World's Best Scientists 2026 revealed!
Sandra Savaglio

Sandra Savaglio

D-Index & Metrics

Physics

D-Index
74
Citations
16641
World Ranking
3486
National Ranking
188

Sandra Savaglio 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 Sandra Savaglio 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: 279 publications — 14th percentile

14% of scientists in this discipline score the same or lower.

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

Sandra Savaglio 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 Sandra Savaglio 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: 74 D-Index — 7th percentile

7% of scientists in this discipline score the same or lower.

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

Overview

Sandra Savaglio is affiliated with the University of Calabria in Italy and works primarily in the field of Physics and Astronomy, with a focus on Astronomy and Astrophysics. Their research encompasses several subfields including Nuclear and High Energy Physics, Instrumentation, Computational Mechanics, and Oceanography.

Their main research topics cover various areas related to celestial phenomena and astrophysical processes, including:

  • Gamma-ray bursts and supernovae
  • Astrophysical Phenomena and Observations
  • Stellar, planetary, and galactic studies
  • Astrophysics and Cosmic Phenomena
  • Pulsars and Gravitational Waves Research
  • Astronomy and Astrophysical Research
  • Astronomical Observations and Instrumentation

Savaglio's publication record includes contributions to a range of scientific journals, with frequent appearances in Astronomy and Astrophysics, where they have published seven times. Other venues include arXiv (Cornell University), Monthly Notices of the Royal Astronomical Society, The Astrophysical Journal, and Nature.

Notable recent papers by Sandra Savaglio include:

  • The Peculiar Short-duration GRB 200826A and Its Supernova, 2022, The Astrophysical Journal
  • A nebular origin for the persistent radio emission of fast radio bursts, 2024, Nature
  • Dissecting the interstellar medium of a z= 6.3 galaxy, 2022, Astronomy and Astrophysics
  • The supernova of the MAGIC gamma-ray burst GRB 190114C, 2021, Astronomy and Astrophysics
  • 2021 research published in Research Portal (King's College London)

The scientist collaborates frequently with a number of coauthors, including:

  • A. Rossi
  • M. de Pasquale
  • D. H. Hartmann
  • P. Jakobsson
  • G. Pugliese

Best Publications

  • The Gemini Deep Deep Survey. VII. The Redshift Evolution of the Mass-Metallicity Relation* **

    S. Savaglio;K. Glazebrook;D. Le Borgne;S. Juneau

  • THE GALAXY POPULATION HOSTING GAMMA-RAY BURSTS

    S. Savaglio;Karl Glazebrook;D. Le Borgne

  • Cosmic Star Formation History and its Dependence on Galaxy Stellar Mass

    S. Juneau;K. Glazebrook;D. Crampton;P. J. McCarthy

  • Cosmic Star Formation History and Its Dependence on Galaxy Stellar Mass

    Stéphanie Juneau;Stéphanie Juneau;Karl Glazebrook;David Crampton;Patrick J. McCarthy

  • A high abundance of massive galaxies 3–6 billion years after the Big Bang

    Karl Glazebrook;Roberto G. Abraham;Patrick J. McCarthy;Sandra Savaglio

  • RED NUGGETS AT z ∼ 1.5: COMPACT PASSIVE GALAXIES AND THE FORMATION OF THE KORMENDY RELATION

    Ivana Damjanov;Patrick J. McCarthy;Roberto G. Abraham;Karl Glazebrook

  • The Gemini Deep Deep Survey. I. Introduction to the Survey, Catalogs, and Composite Spectra

    Roberto G. Abraham;Karl Glazebrook;Patrick J. McCarthy;David Crampton

  • GRB 080913 at redshift 6.7

    J. Greiner;T. Kruehler;J. P. U. Fynbo;A. Rossi

  • A very luminous magnetar-powered supernova associated with an ultra-long γ-ray burst

    Jochen Greiner;Paolo A. Mazzali;D. Alexander Kann;Thomas Krühler

  • GRB 080913 AT REDSHIFT 6.7

    J. Greiner;T. Krühler;J. P. U. Fynbo;A. Rossi

  • GRB hosts through cosmic time - VLT/X-Shooter emission-line spectroscopy of 96 GRB-selected galaxies at 0.1 < z < 3.6

    T. Krühler;D. Malesani;J. P. U. Fynbo;O. E. Hartoog

  • The 2175 A dust feature in a Gamma Ray Burst afterglow at redshift 2.45

    T. Krühler;A. Küpcü Yoldaş;J. Greiner;C. Clemens

  • The 2175 Å Dust Feature in a Gamma-Ray Burst Afterglow at Redshift 2.45

    T. Krühler;A. Küpcü Yoldaş;J. Greiner;C. Clemens

  • The SEDs and Host Galaxies of the dustiest GRB afterglows

    T. Krühler;J. Greiner;P. Schady;S. Savaglio

  • Rapid-Response Mode VLT/UVES spectroscopy of GRB060418: Conclusive evidence for UV pumping from the time evolution of FeII and NiII excited- and metastable-level populations

    P.M. Vreeswijk;C. Ledoux;A. Smette;S.L. Ellison

  • Evolved Galaxies at z > 1.5 from the Gemini Deep Deep Survey: The Formation Epoch of Massive Stellar Systems

    Patrick J. McCarthy;Damien Le Borgne;David Crampton;Hsiao-Wen Chen

  • GRBs as cosmological probes—cosmic chemical evolution

    Sandra Savaglio

  • The SEDs and host galaxies of the dustiest GRB afterglows

    T. Krühler;J. Greiner;P. Schady;S. Savaglio

  • Rapid-response mode VLT/UVES spectroscopy of GRB 060418. Conclusive evidence for UV pumping from the time evolution of Fe II and Ni II excited- and metastable-level populations

    Paul M. Vreeswijk;C. Ledoux;A. Smette;S. Ellison

  • Heavy Element Abundances and Dust Depletions in the Host Galaxies of Three Gamma-Ray Bursts

    S. Savaglio;S. M. Fall;F. Fiore

Frequent Co-Authors

Jochen Greiner
Jochen Greiner Max Planck Society
Patricia Schady
Patricia Schady University of Bath
Eliana Palazzi
Eliana Palazzi National Institute for Astrophysics
Elena Pian
Elena Pian National Institute for Astrophysics
Karl Glazebrook
Karl Glazebrook Swinburne University of Technology
Thomas Krühler
Thomas Krühler Max Planck Society
Hongzheng Chen
Hongzheng Chen Zhejiang University
Roberto Abraham
Roberto Abraham University of Toronto
Stefano Covino
Stefano Covino National Institute for Astrophysics
Raymond G. Carlberg
Raymond G. Carlberg University of Toronto

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