World's Best Scientists 2026 revealed!
Cristiano Porciani

Cristiano Porciani

D-Index & Metrics

Physics

D-Index
79
Citations
31763
World Ranking
3065
National Ranking
292

Cristiano Porciani 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 Cristiano Porciani 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: 220 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.

Cristiano Porciani 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 Cristiano Porciani 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: 79 D-Index — 17th percentile

17% of scientists in this discipline score the same or lower.

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

Overview

Cristiano Porciani is affiliated with the University of Bonn in Germany. Their research work primarily spans the fields of Physics and Astronomy, with a strong focus on Astronomy and Astrophysics as a subfield.

Their publication record includes contributions to various topics within their field of study, notably:

  • Galaxies: Formation, Evolution, Phenomena
  • Astronomy and Astrophysical Research
  • Cosmology and Gravitation Theories
  • Stellar, planetary, and galactic studies
  • Scientific Research and Discoveries
  • Astrophysics and Star Formation Studies
  • Radio Astronomy Observations and Technology

Porciani's recent papers illustrate a focus on cosmological parameters, galaxy power spectrum, bispectrum analysis, and large-scale structure in the universe. Notable works include:

  • "Cosmological parameters from the likelihood analysis of the galaxy power spectrum and bispectrum in real space" (2021), published in ArTS Archivio della ricerca di Trieste (University of Trieste)
  • "The halo bispectrum multipoles in redshift space" (2023), published in Journal of Cosmology and Astroparticle Physics
  • "The reach of next-to-leading-order perturbation theory for the matter bispectrum" (2021), published on arXiv (Cornell University)
  • "The large-scale monopole of the power spectrum in a Euclid-like survey: Wide-angle effects, lensing, and the 'finger of the observer'" (2022), published in Padua Research Archive (University of Padua)
  • "The H i-halo mass relation at redshift z ∼ 1 from the Minkowski functionals of 21-cm intensity maps" (2021), published in Monthly Notices of the Royal Astronomical Society

The scientist collaborates frequently with several colleagues in their field. Among the most frequent co-authors are:

  • E. Sefusatti
  • Andrea Oddo
  • Alexander Eggemeier
  • D. Alkhanishvili
  • Emilio Romano-Díaz

Porciani's work is published predominantly in well-known venues, reflecting their active contribution to academic discourse. Frequent publication venues include:

  • Journal of Cosmology and Astroparticle Physics
  • arXiv (Cornell University)
  • Monthly Notices of the Royal Astronomical Society
  • Astronomy and Astrophysics
  • ArTS Archivio della ricerca di Trieste (University of Trieste)

The scientist's research incorporates aspects of statistical and nonlinear physics, instrumentation, nuclear and high energy physics, and signal processing, supporting interdisciplinary approaches within their core astronomical research.

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

  • Cosmology and Fundamental Physics with the Euclid Satellite

    Luca Amendola;Stephen Appleby;Anastasios Avgoustidis;David Bacon

  • Cosmology and fundamental physics with the Euclid satellite

    Luca Amendola;Stephen Appleby;David Bacon;Tessa Baker

  • 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 First Release COSMOS Optical and Near-IR Data and Catalog

    P. Capak;H. Aussel;M. Ajiki;H. J. McCracken

  • A Universal Angular Momentum Profile for Galactic Halos

    James S. Bullock;Avishai Dekel;Tsafrir S. Kolatt;Andrey V. Kravtsov

  • The First Release COSMOS Optical and Near-IR Data and Catalog

    P. Capak;H. Aussel;H. Aussel;M. Ajiki;H. J. McCracken;H. J. McCracken

  • The zCOSMOS 10k-Bright Spectroscopic Sample

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

  • 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

  • Properties of dark matter haloes in clusters, filaments, sheets and voids

    Oliver Hahn;Cristiano Porciani;C. Marcella Carollo;Avishai Dekel

  • 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

  • On the Association of Gamma-Ray Bursts with Massive Stars: Implications for Number Counts and Lensing Statistics

    Cristiano Porciani;Cristiano Porciani;Piero Madau;Piero Madau

  • Ongoing and co-evolving star formation in zCOSMOS galaxies hosting Active Galactic Nuclei

    J. D. Silverman;F. Lamareille;C. Maier;S. Lilly

  • COSMOS Morphological Classification with the Zurich Estimator of Structural Types (ZEST) and the Evolution Since z = 1 of the Luminosity Function of Early, Disk, and Irregular Galaxies*

    C. Scarlata;C. M. Carollo;S. Lilly;M. T. Sargent

  • The Zurich Extragalactic Bayesian Redshift Analyzer (ZEBRA) and its first application: COSMOS

    R. Feldmann;C. M. Carollo;C. Porciani;S. J. Lilly

  • The Zurich Extragalactic Bayesian Redshift Analyzer and its first application: COSMOS

    R. Feldmann;C. M. Carollo;C. Porciani;S. J. Lilly

  • The evolution of dark matter halo properties in clusters, filaments, sheets and voids

    Oliver Hahn;C. Marcella Carollo;Cristiano Porciani;Avishai Dekel

  • Cosmology and Fundamental Physics with the Euclid Satellite

    L Amendola;S Appleby;A Avgoustidis;D Bacon

Frequent Co-Authors

H. J. McCracken
H. J. McCracken Institut d'Astrophysique de Paris
Alvio Renzini
Alvio Renzini National Institute for Astrophysics
A. Cappi
A. Cappi National Institute for Astrophysics
S. Bardelli
S. Bardelli National Institute for Astrophysics
A. Iovino
A. Iovino National Institute for Astrophysics
Christian Marinoni
Christian Marinoni Aix-Marseille University
Lucia Pozzetti
Lucia Pozzetti National Institute for Astrophysics
Anton M. Koekemoer
Anton M. Koekemoer Space Telescope Science Institute
D. Maccagni
D. Maccagni National Institute for Astrophysics
Luigi Guzzo
Luigi Guzzo University of Milan

If you think any of the details on this page are incorrect, let us know.

Report an issue

We appreciate your kind effort to assist us to improve this page, it would be helpful providing us with as much detail as possible in the text box below:

Best Scientists Citing Cristiano Porciani

Trending Scientists

Recently Published Articles