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Physics

D-Index
82
Citations
26989
World Ranking
2838
National Ranking
1392

Joel N. Bregman 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 Joel N. Bregman 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: 472 publications — 51st percentile

51% of scientists in this discipline score the same or lower.

The last bar groups every scientist with 1,469 publications or more.

Joel N. Bregman 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 Joel N. Bregman 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: 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.

Overview

Joel N. Bregman is affiliated with the University of Michigan-Ann Arbor in the United States. Their research primarily falls within the broad field of Physics and Astronomy, with a focus on Astronomy and Astrophysics among other specialized subfields.

Their scholarly work spans a variety of subfields including:

  • Astronomy and Astrophysics
  • Nuclear and High Energy Physics
  • Instrumentation
  • Atomic and Molecular Physics, and Optics
  • Statistical and Nonlinear Physics

Bregman's main research topics include:

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

Their recent papers comprise works published between 2021 and 2023, including:

  • Hot Extended Galaxy Halos around Local L* Galaxies from Sunyaev-Zeldovich Measurements, 2022, The Astrophysical Journal
  • Line Emission Mapper (LEM): Probing the physics of cosmic ecosystems, 2022, arXiv (Cornell University)
  • Scientific objectives of the Hot Universe Baryon Surveyor (HUBS) mission, 2023, Science China Physics Mechanics and Astronomy
  • eDIG-CHANGES I: extended Hα emission from the extraplanar diffuse ionized gas (eDIG) around CHANG-ES galaxies, 2023, Monthly Notices of the Royal Astronomical Society
  • An X-Ray- and SZ-bright Diffuse Source toward M31: A Local Hot Bridge, 2021, The Astrophysical Journal

Bregman frequently collaborates with a number of coauthors, including:

  • Zhijie Qu
  • Jiangtao Li
  • Taotao Fang
  • Q. Daniel Wang
  • Cameron T. Pratt

The venues where Bregman most often publishes include:

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

Best Publications

  • LOFAR: The LOw-Frequency ARray

    M. P. van Haarlem;M. W. Wise;M. W. Wise;A. W. Gunst;George Heald

  • LOFAR: The LOw-Frequency ARray

    M. P. van Haarlem;M. W. Wise;A. W. Gunst;G. Heald

  • The Hot and Energetic Universe: A White Paper presenting the science theme motivating the Athena+ mission

    Kirpal Nandra;Didier Barret;Xavier Barcons;Andy Fabian

  • The Search for the Missing Baryons at Low Redshift

    Joel N. Bregman

  • An Infrared Survey of Brightest Cluster Galaxies. II: Why are Some Brightest Cluster Galaxies Forming Stars?

    Christopher P. O'Dea;Stefi A. Baum;George Privon;Jacob Noel-Storr

  • Global Models of the Interstellar Medium in Disk Galaxies

    Alexander Rosen;Joel N. Bregman

  • CONSTRAINING THE MILKY WAY'S HOT GAS HALO WITH O VII AND O VIII EMISSION LINES

    Matthew J. Miller;Joel N. Bregman

  • Do Hot Halos Around Galaxies Contain the Missing Baryons

    Michael E. Anderson;Joel N. Bregman

  • Observing pulsars and fast transients with LOFAR

    B. W. Stappers;J. W. T. Hessels;J. W. T. Hessels;A. Alexov;K. Anderson

  • Constraining the Milky Way's Hot Gas Halo with OVII and OVII Emission Lines

    Matthew J. Miller;Joel N. Bregman

  • The Structure of the Milky Way's Hot Gas Halo

    Matthew J. Miller;Joel N. Bregman

  • Creation of cosmic structure in the complex galaxy cluster merger Abell 2744

    J. Merten;D. Coe;R. Dupke;R. Massey

  • Do Hot Haloes Around Galaxies Contain the Missing Baryons

    Michael E. Anderson;Joel N. Bregman

  • Puzzling accretion onto a black hole in the ultraluminous X-ray source M 101 ULX-1

    Ji Feng Liu;Joel N. Bregman;Yu Bai;Stephen Justham

  • DETECTION OF A HOT GASEOUS HALO AROUND THE GIANT SPIRAL GALAXY NGC 1961

    Michael E. Anderson;Joel N. Bregman

  • Optical and radio variability in blazars

    Beth R. Hufnagel;Joel N. Bregman

  • X-Ray Absorption from the Milky Way Halo and the Local Group

    Joel N. Bregman;Edward J. Lloyd-Davies

  • CHANDRA X-RAY OBSERVATIONS OF THE X-RAY FAINT ELLIPTICAL GALAXY NGC 4697

    Craig L. Sarazin;Jimmy A. Irwin;Joel N. Bregman

  • X-Ray Spectral Properties of Low-Mass X-Ray Binaries in Nearby Galaxies

    Jimmy A. Irwin;Alex E. Athey;Joel N. Bregman

  • Ultraluminous X-Ray Sources in Nearby Galaxies from ROSAT High Resolution Imager Observations I. Data Analysis

    Ji-Feng Liu;Joel N. Bregman

Frequent Co-Authors

Craig L. Sarazin
Craig L. Sarazin University of Virginia
Brian R. McNamara
Brian R. McNamara University of Waterloo
Michael W. Wise
Michael W. Wise Netherlands Institute for Space Research
Megan Donahue
Megan Donahue Michigan State University
Christopher P. O'Dea
Christopher P. O'Dea University of Manitoba
Stefi A. Baum
Stefi A. Baum University of Manitoba
Jon M. Miller
Jon M. Miller University of Michigan–Ann Arbor
Heino Falcke
Heino Falcke Radboud University
Michael Kramer
Michael Kramer Max Planck Institute for Radio Astronomy
Jason W. T. Hessels
Jason W. T. Hessels University of Amsterdam

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