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Justyn R. Maund

D-Index & Metrics

Discipline name D-Index World Ranking Current World Ranking National Ranking Current National Ranking Publications Citations
Physics 74 3492 3318 307 295 250 15427

Justyn R. Maund publications per year

The chart shows the history of publications by Justyn R. Maund between 2003 and 2021, highlighting the no. of papers published in each year and offering an overview of the publication velocity of this scholar. Justyn R. Maund published across 19 years, from 2003 to 2021, averaging 12.1 papers a year. Output peaked at 21 publications in 2021. 40 of the 229 publications appeared in the last two years.

No. of publications
5 10 15 20
Bar chart. Horizontal axis: year, 2003 to 2021. Vertical axis: number of publications, 0 to 21. Peak 21 publications in 2021. 2003: 1 publication 2004: 2 publications 2005: 7 publications 2006: 5 publications 2007: 12 publications 2008: 8 publications 2009: 17 publications 2010: 17 publications 2011: 9 publications 2012: 12 publications 2013: 13 publications 2014: 13 publications 2015: 14 publications 2016: 15 publications 2017: 19 publications 2018: 6 publications 2019: 19 publications 2020: 19 publications 2021: 21 publications
2003 2021

229 publications in total across all disciplines

View publications per year as a table
Justyn R. Maund: publications per year, 2003 to 2021
Year Publications
2003 1
2004 2
2005 7
2006 5
2007 12
2008 8
2009 17
2010 17
2011 9
2012 12
2013 13
2014 13
2015 14
2016 15
2017 19
2018 6
2019 19
2020 19
2021 21
Total 229
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Justyn R. Maund 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 Justyn R. Maund 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, 243–262 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: 250 publications — 9th percentile

9% 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
243–262 112 250
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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Justyn R. Maund 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 Justyn R. Maund 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, 74–75 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: 74 D-Index — 7th percentile

7% 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 74
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
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

What is he best known for?

The fields of study he is best known for:

  • Astronomy
  • Galaxy
  • Astrophysics

The scientist’s investigation covers issues in Astrophysics, Astronomy, Galaxy, Supernova and Spectral line. His is involved in several facets of Astrophysics study, as is seen by his studies on Stellar evolution, Type II supernova, Redshift, Stars and Metallicity. His work on Ejecta, Spectroscopy, Stellar black hole and Binary black hole as part of general Astronomy study is frequently linked to Type, therefore connecting diverse disciplines of science.

His study in Quasar and Extinction is done as part of Galaxy. His studies deal with areas such as Supergiant, Red supergiant, Light curve and Spiral galaxy as well as Supernova. The various areas that he examines in his Supergiant study include Variable star, Giant star and Altair.

His most cited work include:

  • The death of massive stars – I. Observational constraints on the progenitors of Type II-P supernovae (658 citations)
  • The death of massive stars – I. Observational constraints on the progenitors of Type II-P supernovae (658 citations)
  • A γ-ray burst at a redshift of z ≈ 8.2 (574 citations)

What are the main themes of his work throughout his whole career to date?

Justyn R. Maund mostly deals with Astrophysics, Supernova, Astronomy, Galaxy and Stars. The Astrophysics study combines topics in areas such as Spectral line and Polarization. His Supernova research incorporates elements of Supergiant, Luminosity, Stellar evolution and Photometry.

His Stellar evolution research incorporates themes from Star formation and Altair. His Galaxy research is multidisciplinary, relying on both Gamma-ray burst and Cosmic dust. In his work, Flattening is strongly intertwined with Radioactive decay, which is a subfield of Light curve.

He most often published in these fields:

  • Astrophysics (109.06%)
  • Supernova (84.15%)
  • Astronomy (50.94%)

What were the highlights of his more recent work (between 2017-2021)?

  • Astrophysics (109.06%)
  • Supernova (84.15%)
  • Light curve (25.28%)

In recent papers he was focusing on the following fields of study:

Justyn R. Maund focuses on Astrophysics, Supernova, Light curve, Stars and Polarization. Justyn R. Maund focuses mostly in the field of Astrophysics, narrowing it down to topics relating to Spectral line and, in certain cases, Helium. Justyn R. Maund has researched Supernova in several fields, including Spectral energy distribution, Polarimetry, Magnetar, Spectroscopy and Red supergiant.

His Magnetar research integrates issues from Galaxy and Spiral galaxy. His Light curve study combines topics in areas such as Radioactive decay, Gravitational microlensing and Envelope. His work on Radial velocity, Orbital period and Bulge as part of general Stars study is frequently connected to Orbit, therefore bridging the gap between diverse disciplines of science and establishing a new relationship between them.

Between 2017 and 2021, his most popular works were:

  • Late-time Flattening of Type Ia Supernova Light Curves: Constraints from SN 2014J in M82 (33 citations)
  • The very young resolved stellar populations around stripped-envelope supernovae (32 citations)
  • The Type II-Plateau Supernova 2017eaw in NGC 6946 and Its Red Supergiant Progenitor (27 citations)

In his most recent research, the most cited papers focused on:

  • Astronomy
  • Milky Way
  • Galaxy

His primary scientific interests are in Astrophysics, Supernova, Polarization, Stars and Light curve. His study in Astrophysics concentrates on Ejecta, Very Large Telescope, Gravitational wave, Neutron star and Supergiant. His work carried out in the field of Supernova brings together such families of science as Polarimetry, Wavelength, Red supergiant and Chandrasekhar limit, White dwarf.

His work deals with themes such as Scattering, Magnetar, Circumstellar dust and Galaxy, Interstellar medium, which intersect with Polarimetry. His study in Red supergiant is interdisciplinary in nature, drawing from both Spectral energy distribution, Photosphere, Metallicity and Spitzer Space Telescope. His study on Radial velocity, Gravitational microlensing, Orbital period and Bulge is often connected to Orbit as part of broader study in Stars.

Best Publications

  • A γ-ray burst at a redshift of z ≈ 8.2

    N. R. Tanvir;D. B. Fox;A. J. Levan;E. Berger

  • The death of massive stars – I. Observational constraints on the progenitors of Type II-P supernovae

    S. J. Smartt;J. J. Eldridge;R. M. Crockett;J. R. Maund;J. R. Maund

  • Low-Resolution Spectroscopy of Gamma-ray Burst Optical Afterglows: Biases in the Swift Sample and Characterization of the Absorbers

    J. P. U. Fynbo;P. Jakobsson;J. X. Prochaska;D. Malesani

  • Low-resolution Spectroscopy of Gamma-ray Burst Optical Afterglows: Biases in the Swift Sample and Characterization of the Absorbers

    J. P. U. Fynbo;J. P. U. Fynbo;P. Jakobsson;J. X. Prochaska;D. Malesani

  • The massive binary companion star to the progenitor of supernova 1993J

    Justyn R. Maund;Stephen J. Smartt;Rolf P. Kudritzki;Philipp Podsiadlowski

  • PESSTO : survey description and products from the first data release by the Public ESO Spectroscopic Survey of Transient Objects

    S. J. Smartt;S. Valenti;M. Fraser;C. Inserra

  • SN 2005cs in M51 II. Complete Evolution in the Optical and the Near-Infrared

    A. Pastorello;S. Valenti;L. Zampieri;H. Navasardyan

  • SN 2005cs in M51 – II. Complete evolution in the optical and the near-infrared

    A. Pastorello;S. Valenti;L. Zampieri;H. Navasardyan

  • PESSTO: survey description and products from the first data release by the Public ESO Spectroscopic Survey of Transient Objects

    S. J. Smartt;S. Valenti;S. Valenti;M. Fraser;C. Inserra

  • The superluminous transient ASASSN-15lh as a tidal disruption event from a Kerr black hole

    G. Leloudas;G. Leloudas;M. Fraser;N. C. Stone;S. van Velzen

  • Rapid formation of large dust grains in the luminous supernova 2010jl

    Christa Gall;Christa Gall;Christa Gall;Jens Hjorth;Darach Watson;Eli Dwek

  • Detection of a red supergiant progenitor star of a type II-plateau supernova.

    Stephen J. Smartt;Justyn R. Maund;Margaret A. Hendry;Christopher A. Tout

  • The Progenitor of SN 2005cs in the Whirlpool Galaxy

    J. R. Maund;S. J. Smartt;I. J. Danziger

  • The Superluminous Transient ASASSN-15lh as a Tidal Disruption Event from a Kerr Black Hole

    G. Leloudas;M. Fraser;N. C. Stone;S. van Velzen

  • THE YELLOW SUPERGIANT PROGENITOR OF THE TYPE II SUPERNOVA 2011dh IN M51

    Justyn Maund;Justyn Maund;Morgan Fraser;M. Ergon;A. Pastorello

  • Galaxy Counterparts of metal-rich Damped Lyman-alpha Absorbers - I: The case of the z=2.35 DLA towards Q2222-0946

    J. P. U. Fynbo;P. Laursen;C. Ledoux;A. K. Durgapal

  • Galaxy counterparts of metal-rich damped Lyman-alpha absorbers - II. A solar-metallicity and dusty DLA at z_abs=2.58

    J. P. U. Fynbo;C. Ledoux;P. Noterdaeme;L. Christensen

  • The first month of evolution of the slow-rising Type IIP SN 2013ej in M74

    S. Valenti;S. Valenti;D. Sand;A. Pastorello;M. L. Graham

  • The progenitor of SN 2005cs in the Whirlpool Galaxy

    Justyn R. Maund;Stephen J. Smartt;I. John Danziger

  • Galaxy counterparts of metal-rich damped Lyα absorbers – I. The case of the z= 2.35 DLA towards Q 2222−0946

    J. P. U. Fynbo;P. Laursen;C. Ledoux;P. Moller

Frequent Co-Authors

Ferdinando Patat
Ferdinando Patat European Southern Observatory
Jesper Sollerman
Jesper Sollerman Stockholm University
Stefano Valenti
Stefano Valenti University of California, Davis
Andrea Pastorello
Andrea Pastorello National Institute for Astrophysics
Avishay Gal-Yam
Avishay Gal-Yam Weizmann Institute of Science
Nancy Elias-Rosa
Nancy Elias-Rosa Spanish National Research Council
John C Wheeler
John C Wheeler The University of Texas at Austin
Stefano Benetti
Stefano Benetti National Institute for Astrophysics
Johan P. U. Fynbo
Johan P. U. Fynbo University of Copenhagen
Enrico Cappellaro
Enrico Cappellaro National Institute for Astrophysics

External Links

Personal website of Justyn R. Maund

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Best Scientists Citing Justyn R. Maund

Jesper Sollerman

Jesper Sollerman

Stockholm University

Publications: 184

Avishay Gal-Yam

Avishay Gal-Yam

Weizmann Institute of Science

Publications: 174

Peter Nugent

Peter Nugent

Lawrence Berkeley National Laboratory

Publications: 157

Stefano Valenti

Stefano Valenti

University of California, Davis

Publications: 153

Paolo A. Mazzali

Paolo A. Mazzali

Liverpool John Moores University

Publications: 143

Johan P. U. Fynbo

Johan P. U. Fynbo

University of Copenhagen

Publications: 140

Maximilian Stritzinger

Maximilian Stritzinger

Aarhus University

Publications: 140

Nancy Elias-Rosa

Nancy Elias-Rosa

Spanish National Research Council

Publications: 125

Daniel A. Perley

Daniel A. Perley

Liverpool John Moores University

Publications: 123

Mario Hamuy

Mario Hamuy

University of Chile

Publications: 119

Alexei V. Filippenko

Alexei V. Filippenko

University of California, Berkeley

Publications: 109

Nathan Smith

Nathan Smith

University of Arizona

Publications: 106

Mansi M. Kasliwal

Mansi M. Kasliwal

California Institute of Technology

Publications: 102

Mark Sullivan

Mark Sullivan

University of Southampton

Publications: 99

Ryan Chornock

Ryan Chornock

Northwestern University

Publications: 94

Nidia Morrell

Nidia Morrell

Carnegie Learning

Publications: 92

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