World's Best Scientists 2026 revealed!

D-Index & Metrics

Physics

D-Index
72
Citations
19688
World Ranking
3581
National Ranking
1

Andrea V. Macciò 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 Andrea V. Macciò 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: 227 publications — 6th percentile

6% of scientists in this discipline score the same or lower.

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

Andrea V. Macciò 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 Andrea V. Macciò 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: 72 D-Index — 3rd percentile

3% of scientists in this discipline score the same or lower.

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

Overview

Andrea V. Macciò is affiliated with New York University Abu Dhabi in the United Arab Emirates. Their research primarily addresses topics within the fields of Physics and Astronomy, with a focus on Astronomy and Astrophysics, Instrumentation, and Nuclear and High Energy Physics, among other related subfields.

The scientist's work covers key areas such as Galaxies: Formation, Evolution, Phenomena; Astronomy and Astrophysical Research; Stellar, planetary, and galactic studies; Cosmology and Gravitation Theories; Astrophysics and Star Formation Studies; Astrophysical Phenomena and Observations; and Gamma-ray bursts and supernovae.

Andrea V. Macciò has contributed frequently to well-known publication venues, including:

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

Their recent papers illustrate a focus on galaxy formation and dark matter, including the following works:

  • "Exploring the origin of low-metallicity stars in Milky-Way-like galaxies with the NIHAO-UHD simulations," 2020, Monthly Notices of the Royal Astronomical Society
  • "The Dekel-Zhao profile: a mass-dependent dark-matter density profile with flexible inner slope and analytic potential, velocity dispersion, and lensing properties," 2020, Monthly Notices of the Royal Astronomical Society
  • "Creating a galaxy lacking dark matter in a dark matter-dominated universe," 2020, Monthly Notices of the Royal Astronomical Society
  • "NIHAO - XXV. Convergence in the cusp-core transformation of cold dark matter haloes at high star formation thresholds," 2020, Monthly Notices of the Royal Astronomical Society
  • "NIHAO-XXIII. Dark matter density shaped by black hole feedback," 2020, Monthly Notices of the Royal Astronomical Society Letters

Collaboration features prominently in their work, with frequent coauthors including Tobias Buck, Aura Obreja, Xi Kang, Marvin Blank, and Stefan Waterval. This reflects an engaged research network within their areas of expertise.

Best Publications

  • Constraints on the relationship between stellar mass and halo mass at low and high redshift

    Benjamin P. Moster;Rachel S. Somerville;Rachel S. Somerville;Christian Maulbetsch;Frank C. van den Bosch

  • Cold dark matter haloes in the Planck era: evolution of structural parameters for Einasto and NFW profiles

    Aaron A. Dutton;Andrea V. Macciò

  • Concentration, spin and shape of dark matter haloes as a function of the cosmological model: WMAP1, WMAP3 and WMAP5 results

    Andrea V. Macciò;Aaron A. Dutton;Frank C. Van Den Bosch

  • Concentration, spin and shape of dark matter haloes: Scatter and the dependence on mass and environment

    Andrea V. Macciò;Andrea V. Macciò;Aaron A. Dutton;Frank C. Van Den Bosch;Ben Moore

  • The dependence of dark matter profiles on the stellar-to-halo mass ratio: a prediction for cusps versus cores

    Arianna Di Cintio;Chris B. Brook;Andrea V. Macciò;Greg S. Stinson

  • Making Galaxies in a Cosmological Context: The Need for Early Stellar Feedback

    G. S. Stinson;C. Brook;A. V. Macciò;J. Wadsley

  • THE NON-CAUSAL ORIGIN OF THE BLACK-HOLE-GALAXY SCALING RELATIONS

    Knud Jahnke;Andrea V. Macciò

  • Towards a Concordant Model of Halo Occupation Statistics

    Frank C. van den Bosch;Xiaohu Yang;H.J. Mo;Simone M. Weinmann

  • NIHAO project – I. Reproducing the inefficiency of galaxy formation across cosmic time with a large sample of cosmological hydrodynamical simulations

    Liang Wang;Liang Wang;Liang Wang;Aaron A. Dutton;Gregory S. Stinson;Andrea V. Macciò

  • A quantitative explanation of the observed population of Milky Way satellite galaxies

    Sergey E. Koposov;Sergey E. Koposov;Sergey E. Koposov;Jaiyul Yoo;Hans-Walter Rix;David H. Weinberg

  • Towards a concordant model of halo occupation statistics

    Frank C. Van Den Bosch;Xiaohu Yang;H. J. Mo;Simone M. Weinmann

  • A mass-dependent density profile for dark matter haloes including the influence of galaxy formation

    Arianna Di Cintio;Chris B. Brook;Aaron A. Dutton;Andrea V. Macciò

  • Non-linear evolution of cosmological structures in warm dark matter models

    Aurel Schneider;Robert E. Smith;Andrea V. Macciò;Ben Moore

  • The Redshift Evolution of LCDM Halo Parameters: Concentration, Spin, and Shape

    J. C. Muñoz-Cuartas;A. V. Macciò;S. Gottlöber;A. A. Dutton

  • Nonlinear Evolution of Cosmological Structures in Warm Dark Matter Models

    Aurel Schneider;Robert E. Smith;Andrea V. Maccio;Ben Moore

  • NIHAO – IV: core creation and destruction in dark matter density profiles across cosmic time

    Edouard Tollet;Edouard Tollet;Andrea V. Macciò;Andrea V. Macciò;Aaron A. Dutton;Aaron A. Dutton;Greg S. Stinson

  • Cores in warm dark matter haloes: a Catch 22 problem

    Andrea V. Macciò;Sinziana Paduroiu;Donnino Anderhalden;Aurel Schneider

  • Luminosity function and radial distribution of Milky Way Satellites in a LCDM Universe

    Andrea V. Maccio;Xi Kang;Fabio Fontanot;Rachel S. Somerville

  • Halo expansion in cosmological hydro simulations: towards a baryonic solution of the cusp/core problem in massive spirals

    Andrea V. Maccio;Greg Stinson;Chris B. Brook;James Wadsley

  • NIHAO - XI. Formation of ultra-diffuse galaxies by outflows

    Arianna Di Cintio;Chris B. Brook;Aaron A. Dutton;Andrea V. Macciò;Andrea V. Macciò

Frequent Co-Authors

Avishai Dekel
Avishai Dekel Hebrew University of Jerusalem
James Wadsley
James Wadsley McMaster University
Ben Moore
Ben Moore University of Zurich
Brad K. Gibson
Brad K. Gibson University of Hull
Thomas R. Quinn
Thomas R. Quinn University of Washington
Rachel S. Somerville
Rachel S. Somerville Flatiron Institute
Sergey E. Koposov
Sergey E. Koposov University of Edinburgh
Joachim Stadel
Joachim Stadel University of Zurich
Anatoly Klypin
Anatoly Klypin New Mexico State University
Frank C. van den Bosch
Frank C. van den Bosch Yale University

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