F. Pozzi

Osservatorio astronomico di Bologna — Italy

Physics and Astronomy · Physical Sciences

54h-index12.8kcitations265works4.82yr avg
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Research Topics

Galaxies: Formation, Evolution, Phenomena(166), Astronomy and Astrophysical Research(129), Astrophysics and Star Formation Studies(60), Gamma-ray bursts and supernovae(58), Astrophysical Phenomena and Observations(49)

Publications265 total

Infrared emission from <i>z</i> ∼ 6.5 quasar host galaxies: a direct estimate of dust physical properties
Astronomy and Astrophysics·2025Open Access
Active galactic nuclei-heated dust revealed in “little red dots”
Astronomy and Astrophysics·2025· 2 citedOpen Access
Tracing AGN-Galaxy Co-Evolution with UV Line-Selected Obscured AGN
ArXiv.org·2025Open Access
The ALPINE-CRISTAL-JWST Survey: The Fast Metal Enrichment of Massive Galaxies at z~5
arXiv (Cornell University)·2025Open Access
The ALPINE-CRISTAL-JWST survey: Spatially resolved star formation relations at <i>z</i> ∼ 5
Astronomy and Astrophysics·2025Open Access
The ALPINE-CRISTAL-JWST survey: spatially resolved star formation relations at $z\sim5$
arXiv (Cornell University)·2025Open Access
Spatially resolved [CII]–gas conversion factor in early galaxies
Astronomy and Astrophysics·2025· 5 citedOpen Access
Need for PRIMA to understand the nature and ISM physical conditions of HST-dark galaxies
Journal of Astronomical Telescopes Instruments and Systems·2025Open Access
Gas properties as a function of environment in the proto-supercluster Hyperion at <i>z</i> ∼ 2.45
Astronomy and Astrophysics·2025· 5 citedOpen Access
Going deeper into the dark with COSMOS-Web
Astronomy and Astrophysics·2025· 1 citedOpen Access
A hidden active galactic nucleus powering bright [O III] nebulae in a protocluster at <i>z</i> = 4.5 revealed by JWST
Astronomy and Astrophysics·2024· 19 citedOpen Access
A hidden active galactic nucleus powering bright [O III] nebulae in a protocluster at $z=4.5$ revealed by JWST
arXiv (Cornell University)·2024Open Access
Dark progenitors and massive descendants: A first ALMA perspective of radio-selected near-IR-dark galaxies in the COSMOS field
Astronomy and Astrophysics·2024· 7 citedOpen Access
The ALPINE-ALMA [CII] survey: Dust emission effective radius up to 3 kpc in the early Universe
Astronomy and Astrophysics·2024· 10 citedOpen Access
ALMA-ALPINE [CII] survey: The sub-kpc morphology of three main sequence galaxy systems at <i>z</i> ∼ 4.5 revealed by ALMA
Astronomy and Astrophysics·2024· 12 citedOpen Access
AGN feedback in the Local Universe: multiphase outflow of the Seyfert galaxy NGC 5506
arXiv (Cornell University)·2024Open Access
COSMOS2020: Investigating the AGN-obscured accretion phase at <i>z</i> ∼ 1 via [Ne V] selection
Astronomy and Astrophysics·2024· 7 citedOpen Access
AGN feedback in the Local Universe: Multiphase outflow of the Seyfert galaxy NGC 5506
Astronomy and Astrophysics·2024· 13 citedOpen Access
Dark progenitors and massive descendants: A first ALMA perspective on Radio-Selected NIRdark galaxies in the COSMOS field
arXiv (Cornell University)·2024Open Access
Illuminating the Dark Side of Cosmic Star Formation. III. Building the Largest Homogeneous Sample of Radio-selected Dusty Star-forming Galaxies in COSMOS with PhoEBO
The Astrophysical Journal·2024· 15 citedOpen Access
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Frequent Co-authors

D. Lutz(27), C. Gruppioni(27), Laura Bisigello(26), S. Berta(26), B. Magnelli(25), R. Maiolino(23), A. Cimatti(21), P. Popesso(21), E. Le Floc’h(21), R. Nordon(19), G. Zamorani(19), E. Daddi(18), P. Andreani(18), P. Santini(18), R. Genzel(17), I Tereno(16), L. Riguccini(16), L. J. Tacconi(16), A. Poglitsch(15), I. Valtchanov(15)