World's Best Scientists 2026 revealed!

D-Index & Metrics

Physics

D-Index
106
Citations
54191
World Ranking
1313
National Ranking
109

Roberto Neri 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 Roberto Neri 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: 358 publications — 29th percentile

29% of scientists in this discipline score the same or lower.

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

Roberto Neri 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 Roberto Neri 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: 106 D-Index — 65th percentile

65% of scientists in this discipline score the same or lower.

The last bar groups every scientist with 185 D-Index or more.

Overview

Roberto Neri is affiliated with the Max Planck Society in Germany and has made significant contributions to the fields of physics and astronomy, with a particular focus on astrophysics and star formation studies.

Their scholarly work spans multiple subfields, including astronomy and astrophysics, spectroscopy, atmospheric science, instrumentation, and nuclear and high energy physics. This breadth is reflected in the diversity of topics within their research portfolio.

Main topics of their research encompass:

  • Astrophysics and Star Formation Studies
  • Galaxies: Formation, Evolution, Phenomena
  • Stellar, planetary, and galactic studies
  • Molecular Spectroscopy and Structure
  • Atmospheric Ozone and Climate
  • Astronomy and Astrophysical Research
  • Astrophysical Phenomena and Observations

Their publications are frequent in recognized scientific journals, with a high number of papers appearing in:

  • Astronomy and Astrophysics
  • arXiv (Cornell University)
  • The Astrophysical Journal
  • Monthly Notices of the Royal Astronomical Society
  • EPJ Web of Conferences

Among their recent research contributions are:

  • "Rotation Curves in z ∼ 1-2 Star-forming Disks: Evidence for Cored Dark Matter Distributions" (2020), published in The Astrophysical Journal
  • "PRODIGE - envelope to disk with NOEMA" (2022), published in Astronomy and Astrophysics
  • "Microwave background temperature at a redshift of 6.34 from H2O absorption" (2022), published in Nature
  • "Plateau de Bure High-z Blue Sequence Survey 2 (PHIBSS2): Search for Secondary Sources, CO Luminosity Functions in the Field, and the Evolution of Molecular Gas Density through Cosmic Time*" (2020), published in The Astronomical Journal
  • "Physical Constraints on the Extended Interstellar Medium of the z = 6.42 Quasar J1148+5251: [C ii]158 μm, [N ii]205 μm, and [O i]146 μm Observations" (2022), published in The Astrophysical Journal

Frequent collaborators in their scientific endeavors include:

  • P. Caselli
  • Dominik A. Riechers
  • P. Cox
  • A. Omont
  • C. Ceccarelli

Their extensive research output has contributed to the understanding of galaxy formation and evolution, molecular spectroscopy, and interstellar medium properties, among other astrophysical phenomena. The scientist's work is widely cited and integrated into ongoing research conversations in the physics and astronomy communities.

Best Publications

  • First M87 Event Horizon Telescope Results. I. The Shadow of the Supermassive Black Hole

    Kazunori Akiyama;Antxon Alberdi;Walter Alef

  • First M87 Event Horizon Telescope Results. IV. Imaging the Central Supermassive Black Hole

    Kazunori Akiyama;Antxon Alberdi;Walter Alef

  • A Study of the Gas-Star Formation Relation over Cosmic Time

    R.Genzel;L.J.Tacconi;J.Gracia-Carpio;A.Sternberg

  • PHIBSS: molecular gas content and scaling relations in z~1-3 normal star forming galaxies

    L. J. Tacconi;R. Neri;R. Genzel;F. Combes

  • First M87 Event Horizon Telescope Results. VI. The Shadow and Mass of the Central Black Hole

    Kazunori Akiyama;Antxon Alberdi;Walter Alef

  • First M87 Event Horizon Telescope Results. V. Physical Origin of the Asymmetric Ring

    Kazunori Akiyama;Antxon Alberdi;Walter Alef

  • High molecular gas fractions in normal massive star-forming galaxies in the young Universe

    L. J. Tacconi;R. Genzel;R. Neri;P. Cox

  • Submillimeter Galaxies at z~2: Evidence for Major Mergers & Constraints on Lifetimes, IMF and CO-H2 Conversion Factor

    L.J. Tacconi;R. Genzel;I. Smail;R. Neri

  • First M87 Event Horizon Telescope Results. II. Array and Instrumentation

    Kazunori Akiyama;Antxon Alberdi;Walter Alef

  • First M87 Event Horizon Telescope Results. III. Data Processing and Calibration

    Kazunori Akiyama;Antxon Alberdi;Walter Alef

  • Massive molecular outflows and evidence for AGN feedback from CO observations

    C. Cicone;R. Maiolino;E. Sturm;J. Gracia-Carpio

  • PHIBSS: Unified Scaling Relations of Gas Depletion Time and Molecular Gas Fractions

    L. J. Tacconi;R. Genzel;A. Saintonge;F. Combes

  • COMBINED CO AND DUST SCALING RELATIONS OF DEPLETION TIME AND MOLECULAR GAS FRACTIONS WITH COSMIC TIME, SPECIFIC STAR-FORMATION RATE, AND STELLAR MASS

    R. Genzel;L. J. Tacconi;D. Lutz;A. Saintonge

  • High-resolution millimeter imaging of submillimeter galaxies

    L. J. Tacconi;R. Neri;S. C. Chapman;R. Genzel

  • A dust-obscured massive maximum-starburst galaxy at a redshift of 6.34

    Dominik A. Riechers;Dominik A. Riechers;C. M. Bradford;C. M. Bradford;D. L. Clements;C. D. Dowell;C. D. Dowell

  • The Detection of a Population of Submillimeter-Bright, Strongly Lensed Galaxies

    Mattia Negrello;R. Hopwood;G. De Zotti;A. Cooray

  • A survey of molecular gas in luminous sub-millimetre galaxies

    M. S. Bothwell;M. S. Bothwell;Ian Smail;S. C. Chapman;R. Genzel

  • Evidence of strong quasar feedback in the early Universe

    R. Maiolino;S. Gallerani;R. Neri;C. Cicone

  • Intense star formation within resolved compact regions in a galaxy at z = 2.3

    A.M. Swinbank;I. Smail;S. Longmore;A.I. Harris

  • First M87 Event Horizon Telescope Results. VIII. Magnetic Field Structure near the Event Horizon

    Kazunori Akiyama;Kazunori Akiyama;Kazunori Akiyama;Juan Carlos Algaba;Antxon Alberdi;Walter Alef

Frequent Co-Authors

Fabian Walter
Fabian Walter Max Planck Society
Santiago García-Burillo
Santiago García-Burillo Spanish National Observatory
Francoise Combes
Francoise Combes Collège de France
Rob Ivison
Rob Ivison European Southern Observatory
Linda J. Tacconi
Linda J. Tacconi Max Planck Institute for Extraterrestrial Physics
Alain Omont
Alain Omont Institut d'Astrophysique de Paris
Remo P. J. Tilanus
Remo P. J. Tilanus University of Arizona
Andreas Eckart
Andreas Eckart University of Cologne
Svetlana G. Jorstad
Svetlana G. Jorstad Boston University
Ue-Li Pen
Ue-Li Pen University of Toronto

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