M. Nonino

Trieste Astronomical Observatory — Italy

Physics and Astronomy · Physical Sciences

77h-index33.9kcitations567works9.92yr avg
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Research Topics

Astronomy and Astrophysical Research(396), Galaxies: Formation, Evolution, Phenomena(310), Stellar, planetary, and galactic studies(239), Gamma-ray bursts and supernovae(119), Astronomical Observations and Instrumentation(90)

Publications566 total

Galaxy mergers in the epoch of reionization – II. Merger-triggered star formation and AGN activities at <i>z</i> = 4.5−8.5
Monthly Notices of the Royal Astronomical Society·2026· 5 citedOpen Access
Globular Clusters in the Galaxy Cluster MACS0416 at <i>z</i>  = 0.397
The Astronomical Journal·2025Open Access
EPOCHS. III. Unbiased UV Continuum Slopes at 6.5 &lt; <i>z</i> &lt; 13 from Combined PEARLS GTO and Public JWST/NIRCam Imaging
The Astrophysical Journal·2025Open Access
Self-consistent JWST Census of Star Formation and AGN Activity at <i>z</i> = 5.5–13.5
The Astrophysical Journal·2025· 3 citedOpen Access
Multi-object spectroscopic survey of the massive galaxy cluster SMACS J0723.3-7327
Astronomy and Astrophysics·2025Open Access
Galaxy mergers in the epoch of reionization – I. A JWST study of pair fractions, merger rates, and stellar mass accretion rates at <i>z</i>  = 4.5–11.5
Monthly Notices of the Royal Astronomical Society·2025· 29 citedOpen Access
Galaxy populations of protoclusters in cosmological hydrodynamical simulations
Astronomy and Astrophysics·2025· 5 citedOpen Access
EPOCHS. I. The Discovery and Star-forming Properties of Galaxies in the Epoch of Reionization at 6.5 &lt; <i>z</i> &lt; 18 with PEARLS and Public JWST Data
The Astrophysical Journal·2025· 14 citedOpen Access
Self-Consistent JWST Census of Star Formation and AGN activity at z=5.5-13.5
arXiv (Cornell University)·2025Open Access
EPOCHS. IV. SED Modeling Assumptions and Their Impact on the Stellar Mass Function at 6.5 ≤ z ≤ 13.5 Using PEARLS and Public JWST Observations
The Astrophysical Journal·2024· 45 citedOpen Access
CLASH-VLT: Galaxy cluster MACS J0329–0211 and its surroundings using galaxies as kinematic tracers
Astronomy and Astrophysics·2024· 2 citedOpen Access
The Next Step in Galaxy Cluster Strong Lensing: Modeling the Surface Brightness of Multiply Imaged Sources*
The Astrophysical Journal·2024· 6 citedOpen Access
JWST View of Four Infant Galaxies at z = 8.31–8.49 in the MACS J0416.1−2403 Field and Implications for Reionization
The Astrophysical Journal·2024· 10 citedOpen Access
CLASH-VLT: Galaxy cluster MACS J0329-0211 and its surroundings using galaxies as kinematic tracers
arXiv (Cornell University)·2024Open Access
CHEX-MATE: Dynamical masses for a sample of 101 Planck Sunyaev-Zeldovich-selected galaxy clusters
arXiv (Cornell University)·2024Open Access
CHEX-MATE: Dynamical masses for a sample of 101 <i>Planck</i> Sunyaev-Zeldovich-selected galaxy clusters
Astronomy and Astrophysics·2024· 5 citedOpen Access
The next step in galaxy cluster strong lensing: modeling the surface brightness of multiply-imaged sources
arXiv (Cornell University)·2024· 1 citedOpen Access
PSZ2 G282.28+49.94, a recently discovered analogue of the famous Bullet Cluster
arXiv (Cornell University)·2024Open Access
Birds of a Feather: Resolving Stellar Mass Assembly with JWST/NIRCam in a Pair of Kindred z ∼ 2 Dusty Star-forming Galaxies Lensed by the PLCK G165.7+67.0 Cluster
The Astrophysical Journal·2024· 5 citedOpen Access
JWST’s PEARLS: 119 multiply imaged galaxies behind MACS0416, lensing properties of caustic crossing galaxies, and the relation between halo mass and number of globular clusters at <i>z</i> = 0.4
Astronomy and Astrophysics·2024· 15 citedOpen Access
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Frequent Co-authors

P. Rosati(32), Anton M. Koekemoer(20), E. Vanzella(19), Wei Zheng(17), S. Cristiani(15), Leonidas A. Moustakas(14), Tom Broadhurst(14), Mark Dickinson(13), Adi Zitrin(13), P. Tozzi(13), A. Fontana(13), C. Grillo(13), Dan Coe(12), M. Meneghetti(12), Mauro Giavalisco(11), Marc Postman(11), Larry Bradley(11), H. C. Ford(11), Keiichi Umetsu(11), Matthias Bartelmann(10)