World's Best Scientists 2026 revealed!

D-Index & Metrics

Physics

D-Index
120
Citations
52687
World Ranking
814
National Ranking
439

John P. Blakeslee 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 John P. Blakeslee 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: 485 publications — 54th percentile

54% of scientists in this discipline score the same or lower.

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

John P. Blakeslee 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 John P. Blakeslee 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: 120 D-Index — 78th percentile

78% of scientists in this discipline score the same or lower.

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

Overview

John P. Blakeslee is affiliated with the National Optical-Infrared Astronomy Research Lab in the United States. Their research primarily spans the broad domain of physics and astronomy, with a focus on astronomy and astrophysics. The subfields they have worked in include astronomy and astrophysics, instrumentation, atomic and molecular physics and optics, computational mechanics, and electrical and electronic engineering.

The scientist's research topics encompass galaxies formation, evolution, and phenomena, stellar, planetary, and galactic studies, astronomy and astrophysical research, gamma-ray bursts and supernovae, adaptive optics and wavefront sensing, astronomical observations and instrumentation, and astrophysics and star formation studies.

Frequent publication venues for their work include arXiv (Cornell University), The Astrophysical Journal, Monthly Notices of the Royal Astronomical Society, The Astrophysical Journal Supplement Series, and Astronomy and Astrophysics. This indicates a consistent contribution to peer-reviewed journals focused on astronomy and astrophysics as well as broader physics subjects.

Among recent published papers authored or co-authored by Blakeslee are:

  • "Cosmology intertwined: A review of the particle physics, astrophysics, and cosmology associated with the cosmological tensions and anomalies," 2022, Archivio istituzionale della ricerca (Alma Mater Studiorum Università di Bologna)
  • "Unveiling the Universe with emerging cosmological probes," 2022, CU Scholar (University of Colorado Boulder)
  • "Cosmicflows-4," 2023, The Astrophysical Journal
  • "The Next Generation Virgo Cluster Survey (NGVS). XIV. The Discovery of Low-mass Galaxies and a New Galaxy Catalog in the Core of the Virgo Cluster*," 2020, The Astrophysical Journal
  • "Infrared Surface Brightness Fluctuation Distances for MASSIVE and Type Ia Supernova Host Galaxies*," 2021, The Astrophysical Journal Supplement Series

Collaborations have featured several frequent co-authors, including Michele Cantiello, Rubén Sánchez-Janssen, Joseph B. Jensen, Laura Ferrarese, and Patrick Côté. The connection with these co-authors reflects interdisciplinary work across observational astronomy and instrumentation.

Best Publications

  • The Seventh Data Release of the Sloan Digital Sky Survey

    Kevork N. Abazajian;Jennifer K. Adelman-Mccarthy;Marcel A. Agüeros;Sahar S. Allam;Sahar S. Allam

  • The Photometric Performance and Calibration of the HST Advanced Camera For Surveys

    M. Sirianni;M. Sirianni;M. Sirianni;M. J. Jee;N. Benitez;J. P. Blakeslee

  • The SBF Survey of Galaxy Distances. IV. SBF Magnitudes, Colors, and Distances

    John L. Tonry;John L. Tonry;Alan Dressler;John P. Blakeslee;Edward A. Ajhar;Edward A. Ajhar

  • The photometric performance and calibration of the Hubble Space Telescope advanced camera for surveys

    M. Sirianni;M. Sirianni;M. Sirianni;M.J. Jee;N. Benítez;N. Benítez;J.P. Blakeslee

  • The ACS Virgo Cluster Survey. XIII. SBF Distance Catalog and the Three-Dimensional Structure of the Virgo Cluster

    Simona Mei;Simona Mei;John P. Blakeslee;Patrick Côté;John L. Tonry

  • The unusual afterglow of the γ-ray burst of 26 March 1998 as evidence for a supernova connection

    J. S. Bloom;S. R. Kulkarni;S. G. Djorgovski;A. C. Eichelberger

  • The ACS Virgo Cluster survey. VI. Isophotal analysis and the structure of early-type galaxies

    Laura Ferrarese;Patrick Côté;Andrés Jordán;Andrés Jordán;Eric W. Peng

  • The unusual afterglow of GRB 980326: evidence for the gamma-ray burst/supernova connection

    J. S. Bloom;S. R. Kulkarni;S. G. Djorgovski;A. C. Eichelberger

  • The ACS Virgo Cluster Survey. VIII. The Nuclei of Early-Type Galaxies*

    Patrick Côté;Slawomir Piatek;Laura Ferrarese;Andrés Jordán;Andrés Jordán

  • The Morphology - Density Relation in z ~ 1 Clusters

    M. Postman;M. Franx;N. Cross;B. Holden

  • Galaxies at z~6: The UV Luminosity Function and Luminosity Density from 506 UDF, UDF-Ps, and GOODS i-dropouts

    R.J. Bouwens;G.D. Illingworth;J.P. Blakeslee;M. Franx

  • Early-Type Galaxies in the Sloan Digital Sky Survey. III. The Fundamental Plane

    Mariangela Bernardi;Mariangela Bernardi;Ravi K. Sheth;Ravi K. Sheth;James Annis;Scott Burles

  • The acs virgo cluster survey. IX. The color distributions of globular cluster systems in early-type galaxies

    Eric W. Peng;Eric W. Peng;Eric W. Peng;Andrés Jordán;Andrés Jordán;Patrick Côté;John P. Blakeslee

  • The ACS Fornax Cluster Survey. V. Measurement and Recalibration of Surface Brightness Fluctuations and a Precise Value of the Fornax-Virgo Relative Distance

    John P. Blakeslee;John P. Blakeslee;Andrés Jordán;Andrés Jordán;Simona Mei;Simona Mei;Patrick Côté

  • Early-type galaxies in the SDSS. III. The Fundamental Plane

    M. Bernardi;R. K. Sheth;J. Annis;S. Burles

  • The Morphology-Density Relation in z ~ 1 Clusters

    M. Postman;M. Franx;N.J.G. Cross;B. Holden

  • THE NEXT GENERATION VIRGO CLUSTER SURVEY (NGVS). I. INTRODUCTION TO THE SURVEY

    Laura Ferrarese;Patrick Côté;Jean-Charles Cuillandre;S. D. J. Gwyn

  • A Fundamental Relation between Compact Stellar Nuclei, Supermassive Black Holes, and Their Host Galaxies

    Laura Ferrarese;Patrick Côté;Elena Dalla Bontà;Elena Dalla Bontà;Eric W. Peng

  • Galaxies at z ~ 6: The UV Luminosity Function and Luminosity Density from 506 HUDF, HUDF Parallel ACS Field, and GOODS i-Dropouts* **

    R. J. Bouwens;G. D. Illingworth;J. P. Blakeslee;M. Franx

  • The ACS Virgo Cluster Survey. VII. Resolving the Connection Between Globular Clusters and Ultra-Compact Dwarf Galaxies

    Monica Hasegan;Andres Jordan;Patrick Cote;S. G. Djorgovski

Frequent Co-Authors

Simona Mei
Simona Mei Université Paris Cité
Patrick Côté
Patrick Côté National Research Council Canada
Laura Ferrarese
Laura Ferrarese National Academies of Sciences, Engineering, and Medicine
Andrés Jordán
Andrés Jordán Adolfo Ibáñez University
Marc Postman
Marc Postman Space Telescope Science Institute
Holland C. Ford
Holland C. Ford Johns Hopkins University
Eric W. Peng
Eric W. Peng Peking University
Garth D. Illingworth
Garth D. Illingworth University of California, Santa Cruz
Gerhardt R. Meurer
Gerhardt R. Meurer University of Western Australia
Felipe Menanteau
Felipe Menanteau University of Illinois at Urbana-Champaign

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