World's Best Scientists 2026 revealed!
Bo Milvang-Jensen

Bo Milvang-Jensen

D-Index & Metrics

Physics

D-Index
96
Citations
29941
World Ranking
1886
National Ranking
14

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.

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: 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.

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.

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: 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.

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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