World's Best Scientists 2026 revealed!

D-Index & Metrics

Physics

D-Index
105
Citations
50086
World Ranking
1363
National Ranking
711

Laura Ferrarese 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 Laura Ferrarese 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: 471 publications — 51st percentile

51% of scientists in this discipline score the same or lower.

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

Laura Ferrarese 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 Laura Ferrarese 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: 105 D-Index — 63rd percentile

63% 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

  • 2020 - Fellow of the Royal Society of Canada Academy of Science

Overview

Laura Ferrarese is affiliated with the National Academies of Sciences, Engineering, and Medicine in the United States. Their research primarily focuses on Physics and Astronomy, with significant contributions across related subfields such as Astronomy and Astrophysics, Instrumentation, Atomic and Molecular Physics, and Nuclear and High Energy Physics.

The scientist's work extensively covers the areas of galaxies formation, evolution, and phenomena, as well as broader topics in astronomy and astrophysical research. Their research topics include stellar, planetary, and galactic studies, astrophysics and star formation studies, astrophysical phenomena and observations, gamma-ray bursts and supernovae, and adaptive optics with wavefront sensing.

Frequent co-authors collaborating with Laura Ferrarese include:

  • Patrick Côté
  • Eric W. Peng
  • Jean-Charles Cuillandre
  • Joel Roediger
  • Stephen Gwyn

They have published numerous papers in a variety of scientific journals and venues. Among the prominent publication venues, the most frequent are:

  • arXiv (Cornell University)
  • The Astrophysical Journal
  • Astronomy and Astrophysics
  • Monthly Notices of the Royal Astronomical Society
  • Publications of the Astronomical Society of the Pacific

Recent significant papers include:

  • "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
  • "Performance of NIRCam on JWST in Flight", 2023, Publications of the Astronomical Society of the Pacific
  • "The Near Infrared Imager and Slitless Spectrograph for the James Webb Space Telescope. I. Instrument Overview and In-flight Performance", 2023, Publications of the Astronomical Society of the Pacific
  • "A Virgo Environmental Survey Tracing Ionised Gas Emission (VESTIGE)", 2020, Astronomy and Astrophysics
  • "The Next Generation Virgo Cluster Survey. XXXIV. Ultracompact Dwarf Galaxies in the Virgo Cluster", 2020, The Astrophysical Journal Supplement Series

Laura Ferrarese's research involves considerable collaboration with other scientists, including Patrick Côté, Eric W. Peng, Jean-Charles Cuillandre, Joel Roediger, and Stephen Gwyn, reflecting a broad network in their field of study.

In recognition of contributions to science, they were awarded the Fellowship of the Royal Society of Canada in 2020 by the Academy of Science.

Best Publications

  • A Fundamental Relation Between Supermassive Black Holes and Their Host Galaxies

    Laura Ferrarese;Laura Ferrarese;David Merritt

  • Final Results from the Hubble Space Telescope Key Project to Measure the Hubble Constant

    Wendy L. Freedman;Barry F. Madore;Barry F. Madore;Brad K. Gibson;Laura Ferrarese

  • CENTRAL MASSES AND BROAD-LINE REGION SIZES OF ACTIVE GALACTIC NUCLEI. II. A HOMOGENEOUS ANALYSIS OF A LARGE REVERBERATION-MAPPING DATABASE

    Bradley M Peterson;Laura Ferrarese;K M Gilbert;K M Gilbert;S Kaspi;S Kaspi

  • Supermassive Black Holes in Galactic Nuclei: Past, Present and Future Research

    Laura Ferrarese;Laura Ferrarese;Holland Ford

  • Supermassive Black Holes in Active Galactic Nuclei. II. Calibration of the M-sigma Relationship for AGNs

    Christopher A. Onken;Laura Ferrarese;David Merritt;Bradley M. Peterson

  • The HST Key Project on the Extragalactic Distance Scale. XXVIII. Combining the Constraints on the Hubble Constant

    Jeremy R Mould;John P Huchra;Wendy L Freedman;Robert C Kennicutt Jr

  • The Hubble Space Telescope Key Project on the Extragalactic Distance Scale. XXVIII. Combining the Constraints on the Hubble Constant

    Jeremy R. Mould;John P. Huchra;Wendy L. Freedman;Robert C. Kennicutt

  • Beyond the bulge: a fundamental relation between supermassive black holes and dark matter halos

    Laura Ferrarese

  • The Hubble Space Telescope Extragalactic Distance Scale Key Project. 1: The discovery of Cepheids and a new distance to M81

    Wendy L. Freedman;Shaun M. Hughes;Barry F. Madore;Jeremy R. Mould

  • 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

  • Distance to the Virgo cluster galaxy M100 from Hubble Space Telescope observations of Cepheids

    Wendy L. Freedman;Barry F. Madore;Jeremy R. Mould;Robert Hill

  • Supermassive black holes in active galactic nuclei. II. Calibration of the black hole mass-velocity dispersion relationship for active galactic nuclei

    Christopher A. Onken;Laura Ferrarese;David Merritt;David Merritt;Bradley M. Peterson

  • The M(BH)-Sigma Relation for Supermassive Black Holes

    David Merritt;Laura Ferrarese

  • 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 M•-σ Relation for Supermassive Black Holes

    David Merritt;Laura Ferrarese

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

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

  • Black Hole Demographics from the M(BH)-sigma Relation

    David Merritt;Laura Ferrarese

  • Black hole demographics from the M● − σ relation

    David Merritt;Laura Ferrarese

  • 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

Frequent Co-Authors

Patrick Côté
Patrick Côté National Research Council Canada
Simona Mei
Simona Mei Université Paris Cité
John P. Blakeslee
John P. Blakeslee National Optical-Infrared Astronomy Research Lab
Andrés Jordán
Andrés Jordán Adolfo Ibáñez University
Eric W. Peng
Eric W. Peng Peking University
Wendy L. Freedman
Wendy L. Freedman University of Chicago
Barry F. Madore
Barry F. Madore Carnegie Institution for Science
Pierre-Alain Duc
Pierre-Alain Duc University of Strasbourg
Alessandro Boselli
Alessandro Boselli Aix-Marseille University
David Merritt
David Merritt Rochester Institute of Technology

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