World's Best Scientists 2026 revealed!

D-Index & Metrics

Physics

D-Index
76
Citations
19549
World Ranking
3334
National Ranking
1576

Robert Antonucci 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 Robert Antonucci 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: 228 publications — 7th percentile

7% of scientists in this discipline score the same or lower.

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

Robert Antonucci 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 Robert Antonucci 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: 76 D-Index — 11th percentile

11% of scientists in this discipline score the same or lower.

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

Overview

Robert Antonucci is affiliated with the University of California, Santa Barbara in the United States. Their research activity is centered primarily in the field of Physics and Astronomy, with a focus on Astronomy and Astrophysics, Nuclear and High Energy Physics, Instrumentation, Global and Planetary Change, and Statistical and Nonlinear Physics.

The scientist's work covers a range of topics including:

  • Galaxies: Formation, Evolution, Phenomena
  • Astrophysical Phenomena and Observations
  • Astrophysics and Star Formation Studies
  • Astrophysics and Cosmic Phenomena
  • Gamma-ray bursts and supernovae
  • Stellar, planetary, and galactic studies
  • Solar and Space Plasma Dynamics

The recent papers authored or co-authored by Robert Antonucci include the following:

  • "Unravelling the origin of extended radio emission in narrow-line Seyfert 1 galaxies with the JVLA" (2022) published in arXiv (Cornell University)
  • "Beyond Simple AGN Unification with Chandra-observed 3CRR Sources at 0.5 < z < 1" (2021) published in The Astrophysical Journal
  • "The Dust Sublimation Region of the Type 1 AGN NGC 4151 at a Hundred Microarcsecond Scale as Resolved by the CHARA Array Interferometer" (2022) published in The Astrophysical Journal
  • "A Walk through AGN Country-For the Somewhat Initiated!" (2023) published in Galaxies
  • "On the Origin of Radio-loudness in Active Galactic Nuclei Using Far-infrared Polarimetric Observations" (2023) published in The Astrophysical Journal

Publication venues frequently featuring Robert Antonucci's research include:

  • arXiv (Cornell University)
  • The Astrophysical Journal
  • Monthly Notices of the Royal Astronomical Society
  • Galaxies
  • Preprints.org

Frequent collaborators in Robert Antonucci's research endeavors are:

  • Enrique López-Rodríguez
  • P. Ogle
  • Makoto Kishimoto
  • Joanna Kuraszkiewicz
  • B. J. Wilkes

Best Publications

  • Vlbi imaging of water maser emission from the nuclear torus of ngc 1068

    L. J. Greenhill;C. R. Gwinn;R. Antonucci;R. Barvainis

  • Multiwavelength tests of the dusty torus model for Seyfert galaxies

    John S. Mulchaey;Anuradha Koratkar;Martin J. Ward;Andrew S. Wilson

  • A Hubble Space Telescope Survey of Extended [OIII]5007A Emission in a Far-Infrared Selected Sample of Seyfert Galaxies: Observations

    H.R. Schmitt;J.L. Donley;R.R.J. Antonucci;J.B. Hutchings

  • Triggered Star Formation in a Massive Galaxy at z = 3.8: 4C 41.17

    Arjun Dey;Wil van Breugel;William D. Vacca;Robert Antonucci

  • Triggered Star Formation in a Massive Galaxy at z=3.8: 4C41.17

    Arjun Dey;Wil van Breugel;William Vacca;Robert Antonucci

  • Dust in the polar region as a major contributor to the IR emission of AGN

    Sebastian F. Hoenig;Makoto Kishimoto;Konrad R. W. Tristram;M. Almudena Prieto

  • Jet Directions in Seyfert Galaxies

    A. L. Kinney;A. L. Kinney;H. R. Schmitt;C. J. Clarke;J. E. Pringle

  • The innermost dusty structure in active galactic nuclei as probed by the Keck interferometer

    M. Kishimoto;S. F. Hönig;R. Antonucci;R. Barvainis

  • A survey for high optical polarization in quasars with core-dominant radio structure : is there a beamed optical continuum ?

    Beverley J. Wills;Derek Wills;Michel Breger;Michel Breger;R. R.J. Antonucci;R. R.J. Antonucci

  • VLA Observations of NGC 253: Supernova Remnants and H II Regions at 1 Parsec Resolution

    James S. Ulvestad;James S. Ulvestad;Robert R. J. Antonucci

  • DUST IN THE POLAR REGION AS A MAJOR CONTRIBUTOR TO THE INFRARED EMISSION OF ACTIVE GALACTIC NUCLEI

    S. F. Hönig;M. Kishimoto;K. R. W. Tristram;M. A. Prieto

  • The innermost dusty structure in active galactic nuclei as probed by the Keck interferometer

    Makoto Kishimoto;Sebastian F. Hoenig;Robert Antonucci;Richard Barvainis

  • A Hubble Space Telescope Survey of Extended [O III] λ5007 Emission in a Far-Infrared Selected Sample of Seyfert Galaxies: Observations*

    H. R. Schmitt;J. L. Donley;J. L. Donley;R. R. J. Antonucci;J. B. Hutchings

  • PARSEC-SCALE DUST EMISSION FROM THE POLAR REGION IN THE TYPE 2 NUCLEUS OF NGC 424

    S. F. Hönig;M. Kishimoto;R. Antonucci;A. Marconi

  • The characteristic blue spectra of accretion disks in quasars as uncovered in the infrared

    Makoto Kishimoto;Makoto Kishimoto;Robert Antonucci;Omer Blaes;Andy Lawrence

  • A Hubble Space Telescope Survey of Extended [O III] λ5007 Å Emission in a Far-Infrared-Selected Sample of Seyfert Galaxies: Results*

    H. R. Schmitt;J. L. Donley;J. L. Donley;R. R. J. Antonucci;J. B. Hutchings

  • HST imaging of the inner 3 arcseconds of NGC 1068 in the light of forbidden O III 5007 A

    I.N. Evans;A.L. Kinney;H.C. Ford;R.R.J. Antonucci

  • Mapping the radial structure of AGN tori

    Makoto Kishimoto;Sebastian F. Hoenig;Robert Antonucci;Florentin Millour

  • The Nuclear Reddening Curve for Active Galactic Nuclei and the Shape of the Infra-Red to X-Ray Spectral Energy Distribution

    C. Martin Gaskell;Rene W. Goosmann;Robert R. J. Antonucci;David H. Whysong

  • The nuclear reddening curve for active galactic nuclei and the shape of the infrared to X-ray spectral energy distribution

    C. Martin Gaskell;René W. Goosmann;René W. Goosmann;Robert R. J. Antonucci;David H. Whysong

Frequent Co-Authors

Arjun Dey
Arjun Dey Harvard University
Charles R. Lawrence
Charles R. Lawrence Jet Propulsion Lab
Belinda Jane Wilkes
Belinda Jane Wilkes Harvard University
Tommaso Treu
Tommaso Treu University of California, Los Angeles
Andrea Cimatti
Andrea Cimatti University of Bologna
Holland C. Ford
Holland C. Ford Johns Hopkins University
Giovanni G. Fazio
Giovanni G. Fazio Harvard University
Julian H. Krolik
Julian H. Krolik Johns Hopkins University
Mark Birkinshaw
Mark Birkinshaw University of Bristol
Vassilis Charmandaris
Vassilis Charmandaris University of Crete

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