical Society
  • The Pristine Inner Galaxy Survey - VIII. Characterizing the orbital properties of the ancient, very metal-poor inner Milky Way, 2024, Monthly Notices of the Royal Astronomical Society
  • The Pristine survey -- XVI. The metallicity of 26 stellar streams around the Milky Way detected with the STREAMFINDER in Gaia EDR3, 2022, arXiv (Cornell University)
  • The Pristine Inner Galaxy Survey (PIGS) VIII: Characterising the orbital properties of the ancient, very metal-poor inner Milky Way, 2023, arXiv (Cornell University)

Best Publications

  • The Supernova Legacy Survey: Measurement of Omega_M, Omega_Lambda,and w from the First Year Data Set

    P. Astier;J. Guy;N. Regnault;R. Pain

  • Improved cosmological constraints from a joint analysis of the SDSS-II and SNLS supernova samples

    M. Betoule;R. Kessler;J. Guy;J. Guy;J. Mosher

  • Overview of the DESI Legacy Imaging Surveys.

    Arjun Dey;David J. Schlegel;Dustin Lang;Robert Blum

  • SUPERNOVA CONSTRAINTS AND SYSTEMATIC UNCERTAINTIES FROM THE FIRST THREE YEARS OF THE SUPERNOVA LEGACY SURVEY

    A. Conley;A. Conley;J. Guy;M. Sullivan;N. Regnault

  • 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

  • SALT2: using distant supernovae to improve the use of type Ia supernovae as distance indicators

    J. Guy;P. Astier;S. Baumont;D. Hardin

  • The Herschel ATLAS

    S. Eales;L. Dunne;D. Clements;A. Cooray

  • The Average Mass and Light Profiles of Galaxy Clusters

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

  • Galaxy cluster virial masses and Omega

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

  • The DESI Experiment Part I: Science,Targeting, and Survey Design

    Amir Aghamousa;Jessica Aguilar;Steve Ahlen

  • The Herschel ATLAS

    Stephen Anthony Eales;L. Dunne;D. Clements;A. Cooray

  • The type Ia supernova SNLS-03D3bb from a super-Chandrasekhar-mass white dwarf star

    D. Andrew Howell;Mark Sullivan;Peter E. Nugent;Richard S. Ellis

  • The Gemini Deep Deep Survey. VII. The Redshift Evolution of the Mass-Metallicity Relation* **

    S. Savaglio;K. Glazebrook;D. Le Borgne;S. Juneau

  • SNLS3: Constraints on Dark Energy Combining the Supernova Legacy Survey Three Year Data with Other Probes

    M. Sullivan;J. Guy;A. Conley;N. Regnault

  • The Supernova Legacy Survey 3-year sample: Type Ia supernovae photometric distances and cosmological constraints ,

    J. Guy;M. Sullivan;A. Conley;A. Conley;N. Regnault

  • SNLS3: Constraints on dark energy combining the supernova legacy survey three-year data with other probes

    M. Sullivan;J. Guy;A. Conley;A. Conley;N. Regnault

  • Rates and Properties of Type Ia Supernovae as a Function of Mass and Star Formation in Their Host Galaxies

    M. Sullivan;D. Le Borgne;C. J. Pritchet;A. Hodsman

  • Spiral instabilities provoked by accretion and star formation

    J. A. Sellwood;R. G. Carlberg

  • The dependence of Type Ia Supernovae luminosities on their host galaxies

    M. Sullivan;A. Conley;D. A. Howell;D. A. Howell;J. D. Neill

  • Overview of the DESI legacy imaging surveys

    Arjun Dey;David J. Schlegel;Dustin Lang;Dustin Lang;Robert Blum

Frequent Co-Authors

Mark Sullivan
Mark Sullivan University of Southampton
Simon L. Morris
Simon L. Morris Durham University
Nicolas Regnault
Nicolas Regnault Princeton University
Roberto Abraham
Roberto Abraham University of Toronto
Patrick B. Hall
Patrick B. Hall York University
Hongzheng Chen
Hongzheng Chen Zhejiang University
Nathalie Palanque-Delabrouille
Nathalie Palanque-Delabrouille University of Paris-Saclay
Sandra Savaglio
Sandra Savaglio University of Calabria
Karl Glazebrook
Karl Glazebrook Swinburne University of Technology
Richard S. Ellis
Richard S. Ellis University College London

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