World's Best Scientists 2026 revealed!

D-Index & Metrics

Physics

D-Index
78
Citations
22911
World Ranking
3165
National Ranking
1506

Ivan Hubeny 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 Ivan Hubeny 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: 365 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.

Ivan Hubeny 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 Ivan Hubeny 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

Ivan Hubeny is affiliated with the University of Arizona in the United States and has an extensive research portfolio primarily focused on physics and astronomy. Their work spans various subfields including astronomy and astrophysics, instrumentation, electrical and electronic engineering, aerospace engineering, and computational mechanics.

Their research topics cover a broad spectrum within stellar, planetary, and galactic studies, as well as astrophysics and star formation studies. Additional key areas include astronomy and astrophysical research, calibration and measurement techniques, astronomical observations and instrumentation, sensor technology and measurement systems, and optical systems and laser technology.

Hubeny has contributed numerous papers to scientific literature. Notable publications include:

  • An improved model for the spectra of discs of nova-like variables, 2021, Monthly Notices of the Royal Astronomical Society
  • The updated BOSZ synthetic stellar spectral library, 2024, Astronomy and Astrophysics
  • WD 1145+017: Alternative models of the atmosphere, dust clouds, and gas rings, 2022, Astronomy and Astrophysics
  • Opacity for realistic 3D MHD simulations of cool stellar atmospheres, 2023, Astronomy and Astrophysics
  • H-He collision-induced satellite in the Lyman α profile of DBA white dwarf stars, 2020, Monthly Notices of the Royal Astronomical Society

Frequent collaboration plays a significant role in their work. Regular co-authors include:

  • R. C. Bohlin (14 joint publications)
  • Susana E. Deustua (12 joint publications)
  • Gautham Narayan (11 joint publications)
  • Abhijit Saha (11 joint publications)
  • A. Calamida (11 joint publications)

Hubeny's research appears prominently in several publication venues with multiple contributions, including:

  • arXiv (Cornell University) - 5 publications
  • Zenodo (CERN European Organization for Nuclear Research) - 4 publications
  • Monthly Notices of the Royal Astronomical Society - 3 publications
  • Astronomy and Astrophysics - 3 publications
  • The Astrophysical Journal - 3 publications

Best Publications

  • Non-LTE line-blanketed model atmospheres of hot stars. 1: Hybrid complete linearization/accelerated lambda iteration method

    I. Hubeny;T. Lanz;T. Lanz

  • A Grid of NLTE Line-Blanketed Model Atmospheres of O-type Stars

    Thierry Lanz;Ivan Hubeny

  • A computer program for calculating non-LTE model stellar atmospheres

    I. Hubeny

  • A Grid of Non-LTE Line-blanketed Model Atmospheres of O-Type Stars

    Thierry Lanz;Thierry Lanz;Ivan Hubeny

  • A Grid of NLTE Line-blanketed Model Atmospheres of Early B-Type Stars

    Thierry Lanz;Ivan Hubeny

  • A Possible Bifurcation in Atmospheres of Strongly Irradiated Stars and Planets

    Ivan Hubeny;Adam Burrows;David Sudarsky

  • Theoretical Spectra and Atmospheres of Extrasolar Giant Planets

    David Sudarsky;Adam Burrows;Ivan Hubeny

  • Possible Solutions to the Radius Anomalies of Transiting Giant Planets

    A. Burrows;I. Hubeny;J. Budaj;W. B. Hubbard

  • L AND T DWARF MODELS AND THE L TO T TRANSITION

    Adam Burrows;David Sudarsky;Ivan Hubeny

  • Vertical structure of accretion disks: A simplified analytical model

    I. Hubeny

  • Stellar Atmospheres: Beyond Classical Models

    L Crivellari;I Hubeny;David G. Hummer

  • Quantitative Spectroscopy of O Stars at Low Metallicity: O Dwarfs in NGC 346*

    J.-C. Bouret;T. Lanz;T. Lanz;D. J. Hillier;S. R. Heap

  • Theoretical Spectra and Light Curves of Close-in Extrasolar Giant Planets and Comparison with Data

    Adam Burrows;J. Budaj;I. Hubeny

  • STIS Coronagraphic Observations of Beta Pictoris

    Sara R. Heap;Don J. Lindler;Thierry M. Lanz;Robert H. Cornett

  • Space Telescope Imaging Spectrograph Coronagraphic Observations of β Pictoris

    Sara R. Heap;Don J. Lindler;Thierry M. Lanz;Thierry M. Lanz;Robert H. Cornett;Robert H. Cornett

  • A Tale of Two Stars: The Extreme O7 Iaf+ Supergiant AV 83 and the OC7.5 III((f)) star AV 69

    D. John Hillier;T. Lanz;T. Lanz;S. R. Heap;I. Hubeny

  • Accelerated complete-linearization method for calculating NLTE model stellar atmospheres

    I. Hubeny;T. Lanz

  • Theoretical Spectral Models of the Planet HD 209458b with a Thermal Inversion and Water Emission Bands

    A. S. Burrows;I. Hubeny;J. Budaj;H. A. Knutson

  • On the Evolutionary Phase and Mass Loss of the Wolf-Rayet-like Stars in R136a*

    Alex de Koter;Sara R. Heap;Ivan Hubeny

  • Non-LTE Models and Theoretical Spectra of Accretion Disks in Active Galactic Nuclei. IV. Effects of Compton Scattering and Metal Opacities

    Ivan Hubeny;Omer Blaes;Julian H. Krolik;Eric Agol;Eric Agol

Frequent Co-Authors

Adam Burrows
Adam Burrows Princeton University
Paula Szkody
Paula Szkody University of Washington
Knox S. Long
Knox S. Long Space Telescope Science Institute
Boris T. Gänsicke
Boris T. Gänsicke University of Warwick
Katia Cunha
Katia Cunha University of Arizona
Keith Horne
Keith Horne University of St Andrews
D. J. Lennon
D. J. Lennon University of La Laguna
Eric Agol
Eric Agol University of Washington
Julian H. Krolik
Julian H. Krolik Johns Hopkins University
Edward W. Olszewski
Edward W. Olszewski University of Arizona

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