World's Best Scientists 2026 revealed!
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Best Female Scientists
2025

D-Index & Metrics

Best Female Scientists

D-Index
125
Citations
59105
World Ranking
438
National Ranking
10

Physics

D-Index
129
Citations
62356
World Ranking
584
National Ranking
22

Lucia Pozzetti 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 Lucia Pozzetti 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: 487 publications — 54th percentile

54% of scientists in this discipline score the same or lower.

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

Lucia Pozzetti 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 Lucia Pozzetti 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: 129 D-Index — 85th percentile

85% of scientists in this discipline score the same or lower.

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

Research.com Recognitions

  • 2025 - Research.com Best Female Scientists Award

Overview

Lucia Pozzetti is affiliated with the National Institute for Astrophysics in Italy. Their research spans the domain of Physics and Astronomy, with a concentration on several subfields including Astronomy and Astrophysics, Instrumentation, Computational Mechanics, Nuclear and High Energy Physics, and Electrical and Electronic Engineering.

The scientist's work addresses a variety of main topics such as Astronomy and Astrophysical Research, Galaxies: Formation, Evolution, Phenomena, Stellar, planetary, and galactic studies, Cosmology and Gravitation Theories, Astronomical Observations and Instrumentation, Gamma-ray bursts and supernovae, and CCD and CMOS Imaging Sensors.

Among recent contributions, notable papers include:

  • Unveiling the Universe with emerging cosmological probes, 2022, CU Scholar (University of Colorado Boulder)
  • The stellar-to-halo mass relation over the past 12 Gyr, 2020, Springer Link (Chiba Institute of Technology)
  • The VANDELS ESO public spectroscopic survey, 2021, Astronomy and Astrophysics
  • Timing the earliest quenching events with a robust sample of massive quiescent galaxies at 2 < z < 5, 2020, Monthly Notices of the Royal Astronomical Society
  • The star formation histories of z ∼ 1 post-starburst galaxies, 2020, Monthly Notices of the Royal Astronomical Society

Frequent collaborators in research include:

  • M. Moresco
  • E. Franceschi
  • M. Castellano
  • C. Carbone
  • V. Capobianco

The most common venues for publication are:

  • Astronomy and Astrophysics (38 publications)
  • arXiv (Cornell University) (24 publications)
  • Monthly Notices of the Royal Astronomical Society (9 publications)
  • University of Groningen research database (University of Groningen / Centre for Information Technology) (2 publications)
  • CU Scholar (University of Colorado Boulder) (1 publication)

Best Publications

  • Mass and environment as drivers of galaxy evolution in SDSS and zCOSMOS and the origin of the Schechter function

    Y. Peng;S. J. Lilly;K. Kovac;M. Bolzonella

  • Mass and environment as drivers of galaxy evolution in SDSS and zCOSMOS and the origin of the Schechter function

    Ying-jie Peng;Simon J. Lilly;Katarina Kovač;Micol Bolzonella

  • Accurate photometric redshifts for the CFHT Legacy Survey calibrated using the VIMOS VLT Deep Survey

    O. Ilbert;S. Arnouts;H.J. McCracken;M. Bolzonella

  • Euclid Definition Study Report

    R. Laureijs;J. Amiaux;S. Arduini;J.-L. Auguères

  • The Star formation history of field galaxies

    Piero Madau;Lucia Pozzetti;Mark Dickinson;Mark Dickinson

  • Accurate photometric redshifts for the CFHT legacy survey calibrated using the VIMOS VLT deep survey

    O. Ilbert;O. Ilbert;S. Arnouts;H. J. Mccracken;M. Bolzonella

  • zCOSMOS: A Large VLT/VIMOS redshift survey covering 0 < z < 3 in the COSMOS field

    S.J. Lilly;O. Le Fevre;A. Renzini;G. Zamorani

  • zCOSMOS: A Large VLT/VIMOS Redshift Survey Covering 0 < z < 3 in the COSMOS Field*

    S. J. Lilly;O. Le Fèvre;A. Renzini;G. Zamorani

  • The VIMOS VLT Deep Survey - First epoch VVDS-Deep survey: 11564 spectra with 17.5<=IAB<=24, and the redshift distribution over 0< z <=5

    O. Le Fevre;G. Vettolani;B. Garilli;L. Tresse

  • A 6% measurement of the Hubble parameter at z∼0.45: direct evidence of the epoch of cosmic re-acceleration

    Michele Moresco;Michele Moresco;Lucia Pozzetti;Andrea Cimatti;Raul Jimenez

  • 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

  • GMASS Ultradeep Spectroscopy of Galaxies at 1.4<z<2. II. Superdense passive galaxies: how did they form and evolve ?

    A. Cimatti;P. Cassata;L. Pozzetti;J. Kurk

  • A test of the nature of cosmic acceleration using galaxy redshift distortions

    L. Guzzo;M. Pierleoni;B. Meneux;E. Branchini

  • A 6% measurement of the Hubble parameter at $z\sim0.45$: direct evidence of the epoch of cosmic re-acceleration

    Michele Moresco;Lucia Pozzetti;Andrea Cimatti;Raul Jimenez

  • The zCOSMOS 10k-Bright Spectroscopic Sample

    Simon J. Lilly;Vincent Le Brun;Christian Maier;Vincenzo Mainieri

  • The VIMOS VLT deep survey. First epoch VVDS-deep survey: 11 564 spectra with 17.5 ≤ IAB ≤ 24, and the redshift distribution over 0 ≤ z ≤ 5

    O. Le Fèvre;G. Vettolani;B. Garilli;L. Tresse

  • GMASS ultradeep spectroscopy of galaxies at $z$ ~ 2 - II. Superdense passive galaxies: how did they form and evolve?

    A. Cimatti;P. Cassata;L. Pozzetti;J. Kurk

  • zCOSMOS - 10k-bright spectroscopic sample. The bimodality in the Galaxy Stellar Mass Function: exploring its evolution with redshift

    L. Pozzetti;M. Bolzonella;E. Zucca;G. Zamorani

  • Improved constraints on the expansion rate of the Universe up to z ∼ 1.1 from the spectroscopic evolution of cosmic chronometers

    M. Moresco;A. Cimatti;R. Jimenez;L. Pozzetti

  • The K20 survey - I. Disentangling old and dusty star-forming galaxies in the ERO population

    A. Cimatti;E. Daddi;M. Mignoli;L. Pozzetti

Frequent Co-Authors

S. Bardelli
S. Bardelli National Institute for Astrophysics
H. J. McCracken
H. J. McCracken Institut d'Astrophysique de Paris
A. Iovino
A. Iovino National Institute for Astrophysics
A. Cappi
A. Cappi National Institute for Astrophysics
Elena Zucca
Elena Zucca National Institute for Astrophysics
Alvio Renzini
Alvio Renzini National Institute for Astrophysics
G. Zamorani
G. Zamorani National Institute for Astrophysics
Andrea Cimatti
Andrea Cimatti University of Bologna
D. Maccagni
D. Maccagni National Institute for Astrophysics
Luigi Guzzo
Luigi Guzzo University of Milan

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