World's Best Scientists 2026 revealed!
Dovi Poznanski

Dovi Poznanski

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Physics
Israel
2023

D-Index & Metrics

Physics

D-Index
82
Citations
25637
World Ranking
2846
National Ranking
25

Dovi Poznanski 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 Dovi Poznanski 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: 161 publications — 1st percentile

1% of scientists in this discipline score the same or lower.

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

Dovi Poznanski 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 Dovi Poznanski 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: 82 D-Index — 24th percentile

24% 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

  • 2023 - Research.com Physics in Israel Leader Award
  • 2022 - Research.com Physics in Israel Leader Award

Overview

Dovi Poznanski is affiliated with Tel Aviv University in Israel and has an extensive research portfolio in the field of Physics and Astronomy. Their work spans various subfields including Astronomy and Astrophysics, Instrumentation, Nuclear and High Energy Physics, Artificial Intelligence, and Atomic and Molecular Physics, and Optics.

The research conducted by Poznanski covers main topics such as:

  • Gamma-ray bursts and supernovae
  • Pulsars and Gravitational Waves Research
  • Astronomy and Astrophysical Research
  • Stellar, planetary, and galactic studies
  • Astrophysical Phenomena and Observations
  • Adaptive optics and wavefront sensing
  • Astrophysics and Cosmic Phenomena

Frequent coauthors in their publications include M. Kowalski, I. Arcavi, Maayane T. Soumagnac, J. S. Bloom, and A. V. Filippenko, each collaborating on multiple papers.

Publication venues commonly featuring Poznanski's work are diverse, with a strong presence in arXiv (Cornell University), where eight papers have appeared, followed by The Astrophysical Journal, Nature, OPAL (Open@LaTrobe) at La Trobe University, and Astronomy and Astrophysics.

Selected recent papers include:

  • "ULTRASAT: A Wide-field Time-domain UV Space Telescope," 2024, The Astrophysical Journal
  • "PTF10iya: a short-lived, luminous flare from the nuclear region of a star-forming galaxy," 2024, OPAL (Open@LaTrobe) (La Trobe University)
  • "Spherical symmetry in the kilonova AT2017gfo/GW170817," 2023, Nature
  • "A semisupervised machine learning search for never-seen gravitational-wave sources," 2020, Monthly Notices of the Royal Astronomical Society
  • "ULTRASAT: A wide-field time-domain UV space telescope," 2023, arXiv (Cornell University)

Best Publications

  • The Palomar Transient Factory: System Overview, Performance and First Results

    N. M. Law;S. R. Kulkarni;R. G. Dekany;E. O. Ofek

  • The Palomar Transient Factory: system overview, performance and first results

    Nicholas M. Law;Shrinivas R. Kulkarni;Richard G. Dekany;Eran O. Ofek

  • A gravitational-wave standard siren measurement of the Hubble constant

    B. P. Abbott;R. Abbott;T. D. Abbott;F. Acernese;F. Acernese

  • Exploring the Optical Transient Sky with the Palomar Transient Factory

    Arne Rau;Shrinivas R. Kulkarni;Nicholas M. Law;Joshua S. Bloom

  • Nearby Supernova Rates from the Lick Observatory Supernova Search. II. The Observed Luminosity Functions and Fractions of Supernovae in a Complete Sample

    Weidong Li;Jesse Leaman;Jesse Leaman;Ryan Chornock;Ryan Chornock;Alexei V. Filippenko

  • Nearby supernova rates from the Lick Observatory Supernova Search – III. The rate–size relation, and the rates as a function of galaxy Hubble type and colour

    Weidong Li;Ryan Chornock;Ryan Chornock;Jesse Leaman;Jesse Leaman;Alexei V. Filippenko

  • Hydrogen-poor superluminous stellar explosions

    R. M. Quimby;S. R. Kulkarni;M. M. Kasliwal;A. Gal-Yam

  • Supernova SN 2011fe from an exploding carbon–oxygen white dwarf star

    Peter E. Nugent;Peter E. Nugent;Mark Sullivan;S. Bradley Cenko;Rollin C. Thomas

  • Optical emission from a kilonova following a gravitational-wave-detected neutron-star merger

    Iair Arcavi;Iair Arcavi;Griffin Hosseinzadeh;Griffin Hosseinzadeh;D. Andrew Howell;D. Andrew Howell;Curtis McCully;Curtis McCully

  • Supernova 2007bi as a pair-instability explosion.

    Avishay Gal-Yam;P. Mazzali;E. O. Ofek;P. E. Nugent

  • From Shock Breakout to Peak and Beyond: Extensive Panchromatic Observations of the Type Ib Supernova 2008D associated with Swift X-ray Transient 080109

    Maryam Modjaz;W. Li;N. Butler;R. Chornock

  • An Extremely Luminous Panchromatic Outburst from the Nucleus of a Distant Galaxy

    A. J. Levan;N. R. Tanvir;S. B. Cenko;D. A. Perley

  • PTF 11kx: a type Ia supernova with a symbiotic nova progenitor

    B. Dilday;B. Dilday;D. A. Howell;D. A. Howell;S. B. Cenko;J. M. Silverman

  • Exclusion of a luminous red giant as a companion star to the progenitor of supernova SN 2011fe

    Weidong Li;Joshua S. Bloom;Philipp Podsiadlowski;Adam A. Miller

  • A faint type of supernova from a white dwarf with a helium-rich companion

    H. B. Perets;H. B. Perets;A. Gal-Yam;P. A. Mazzali;D. Arnett

  • Berkeley Supernova Ia Program – I. Observations, data reduction and spectroscopic sample of 582 low-redshift Type Ia supernovae

    Jeffrey M. Silverman;Ryan J. Foley;Alexei V. Filippenko;Mohan Ganeshalingam

  • The broad‐lined Type Ic supernova 2003jd★

    S. Valenti;S. Benetti;E. Cappellaro;F. Patat

  • An empirical relation between sodium absorption and dust extinction

    Dovi Poznanski;J. Xavier Prochaska;Joshua S. Bloom;Joshua S. Bloom

  • The Broad-lined Type Ic SN 2003jd

    S. Valenti;S. Benetti;E. Cappellaro;F. Patat

  • From shock breakout to peak and beyond: Extensive panchromatic observations of the type Ib supernova 2008D associated with swift x-ray transient 080109

    M. Modjaz;W. Li;N. Butler;R. Chornock

Frequent Co-Authors

Peter Nugent
Peter Nugent Lawrence Berkeley National Laboratory
Avishay Gal-Yam
Avishay Gal-Yam Weizmann Institute of Science
Mansi M. Kasliwal
Mansi M. Kasliwal California Institute of Technology
Eran O. Ofek
Eran O. Ofek Weizmann Institute of Science
Joshua S. Bloom
Joshua S. Bloom University of California, Berkeley
Shrinivas R. Kulkarni
Shrinivas R. Kulkarni California Institute of Technology
Mark Sullivan
Mark Sullivan University of Southampton
Alexei V. Filippenko
Alexei V. Filippenko University of California, Berkeley
Lars Bildsten
Lars Bildsten University of California, Santa Barbara
Dan Maoz
Dan Maoz Tel Aviv University

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