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Dovi Poznanski

Dovi Poznanski

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Physics
Israel
2023

D-Index & Metrics

Discipline name D-Index World Ranking Current World Ranking National Ranking Current National Ranking Publications Citations
Physics 82 2846 2703 25 24 161 25637

Dovi Poznanski publications per year

The chart shows the history of publications by Dovi Poznanski between 2002 and 2025, highlighting the no. of papers published in each year and offering an overview of the publication velocity of this scholar. Dovi Poznanski published across 24 years, from 2002 to 2025, averaging 7.2 papers a year. Output peaked at 29 publications in 2011. 8 of the 173 publications appeared in the last two years.

No. of publications
5 10 15 20 25
Bar chart. Horizontal axis: year, 2002 to 2025. Vertical axis: number of publications, 0 to 29. Peak 29 publications in 2011. 2002: 1 publication 2003: 1 publication 2004: 3 publications 2005: 5 publications 2006: 1 publication 2007: 5 publications 2008: 6 publications 2009: 18 publications 2010: 13 publications 2011: 29 publications 2012: 22 publications 2013: 8 publications 2014: 7 publications 2015: 7 publications 2016: 5 publications 2017: 10 publications 2018: 6 publications 2019: 8 publications 2020: 2 publications 2021: 2 publications 2022: 1 publication 2023: 5 publications 2024: 2 publications 2025: 6 publications
2002 2025

173 publications in total across all disciplines

View publications per year as a table
Dovi Poznanski: publications per year, 2002 to 2025
Year Publications
2002 1
2003 1
2004 3
2005 5
2006 1
2007 5
2008 6
2009 18
2010 13
2011 29
2012 22
2013 8
2014 7
2015 7
2016 5
2017 10
2018 6
2019 8
2020 2
2021 2
2022 1
2023 5
2024 2
2025 6
Total 173
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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.

No. of scientists
50 100 150
Bar chart with 70 bars. Horizontal axis: publications, 103–122 to 1,469+. Vertical axis: number of scientists, 0 to 162. Most scientists, 162, have 323–342 publications. The last bar groups every scientist with 1,469 publications or more. The highlighted bar, 143–162 publications, is where this scientist sits. 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
103–122 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.

View publications distribution as a table
Number of Physics scientists by publication count, Research.com 2026 ranking edition. Based on 3,678 ranked scientists.
Publications Scientists This scientist
103–122 7
123–142 10
143–162 31 161
163–182 35
183–202 53
203–222 81
223–242 85
243–262 112
263–282 114
283–302 126
303–322 136
323–342 162
343–362 155
363–382 156
383–402 134
403–422 145
423–442 147
443–462 131
463–482 131
483–502 116
503–522 106
523–542 103
543–562 87
563–582 84
583–602 94
603–622 70
623–642 76
643–662 60
663–682 54
683–702 60
703–722 48
723–742 64
743–762 48
763–782 37
783–802 43
803–822 34
823–842 36
843–862 32
863–882 32
883–902 31
903–922 25
923–942 15
943–962 24
963–982 13
983–1,002 21
1,003–1,022 21
1,023–1,042 16
1,043–1,062 9
1,063–1,082 19
1,083–1,102 11
1,103–1,122 17
1,123–1,142 11
1,143–1,162 7
1,163–1,182 4
1,183–1,202 10
1,203–1,222 8
1,223–1,242 16
1,243–1,262 4
1,263–1,282 10
1,283–1,302 5
1,303–1,322 7
1,323–1,342 4
1,343–1,362 8
1,363–1,382 6
1,383–1,402 7
1,403–1,422 3
1,423–1,442 4
1,443–1,462 4
1,463–1,468 3
1,469+ 100
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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.

No. of scientists
50 100 150
Bar chart with 59 bars. Horizontal axis: D-Index, 70–71 to 185+. Vertical axis: number of scientists, 0 to 167. Most scientists, 167, have 80–81 D-Index. The last bar groups every scientist with 185 D-Index or more. The highlighted bar, 82–83 D-Index, is where this scientist sits. 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
70–71 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.

View D-Index distribution as a table
Number of Physics scientists by D-index, Research.com 2026 ranking edition. Based on 3,678 ranked scientists.
D-Index Scientists This scientist
70–71 76
72–73 110
74–75 143
76–77 153
78–79 144
80–81 167
82–83 167 82
84–85 166
86–87 132
88–89 155
90–91 134
92–93 137
94–95 102
96–97 112
98–99 110
100–101 116
102–103 97
104–105 103
106–107 87
108–109 90
110–111 67
112–113 78
114–115 75
116–117 67
118–119 69
120–121 60
122–123 59
124–125 53
126–127 42
128–129 41
130–131 33
132–133 32
134–135 45
136–137 19
138–139 24
140–141 28
142–143 31
144–145 22
146–147 20
148–149 12
150–151 16
152–153 24
154–155 23
156–157 15
158–159 15
160–161 11
162–163 17
164–165 12
166–167 11
168–169 9
170–171 9
172–173 11
174–175 4
176–177 8
178–179 5
180–181 3
182–183 4
184 4
185+ 99
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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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