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Bo Milvang-Jensen

Bo Milvang-Jensen

D-Index & Metrics

Discipline name D-Index World Ranking Current World Ranking National Ranking Current National Ranking Publications Citations
Physics 96 1886 1791 14 14 361 29941

Bo Milvang-Jensen publications per year

The chart shows the history of publications by Bo Milvang-Jensen between 1997 and 2024, highlighting the no. of papers published in each year and offering an overview of the publication velocity of this scholar. Bo Milvang-Jensen published across 28 years, from 1997 to 2024, averaging 13 papers a year. Output peaked at 43 publications in 2012. 9 of the 365 publications appeared in the last two years.

No. of publications
10 20 30 40
Bar chart. Horizontal axis: year, 1997 to 2024. Vertical axis: number of publications, 0 to 43. Peak 43 publications in 2012. 1997: 1 publication 1998: 0 publications 1999: 2 publications 2000: 1 publication 2001: 0 publications 2002: 3 publications 2003: 4 publications 2004: 11 publications 2005: 11 publications 2006: 14 publications 2007: 10 publications 2008: 21 publications 2009: 22 publications 2010: 14 publications 2011: 31 publications 2012: 43 publications 2013: 29 publications 2014: 20 publications 2015: 18 publications 2016: 18 publications 2017: 26 publications 2018: 13 publications 2019: 22 publications 2020: 7 publications 2021: 9 publications 2022: 6 publications 2023: 6 publications 2024: 3 publications
1997 2024

365 publications in total across all disciplines

View publications per year as a table
Bo Milvang-Jensen: publications per year, 1997 to 2024
Year Publications
1997 1
1998 0
1999 2
2000 1
2001 0
2002 3
2003 4
2004 11
2005 11
2006 14
2007 10
2008 21
2009 22
2010 14
2011 31
2012 43
2013 29
2014 20
2015 18
2016 18
2017 26
2018 13
2019 22
2020 7
2021 9
2022 6
2023 6
2024 3
Total 365
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Bo Milvang-Jensen 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 Bo Milvang-Jensen 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, 343–362 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: 361 publications — 30th percentile

30% 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
343–362 155 361
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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Bo Milvang-Jensen 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 Bo Milvang-Jensen 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, 96–97 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: 96 D-Index — 50th percentile

50% 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 96
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

Bo Milvang-Jensen is affiliated with the University of Copenhagen in Denmark and specializes in the field of Physics and Astronomy. Their research has a significant focus on Astronomy and Astrophysics, covering aspects such as instrumentation, nuclear and high-energy physics, computer vision and pattern recognition, and electrical and electronic engineering.

The scientist's scholarly work centers on several main topics, including:

  • Gamma-ray bursts and supernovae
  • Galaxies: Formation, Evolution, Phenomena
  • Astronomy and Astrophysical Research
  • Astrophysical Phenomena and Observations
  • Stellar, planetary, and galactic studies
  • Pulsars and Gravitational Waves Research
  • Astrophysics and Cosmic Phenomena

Bo Milvang-Jensen has contributed to numerous peer-reviewed papers published in well-regarded venues, with recent examples comprising:

  • COSMOS2020: A Panchromatic View of the Universe to z ∼ 10 from Two Complementary Catalogs, 2022, The Astrophysical Journal Supplement Series
  • The evolution of the galaxy UV luminosity function at redshifts z ≃ 8 - 15 from deep JWST and ground-based near-infrared imaging, 2022, Monthly Notices of the Royal Astronomical Society
  • A lack of evolution in the very bright end of the galaxy luminosity function from z ≃ 8 to 10, 2020, Monthly Notices of the Royal Astronomical Society
  • A first look at the SMACS0723 JWST ERO: spectroscopic redshifts, stellar masses, and star-formation histories, 2022, Monthly Notices of the Royal Astronomical Society Letters
  • COSMOS2020: Cosmic evolution of the stellar-to-halo mass relation for central and satellite galaxies up to z ∼ 6.5, 2022, Astronomy and Astrophysics

Key publication venues where Bo Milvang-Jensen frequently publishes include:

  • Monthly Notices of the Royal Astronomical Society
  • Astronomy and Astrophysics
  • arXiv (Cornell University)
  • The Astrophysical Journal Supplement Series
  • Monthly Notices of the Royal Astronomical Society Letters

Collaborations are an important aspect of this scientist's research. Frequent co-authors include:

  • J. P. U. Fynbo
  • K. E. Heintz
  • A. J. Levan
  • N. R. Tanvir
  • H. J. McCracken

Best Publications

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

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

  • The COSMOS2015 Catalog: Exploring the 1 < z < 6 Universe with Half a Million Galaxies

    C. Laigle;H. J. McCracken;O. Ilbert;B. C. Hsieh

  • Mass assembly in quiescent and star-forming galaxies since z ≃ 4 from UltraVISTA

    O. Ilbert;H. J. McCracken;O. Le Fevre;P. Capak

  • THE EVOLUTION OF THE STELLAR MASS FUNCTIONS OF STAR-FORMING AND QUIESCENT GALAXIES TO z = 4 FROM THE COSMOS/UltraVISTA SURVEY*

    Adam Muzzin;Danilo Marchesini;Mauro Stefanon;Marijn Franx

  • The Emergence of a Lanthanide-Rich Kilonova Following the Merger of Two Neutron Stars

    N. R. Tanvir;A. J. Levan;C. González-Fernández;O. Korobkin

  • UltraVISTA: a new ultra-deep near-infrared survey in COSMOS

    H. J. McCracken;B. Milvang-Jensen;J. Dunlop;M. Franx

  • The Emergence of a Lanthanide-Rich Kilonova Following the Merger of Two Neutron Stars

    N. R. Tanvir;A. J. Levan;C. Gonzalez-Fernandez;O. Korobkin

  • 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

  • A Public Ks-selected Catalog in the COSMOS/UltraVISTA Field: Photometry, Photometric Redshifts and Stellar Population Parameters

    Adam Muzzin;Danilo Marchesini;Mauro Stefanon;Marijn Franx

  • A PUBLIC K-s-SELECTED CATALOG IN THE COSMOS/ULTRAVISTA FIELD: PHOTOMETRY, PHOTOMETRIC REDSHIFTS, AND STELLAR POPULATION PARAMETERS

    Adam Muzzin;Danilo Marchesini;Mauro Stefanon;Marijn Franx

  • 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 evolution of the star formation activity in galaxies and its dependence on environment

    B. M. Poggianti;A. von der Linden;G. De Lucia;V. Desai

  • The evolution of the star formation activity in galaxies and its dependence on environment

    Bianca M. Poggianti;Anja von der Linden;Gabriella De Lucia;Vandana Desai

  • Localization and broadband follow-up of the gravitational-wave transient GW150914

    B. P. Abbott;R. Abbott;T. D. Abbott;M. R. Abernathy

  • Localization and broadband follow-up of the gravitational-wave transient GW150914

    B. P. Abbott;R. Abbott;T. D. Abbott;M. R. Abernathy

  • GRB 080913 at redshift 6.7

    J. Greiner;T. Kruehler;J. P. U. Fynbo;A. Rossi

  • Ultraviolet emission lines in young low-mass galaxies at z ≃ 2: physical properties and implications for studies at z > 7

    Daniel P. Stark;Johan Richard;Brian Siana;Stéphane Charlot

  • GRB 080913 AT REDSHIFT 6.7

    J. Greiner;T. Krühler;J. P. U. Fynbo;A. Rossi

  • A Population of Massive, Luminous Galaxies Hosting Heavily Dust-Obscured Gamma-Ray Bursts: Implications for the Use of GRBs as Tracers of Cosmic Star Formation

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

  • GRB hosts through cosmic time - VLT/X-Shooter emission-line spectroscopy of 96 GRB-selected galaxies at 0.1 < z < 3.6

    T. Krühler;D. Malesani;J. P. U. Fynbo;O. E. Hartoog

Frequent Co-Authors

Johan P. U. Fynbo
Johan P. U. Fynbo University of Copenhagen
Jens Hjorth
Jens Hjorth University of Copenhagen
Pall Jakobsson
Pall Jakobsson University of Iceland
Pascale Jablonka
Pascale Jablonka École Polytechnique Fédérale de Lausanne
Alfonso Aragón-Salamanca
Alfonso Aragón-Salamanca University of Nottingham
Dennis Zaritsky
Dennis Zaritsky University of Arizona
Darach Watson
Darach Watson University of Copenhagen
Nial R. Tanvir
Nial R. Tanvir University of Leicester
Roberto P. Saglia
Roberto P. Saglia Max Planck Society
H. J. McCracken
H. J. McCracken Institut d'Astrophysique de Paris

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