World's Best Scientists 2026 revealed!

D-Index & Metrics

Physics

D-Index
89
Citations
31620
World Ranking
2302
National Ranking
119

Giuseppe Bono 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 Giuseppe Bono 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: 605 publications — 69th percentile

69% of scientists in this discipline score the same or lower.

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

Giuseppe Bono 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 Giuseppe Bono 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: 89 D-Index — 38th percentile

38% of scientists in this discipline score the same or lower.

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

Overview

Giuseppe Bono is affiliated with the University of Rome Tor Vergata in Italy. Their research primarily centers on the field of Physics and Astronomy, with a substantial focus on Astronomy and Astrophysics. Their scholarly output encompasses diverse subfields including Instrumentation, Spectroscopy, Computational Mechanics, and Atomic and Molecular Physics, and Optics.

The main topics of their work include:

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

Giuseppe Bono has published extensively, with significant contributions appearing in notable publication venues. Frequent venues for their work include:

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

Recent papers authored or co-authored by Giuseppe Bono include:

  • "Tracing the Milky Way warp and spiral arms with classical Cepheids," 2022, Astronomy and Astrophysics
  • "Rubin Observatory LSST Transients and Variable Stars Roadmap," 2023, Publications of the Astronomical Society of the Pacific
  • "On the Use of Field RR Lyrae As Galactic Probes: IV. New Insights Into and Around the Oosterhoff Dichotomy," 2021, The Astrophysical Journal
  • "A new and Homogeneous metallicity scale for Galactic classical Cepheids," 2022, Astronomy and Astrophysics
  • "Separation between RR Lyrae and type II Cepheids and their importance for a distance determination: the case of omega Cen," 2020, Astronomy and Astrophysics

Collaboration plays a significant role in their work, with frequent co-authors including:

  • V. F. Braga
  • M. Dall'Ora
  • G. Fiorentino
  • M. Monelli
  • M. Fabrizio

Giuseppe Bono's research contributions address various aspects of star formation, stellar populations, and galactic structure. Their work often involves observational data analysis paired with astrophysical theory and instrumentation techniques. This multidisciplinary approach advances knowledge in the domains of stellar and galactic astronomy.

Best Publications

  • The Gaia mission

    T. Prusti;J. H. J. de Bruijne;A. G. A. Brown

  • Gaia Data Release 1 Summary of the astrometric, photometric, and survey properties

    A. G. A. Brown;A. Vallenari;T. Prusti

  • An eclipsing-binary distance to the Large Magellanic Cloud accurate to two per cent

    G. Pietrzyński;G. Pietrzyński;D. Graczyk;W. Gieren;I. B. Thompson

  • ON A NEW THEORETICAL FRAMEWORK FOR RR LYRAE STARS. I. THE METALLICITY DEPENDENCE

    M. Marconi;G. Coppola;G. Bono;G. Bono;V. Braga;V. Braga

  • The influence of chemical composition on the properties of Cepheid stars. II - The iron content ⋆

    M. Romaniello;F. Primas;M. Mottini;S. Pedicelli

  • Insights into the Cepheid Distance Scale

    G. Bono;G. Bono;F. Caputo;M. Marconi;I. Musella

  • Pulsation and stability of RR Lyrae stars. 1: Instability strip

    G. Bono;R. F. Stellingwerf

  • A pulsational approach to near infrared and visual magnitudes of RR Lyrae stars

    G. Bono;F. Caputo;V. Castellani;M. Marconi

  • CLUSTERING OF LOCAL GROUP DISTANCES: PUBLICATION BIAS OR CORRELATED MEASUREMENTS? I. THE LARGE MAGELLANIC CLOUD

    Richard de Grijs;James E. Wicker;Giuseppe Bono;Giuseppe Bono

  • Relative Frequencies of Blue Stragglers in Galactic Globular Clusters: Constraints for the Formation Mechanisms*

    Giampaolo Piotto;Francesca De Angeli;Ivan R. King;S. G. Djorgovski

  • Classical Cepheid Pulsation Models. X. The Period-Age Relation

    G. Bono;M. Marconi;S. Cassisi;F. Caputo

  • The dynamical mass of a classical Cepheid variable star in an eclipsing binary system

    G. Pietrzyński;I. B. Thompson;W. Gieren;D. Graczyk

  • Nonlinear investigation of the pulsational properties of RR Lyrae variables

    G. Bono;F. Caputo;V. Castellani;M. Marconi

  • Clustering of Local Group distances: publication bias or correlated measurements? III. The Small Magellanic Cloud

    Richard de Grijs;Giuseppe Bono;Giuseppe Bono

  • INTERMEDIATE-MASS STAR MODELS WITH DIFFERENT HELIUM AND METAL CONTENTS

    Giuseppe Bono;Filippina Caputo;Santi Cassisi;Marcella Marconi

  • A pulsational approach to near-infrared and visual magnitudes of RR Lyr stars

    G. Bono;F. Caputo;V. Castellani;M. Marconi

  • Classical Cepheid Pulsation Models. I. Physical Structure

    Giuseppe Bono;Marcella Marconi;Robert F. Stellingwerf

  • Gaia Data Release 1. Open cluster astrometry: performance, limitations, and future prospects

    F. van Leeuwen;A. Vallenari;C. Jordi

  • The distance to the Galactic Centre based on Population-II Cepheids and RR Lyrae stars

    M. A. T. Groenewegen;A. Udalski;G. Bono;G. Bono

  • Direct detection of the close companion of polaris with the hubble space telescope

    Nancy Remage Evans;Gail H. Schaefer;Howard E. Bond;Giuseppe Bono;Giuseppe Bono

Frequent Co-Authors

Marcella Marconi
Marcella Marconi National Institute for Astrophysics
Mario Nonino
Mario Nonino National Institute for Astrophysics
Santi Cassisi
Santi Cassisi National Institute for Astrophysics
Alistair R. Walker
Alistair R. Walker National Optical-Infrared Astronomy Research Lab
Peter B. Stetson
Peter B. Stetson University of Victoria
Grzegorz Pietrzyński
Grzegorz Pietrzyński Polish Academy of Sciences
Antonio Aparicio
Antonio Aparicio University of La Laguna
Wendy L. Freedman
Wendy L. Freedman University of Chicago
Martin A.T. Groenewegen
Martin A.T. Groenewegen Royal Observatory of Belgium
Pauline Barmby
Pauline Barmby University of Western Ontario

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