World's Best Scientists 2026 revealed!
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Ryan Chornock

D-Index & Metrics

Discipline name D-Index World Ranking Current World Ranking National Ranking Current National Ranking Publications Citations
Physics 130 559 538 309 295 596 75822

Ryan Chornock publications per year

The chart shows the history of publications by Ryan Chornock between 2000 and 2026, highlighting the no. of papers published in each year and offering an overview of the publication velocity of this scholar. Ryan Chornock published across 27 years, from 2000 to 2026, averaging 24.7 papers a year. Output peaked at 50 publications in 2013. 33 of the 668 publications appeared in the last two years.

No. of publications
10 20 30 40 50
Bar chart. Horizontal axis: year, 2000 to 2026. Vertical axis: number of publications, 0 to 50. Peak 50 publications in 2013. 2000: 6 publications 2001: 13 publications 2002: 17 publications 2003: 22 publications 2004: 16 publications 2005: 24 publications 2006: 16 publications 2007: 9 publications 2008: 24 publications 2009: 35 publications 2010: 42 publications 2011: 30 publications 2012: 26 publications 2013: 50 publications 2014: 23 publications 2015: 18 publications 2016: 32 publications 2017: 48 publications 2018: 30 publications 2019: 44 publications 2020: 19 publications 2021: 22 publications 2022: 16 publications 2023: 26 publications 2024: 27 publications 2025: 31 publications 2026: 2 publications
2000 2026

668 publications in total across all disciplines

View publications per year as a table
Ryan Chornock: publications per year, 2000 to 2026
Year Publications
2000 6
2001 13
2002 17
2003 22
2004 16
2005 24
2006 16
2007 9
2008 24
2009 35
2010 42
2011 30
2012 26
2013 50
2014 23
2015 18
2016 32
2017 48
2018 30
2019 44
2020 19
2021 22
2022 16
2023 26
2024 27
2025 31
2026 2
Total 668
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Ryan Chornock 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 Ryan Chornock 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, 583–602 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: 596 publications — 68th percentile

68% 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
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 94 596
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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Ryan Chornock 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 Ryan Chornock 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, 130–131 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: 130 D-Index — 85th percentile

85% 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
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 33 130
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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Overview

Ryan Chornock is affiliated with Northwestern University in the United States. Their research primarily focuses on the field of Physics and Astronomy, with a strong emphasis on Astronomy and Astrophysics, Nuclear and High Energy Physics, Instrumentation, Computational Mechanics, and Biomedical Engineering.

Their work covers numerous key research topics, including:

  • Gamma-ray bursts and supernovae
  • Astrophysical Phenomena and Observations
  • Astrophysics and Cosmic Phenomena
  • Pulsars and Gravitational Waves Research
  • Stellar, planetary, and galactic studies
  • Astronomy and Astrophysical Research
  • Astro and Planetary Science

Some of their recent papers include:

  • A kilonova following a long-duration gamma-ray burst at 350 Mpc (2022, Nature)
  • Short GRB Host Galaxies. I. Photometric and Spectroscopic Catalogs, Host Associations, and Galactocentric Offsets (2022, The Astrophysical Journal)
  • SN 2023ixf in Messier 101: Photo-ionization of Dense, Close-in Circumstellar Material in a Nearby Type II Supernova (2023, The Astrophysical Journal Letters)
  • The Radio to GeV Afterglow of GRB 221009A (2023, The Astrophysical Journal Letters)
  • Evidence for X-Ray Emission in Excess to the Jet-afterglow Decay 3.5 yr after the Binary Neutron Star Merger GW 170817: A New Emission Component (2022, The Astrophysical Journal Letters)

Frequent coauthors in their publications include:

  • R. Margutti
  • E. Berger
  • K. D. Alexander
  • T. Laskar
  • D. Milisavljević

Ryan Chornock has contributed extensively to several scientific venues. These include:

  • arXiv (Cornell University)
  • The Astrophysical Journal
  • The Astrophysical Journal Letters
  • Monthly Notices of the Royal Astronomical Society
  • Zenodo (CERN European Organization for Nuclear Research)

Best Publications

  • Type Ia Supernova Discoveries at z>1 From the Hubble Space Telescope: Evidence for Past Deceleration and Constraints on Dark Energy Evolution

    Adam G. Riess;Louis-Gregory Strolger;John Tonry;Stefano Casertano

  • Type Ia supernova discoveries at z > 1 from the Hubble Space Telescope: Evidence for past deceleration and constraints on dark energy evolution

    Adam G. Riess;Louis-Gregory Strolger;John Tonry;Stefano Casertano

  • The Complete Light-curve Sample of Spectroscopically Confirmed SNe Ia from Pan-STARRS1 and Cosmological Constraints from the Combined Pantheon Sample

    D. M. Scolnic;D. O. Jones;A. Rest;A. Rest;Y. C. Pan

  • A 2.4% DETERMINATION OF THE LOCAL VALUE OF THE HUBBLE CONSTANT*

    Adam G. Riess;Adam G. Riess;Lucas M. Macri;Samantha L. Hoffmann;Dan Scolnic;Dan Scolnic

  • A 3% Solution: Determination of the Hubble Constant with the Hubble Space Telescope and Wide Field Camera 3

    Adam G. Riess;Adam G. Riess;Lucas Macri;Stefano Casertano;Hubert Lampeitl

  • The Complete Light-curve Sample of Spectroscopically Confirmed Type Ia Supernovae from Pan-STARRS1 and Cosmological Constraints from The Combined Pantheon Sample

    D. M. Scolnic;D. O. Jones;A. Rest;Y. C. Pan

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

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

  • A REDETERMINATION OF THE HUBBLE CONSTANT WITH THE HUBBLE SPACE TELESCOPE FROM A DIFFERENTIAL DISTANCE LADDER

    Adam G. Riess;Adam G. Riess;Lucas Macri;Stefano Casertano;Megan Sosey

  • The Electromagnetic Counterpart of the Binary Neutron Star Merger LIGO/Virgo GW170817. II. UV, Optical, and Near-infrared Light Curves and Comparison to Kilonova Models

    P. S. Cowperthwaite;E. Berger;V. A. Villar;B. D. Metzger

  • 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

  • The Electromagnetic Counterpart of the Binary Neutron Star Merger LIGO/VIRGO GW170817. II. UV, Optical, and Near-IR Light Curves and Comparison to Kilonova Models

    P. S. Cowperthwaite;E. Berger;V. A. Villar;B. D. Metzger

  • SN 2006gy: Discovery of the most luminous supernova ever recorded, powered by the death of an extremely massive star like Eta Carinae

    Nathan Smith;Weidong Li;Ryan J. Foley;J. Craig Wheeler

  • Observed Fractions of Core-Collapse Supernova Types and Initial Masses of their Single and Binary Progenitor Stars

    Nathan Smith;Nathan Smith;Weidong Li;Alexei V. Filippenko;Ryan Chornock

  • Sn 2006gy : Discovery of the most luminous supernova ever recorded, powered by the death of an extremely massive star like η carinae

    Nathan Smith;Weidong Li;Ryan J. Foley;J. Craig Wheeler

  • 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

  • 23 High Redshift Supernovae from the IfA Deep Survey: Doubling the SN Sample at z>0.7

    Brian J. Barris;John Tonry;Stephane Blondin;Peter Challis

  • An r-process Kilonova Associated with the Short-hard GRB 130603B

    Edo Berger;W Fong;R Chornock

  • Twenty-Three High-Redshift Supernovae from the Institute for Astronomy Deep Survey: Doubling the Supernova Sample at z > 0.7 * **

    Brian J. Barris;John L. Tonry;Stéphane Blondin;Peter Challis

  • Supernova 2007bi as a pair-instability explosion.

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

  • The Electromagnetic Counterpart of the Binary Neutron Star Merger LIGO/Virgo GW170817. I. Dark Energy Camera Discovery of the Optical Counterpart

    M. Soares-Santos;D. E. Holz;J. Annis;R. Chornock

Frequent Co-Authors

Edo Berger
Edo Berger Harvard University
Raffaella Margutti
Raffaella Margutti Northwestern University
Alexei V. Filippenko
Alexei V. Filippenko University of California, Berkeley
Ryan J. Foley
Ryan J. Foley University of California, Santa Cruz
Robert P. Kirshner
Robert P. Kirshner Harvard University
Adam G. Riess
Adam G. Riess Johns Hopkins University
Wen-fai Fong
Wen-fai Fong Northwestern University
Weidong Li
Weidong Li University of California, Berkeley
Brian D. Metzger
Brian D. Metzger Columbia University
Nathan Smith
Nathan Smith University of Arizona

External Links

Personal website of Ryan Chornock

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Best Scientists Citing Ryan Chornock

Peter Nugent

Peter Nugent

Lawrence Berkeley National Laboratory

Publications: 418

Jesper Sollerman

Jesper Sollerman

Stockholm University

Publications: 329

Avishay Gal-Yam

Avishay Gal-Yam

Weizmann Institute of Science

Publications: 328

Paolo A. Mazzali

Paolo A. Mazzali

Liverpool John Moores University

Publications: 299

Mansi M. Kasliwal

Mansi M. Kasliwal

California Institute of Technology

Publications: 251

Alexei V. Filippenko

Alexei V. Filippenko

University of California, Berkeley

Publications: 247

Daniel A. Perley

Daniel A. Perley

Liverpool John Moores University

Publications: 244

Adam G. Riess

Adam G. Riess

Johns Hopkins University

Publications: 242

Maximilian Stritzinger

Maximilian Stritzinger

Aarhus University

Publications: 231

Mark Sullivan

Mark Sullivan

University of Southampton

Publications: 226

Shrinivas R. Kulkarni

Shrinivas R. Kulkarni

California Institute of Technology

Publications: 218

Stefano Valenti

Stefano Valenti

University of California, Davis

Publications: 217

Ken'ichi Nomoto

Ken'ichi Nomoto

University of Tokyo

Publications: 214

Ryan J. Foley

Ryan J. Foley

University of California, Santa Cruz

Publications: 197

Masaomi Tanaka

Masaomi Tanaka

Tohoku University

Publications: 173

Nidia Morrell

Nidia Morrell

Carnegie Learning

Publications: 163

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Gustavo Tomás

Gustavo Tomás

Spanish National Research Council

Akira Fujiwara

Akira Fujiwara

NTT (Japan)

Mihai Ciobotaru

Mihai Ciobotaru

Macquarie University

Matthew A. Lambon Ralph

Matthew A. Lambon Ralph

University of Cambridge

Sonja Utz

Sonja Utz

Leibniz-Institut für Wissensmedien

Steve Schnetzer

Steve Schnetzer

Rutgers, The State University of New Jersey

Matthew L. Lister

Matthew L. Lister

Purdue University West Lafayette

Teun Boekhout

Teun Boekhout

University of Amsterdam

Jacques Laval

Jacques Laval

Institut Gustave Roussy

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Johannes Nimpf

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