World's Best Scientists 2026 revealed!

D-Index & Metrics

Physics

D-Index
108
Citations
36945
World Ranking
1266
National Ranking
664

Stefano Valenti 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 Stefano Valenti 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: 364 publications — 31st percentile

31% of scientists in this discipline score the same or lower.

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

Stefano Valenti 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 Stefano Valenti 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: 108 D-Index — 67th percentile

67% of scientists in this discipline score the same or lower.

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

Overview

Stefano Valenti is affiliated with the University of California, Davis in the United States. Their research activity is primarily situated within the field of Physics and Astronomy, with a focus on several subfields including Astronomy and Astrophysics, Nuclear and High Energy Physics, Instrumentation, General Health Professions, and Oceanography.

Valenti's work covers numerous topics, notably Gamma-ray bursts and supernovae, Astrophysical Phenomena and Observations, Astrophysics and Cosmic Phenomena, Stellar, planetary, and galactic studies, Pulsars and Gravitational Waves Research, Astro and Planetary Science, and Astronomy and Astrophysical Research.

Among recent publications by Valenti are:

  • Intensive disc-reverberation mapping of Fairall 9: first year of Swift and LCO monitoring, 2020, Monthly Notices of the Royal Astronomical Society
  • Early Spectroscopy and Dense Circumstellar Medium Interaction in SN 2023ixf, 2023, The Astrophysical Journal Letters
  • A Luminous Red Supergiant and Dusty Long-period Variable Progenitor for SN 2023ixf, 2023, The Astrophysical Journal Letters
  • Shock Cooling and Possible Precursor Emission in the Early Light Curve of the Type II SN 2023ixf, 2023, The Astrophysical Journal Letters
  • The Lick AGN Monitoring Project 2016: Velocity-resolved Hβ Lags in Luminous Seyfert Galaxies, 2022, The Astrophysical Journal

Frequent coauthors collaborating with Valenti include:

  • D. A. Howell
  • C. McCully
  • David J. Sand
  • Jennifer E. Andrews
  • Yize Dong

Valenti commonly publishes in these scientific venues:

  • The Astrophysical Journal
  • arXiv (Cornell University)
  • The Astrophysical Journal Letters
  • Monthly Notices of the Royal Astronomical Society
  • UNC Libraries

Best Publications

  • The Man Behind the Curtain: X-rays Drive the UV through NIR Variability in the 2013 AGN Outburst in NGC 2617

    B. J. Shappee;J. L. Prieto;D. Grupe;C. S. Kochanek

  • THE MAN BEHIND THE CURTAIN: X-RAYS DRIVE THE UV THROUGH NIR VARIABILITY IN THE 2013 ACTIVE GALACTIC NUCLEUS OUTBURST IN NGC 2617

    B. J. Shappee;J. L. Prieto;D. Grupe;C. S. Kochanek

  • A gravitational-wave standard siren measurement of the Hubble constant

    B. P. Abbott;R. Abbott;T. D. Abbott;F. Acernese;F. Acernese

  • Optical emission from a kilonova following a gravitational-wave-detected neutron-star merger

    Iair Arcavi;Iair Arcavi;Griffin Hosseinzadeh;Griffin Hosseinzadeh;D. Andrew Howell;D. Andrew Howell;Curtis McCully;Curtis McCully

  • Cosmological Constraints from Measurements of Type Ia Supernovae discovered during the first 1.5 years of the Pan-STARRS1 Survey

    A. Rest;D. Scolnic;R. J. Foley;M. E. Huber

  • Super-luminous Type Ic Supernovae: Catching a Magnetar by the Tail

    C. Inserra;S.J. Smartt;A. Jerkstrand;S. Valenti

  • A giant outburst two years before the core-collapse of a massive star

    A. Pastorello;S. J. Smartt;S. Mattila;J. J. Eldridge

  • Ultra-bright optical transients are linked with type Ic supernovae

    A. Pastorello;S. J. Smartt;M. T. Botticella;K. Maguire

  • Localization and broadband follow-up of the gravitational-wave transient GW150914

    B. P. Abbott;R. Abbott;T. D. Abbott;M. R. Abernathy

  • Localization and broadband follow-up of the gravitational-wave transient GW150914

    B. P. Abbott;R. Abbott;T. D. Abbott;M. R. Abernathy

  • PESSTO : survey description and products from the first data release by the Public ESO Spectroscopic Survey of Transient Objects

    S. J. Smartt;S. Valenti;M. Fraser;C. Inserra

  • Cosmological Constraints from Measurements of Type Ia Supernovae Discovered During the First 1.5 Yr of the Pan-STARRS1 Survey

    Armin Wolfgang Rest;D. Scolnic;R. J. Foley;R. J. Foley;M. E. Huber

  • The broad‐lined Type Ic supernova 2003jd★

    S. Valenti;S. Benetti;E. Cappellaro;F. Patat

  • Confined dense circumstellar material surrounding a regular type II supernova

    O. Yaron;D. A. Perley;D. A. Perley;A. Gal-Yam;J. H. Groh

  • The diversity of Type II supernova versus the similarity in their progenitors

    S. Valenti;D. A. Howell;D. A. Howell;M. D. Stritzinger;M. L. Graham

  • Slowly fading super-luminous supernovae that are not pair-instability explosions

    M. Nicholl;S. J. Smartt;A. Jerkstrand;C. Inserra

  • The Discovery of the Electromagnetic Counterpart of GW170817: Kilonova AT 2017gfo/DLT17ck

    Stefano Valenti;David J. Sand;Sheng Yang;Enrico Cappellaro

  • SN 2005cs in M51 II. Complete Evolution in the Optical and the Near-Infrared

    A. Pastorello;S. Valenti;L. Zampieri;H. Navasardyan

  • The Broad-lined Type Ic SN 2003jd

    S. Valenti;S. Benetti;E. Cappellaro;F. Patat

  • INTERACTING SUPERNOVAE AND SUPERNOVA IMPOSTORS: SN 2009ip, IS THIS THE END?

    A. Pastorello;E. Cappellaro;C. Inserra;S. J. Smartt

Frequent Co-Authors

Paolo A. Mazzali
Paolo A. Mazzali Liverpool John Moores University
Nancy Elias-Rosa
Nancy Elias-Rosa Spanish National Research Council
Andrea Pastorello
Andrea Pastorello National Institute for Astrophysics
Avishay Gal-Yam
Avishay Gal-Yam Weizmann Institute of Science
Stefano Benetti
Stefano Benetti National Institute for Astrophysics
Jesper Sollerman
Jesper Sollerman Stockholm University
Enrico Cappellaro
Enrico Cappellaro National Institute for Astrophysics
Peter Nugent
Peter Nugent Lawrence Berkeley National Laboratory
Mark Sullivan
Mark Sullivan University of Southampton
Maximilian Stritzinger
Maximilian Stritzinger Aarhus University

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