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D-Index & Metrics

Physics

D-Index
105
Citations
41209
World Ranking
1392
National Ranking
73

Paolo Tozzi 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 Paolo Tozzi 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: 449 publications — 47th percentile

47% of scientists in this discipline score the same or lower.

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

Paolo Tozzi 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 Paolo Tozzi 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: 105 D-Index — 63rd percentile

63% of scientists in this discipline score the same or lower.

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

Overview

Paolo Tozzi is affiliated with the National Institute for Astrophysics in Italy. Their research primarily falls within the field of Physics and Astronomy, with a specialized focus on Astronomy and Astrophysics.

Tozzi's work covers multiple subfields, including:

  • Astronomy and Astrophysics
  • Instrumentation
  • Nuclear and High Energy Physics
  • Atomic and Molecular Physics, and Optics
  • Pulmonary and Respiratory Medicine

Their main research topics encompass:

  • Galaxies: Formation, Evolution, Phenomena
  • Astrophysical Phenomena and Observations
  • Astronomy and Astrophysical Research
  • Gamma-ray bursts and supernovae
  • Stellar, planetary, and galactic studies
  • Astrophysics and Cosmic Phenomena
  • Adaptive optics and wavefront sensing

Some of Paolo Tozzi's recent significant publications include:

  • The Cluster HEritage project with XMM-Newton: Mass Assembly and Thermodynamics at the Endpoint of structure formation, 2021, Astronomy and Astrophysics
  • High star cluster formation efficiency in the strongly lensed Sunburst Lyman-continuum galaxy at z = 2.37, 2021, Astronomy and Astrophysics
  • The MUSE Deep Lensed Field on the Hubble Frontier Field MACS J0416, 2020, Astronomy and Astrophysics
  • Galaxy-scale ionised winds driven by ultra-fast outflows in two nearby quasars, 2020, Astronomy and Astrophysics
  • Candidate Population III stellar complex at z = 6.629 in the MUSE Deep Lensed Field, 2020, Monthly Notices of the Royal Astronomical Society Letters

Frequent co-authors who have collaborated extensively with Paolo Tozzi include:

  • R. Gilli
  • Fabio Vito
  • P. Rosati
  • C. Vignali
  • A. Comastri

The scientist's findings have been published predominantly in the following venues:

  • Astronomy and Astrophysics
  • arXiv (Cornell University)
  • The Astrophysical Journal
  • Springer Link (Chiba Institute of Technology)
  • SSRN Electronic Journal

Best Publications

  • Dark Matter Substructure in Galactic Halos

    Ben Moore;Sebastiano Ghigna;Fabio Governato;George Lake

  • Dark Matter Substructure within Galactic Halos

    Ben Moore;Sebastiano Ghigna;Fabio Governato;George Lake

  • A New Photometric Technique for the Joint Selection of Star-forming and Passive Galaxies at 1.4 <~ z <~ 2.5

    E. Daddi;Andrea Cimatti;A. Renzini;A. Fontana

  • The Chandra Deep Field South: the 1 Million Second

    P. Rosati;P. Tozzi;R. Giacconi;R. Gilli

  • Chandra Deep Field South: The 1 Ms Catalog

    Riccardo Giacconi;Riccardo Giacconi;Andrew Zirm;JunXian Wang;Piero Rosati

  • The Chandra Deep Field-South: Optical Spectroscopy. I.*

    G. P. Szokoly;J. Bergeron;G. Hasinger;I. Lehmann

  • First Results from the X-Ray and Optical Survey of the Chandra Deep Field South

    R. Giacconi;R. Giacconi;P. Rosati;P. Tozzi;M. Nonino

  • THE CHANDRA DEEP FIELD-SOUTH SURVEY: 4 Ms SOURCE CATALOGS

    Yongquan Xue;Bin Luo;William Nielsen Brandt;Franz E. Bauer;Franz E. Bauer

  • The Evolution of X-ray Clusters and the Entropy of the Intra Cluster Medium

    Paolo Tozzi;Colin Norman

  • X-ray spectral properties of AGN in the Chandra Deep Field South

    P. Tozzi;R. Gilli;V. Mainieri;C. Norman

  • The Evolution of X-Ray Clusters and the Entropy of the Intracluster Medium

    Paolo Tozzi;Colin Norman

  • X-ray spectral properties of active galactic nuclei in the Chandra deep field south

    P. Tozzi;R. Gilli;V. Mainieri;C. Norman;C. Norman

  • X‐ray properties of galaxy clusters and groups from a cosmological hydrodynamical simulation

    Stefano Borgani;G. Murante;V. Springel;A. Diaferio

  • THE CHANDRA DEEP FIELD-SOUTH SURVEY: 7 MS SOURCE CATALOGS

    Bin Luo;William Nielsen Brandt;Yongquan Xue;Bret Lehmer

  • The Chandra Deep Field-South: The 1 Million Second Exposure*

    P. Rosati;P. Tozzi;R. Giacconi;R. Giacconi;R. Gilli

  • The Assembly History of Field Spheroidals: Evolution of Mass-to-light Ratios and Signatures of Recent Star Formation

    T. Treu;R. S. Ellis;T. X. Liao;P. G. van Dokkum

  • Measuring Ωm with the ROSAT Deep Cluster Survey

    Stefano Borgani;Piero Rosati;Paolo Tozzi;S. A. Stanford;S. A. Stanford

  • Measuring $\Omega_m$ with the ROSAT Deep Cluster Survey

    S. Borgani;P. Rosati;P. Tozzi;S.A. Stanford

  • The Chandra Deep Field-South Survey: 2 Ms Source Catalogs

    Bin Luo;Franz E. Bauer;William Nielsen Brandt;David M. Alexander

  • The extended Chandra deep field-south survey: Chandra point-source catalogs

    B. D. Lehmer;W. N. Brandt;D. M. Alexander;F. E. Bauer

Frequent Co-Authors

Stefano Borgani
Stefano Borgani University of Trieste
Colin Norman
Colin Norman Space Telescope Science Institute
Roberto Gilli
Roberto Gilli National Institute for Astrophysics
Mario Nonino
Mario Nonino National Institute for Astrophysics
Vincenzo Mainieri
Vincenzo Mainieri European Southern Observatory
Stefano Ettori
Stefano Ettori National Institute for Astrophysics
Franz E. Bauer
Franz E. Bauer Pontificia Universidad Católica de Chile
Anton M. Koekemoer
Anton M. Koekemoer Space Telescope Science Institute
Andrea Comastri
Andrea Comastri National Institute for Astrophysics
Cristian Vignali
Cristian Vignali University of Bologna

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