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 Piero Rosati sits on this spectrum.
This scientist: 491 publications — 55th percentile
55% of scientists in this discipline score the same or lower.
The last bar groups every scientist with 1,469 publications or more.
The chart shows the D-index (discipline H-index) distribution of Physics scientists ranked by Research.com in 2026. The highlighted bar marks where Piero Rosati sits on this spectrum.
This scientist: 139 D-Index — 89th percentile
89% of scientists in this discipline score the same or lower.
The last bar groups every scientist with 185 D-Index or more.
Piero Rosati is affiliated with the University of Ferrara in Italy. Their research contributions are primarily situated within the field of Physics and Astronomy, with a focus on subfields such as Astronomy and Astrophysics, Instrumentation, Nuclear and High Energy Physics, Atomic and Molecular Physics and Optics, and Radiation.
Their work covers main topics including Galaxies: Formation, Evolution, Phenomena; Astronomy and Astrophysical Research; Gamma-ray bursts and supernovae; Stellar, planetary, and galactic studies; Adaptive optics and wavefront sensing; Astrophysical Phenomena and Observations; and Astrophysics and Star Formation Studies.
Rosati has published extensively, with frequent appearances in several notable scientific venues. The primary publication venues include:
The most recent papers associated with Rosati reflect active engagement in observational cosmology and astrophysics. These include:
Frequent co-authorship patterns indicate collaboration with several researchers, including:
Rosati's scientific contributions indicate a consistent focus on studying galaxies, cosmic structure formation, and phenomena observed through advanced astronomical instrumentation and methods. Their work combines observational data from space telescopes, such as the James Webb Space Telescope, with cosmological modeling and analysis.
Anton M. Koekemoer;S. M. Faber;Henry C. Ferguson;Norman A. Grogin
M. Giavalisco
Norman A. Grogin;Dale D. Kocevski;S. M. Faber;Henry C. Ferguson
M. Giavalisco;H. C. Ferguson;H. C. Ferguson;A. M. Koekemoer;M. Dickinson;M. Dickinson
N. Suzuki;N. Suzuki;D. Rubin;D. Rubin;C. Lidman;G. Aldering
Anton M. Koekemoer;S. M. Faber;Henry C. Ferguson;Norman A. Grogin
Marc Postman;Dan Coe;Narciso Benítez;Larry Bradley
Riccardo Giacconi;Riccardo Giacconi;Andrew Zirm;JunXian Wang;Piero Rosati
H. Boehringer;W. Voges;J. P. Huchra;B. McLean
G. P. Szokoly;J. Bergeron;G. Hasinger;I. Lehmann
R. Giacconi;R. Giacconi;P. Rosati;P. Tozzi;M. Nonino
Yongquan Xue;Bin Luo;William Nielsen Brandt;Franz E. Bauer;Franz E. Bauer
H. Böhringer;W. Voges;J. P. Huchra;B. McLean
Piero Rosati;Stefano Borgani;Colin Norman
A. Cimatti;P. Cassata;L. Pozzetti;J. Kurk
M. Moresco;A. Cimatti;R. Jimenez;L. Pozzetti
Piero Rosati;Roberto Della Ceca;Colin Norman;Riccardo Giacconi
M. Postman;M. Franx;N. Cross;B. Holden
P. Rosati;R. Della Ceca;C. Norman;R. Giacconi
P. Tozzi;R. Gilli;V. Mainieri;C. Norman;C. Norman
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