Michele Ginolfi

Research Assistant Professor

Università degli Studi di Napoli Federico II

Italy

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About

Dr. Michele Ginolfi is a Research Assistant Professor at the Università degli Studi di Firenze, Italy. His research focuses on astro-particle physics, including topics such as star formation in quiescent galaxies, classification of emission-line spectra, and assessing dark matter content in quasar host galaxies. He has also explored the application of machine learning techniques in astrophysical data analysis and galaxy properties inference.

Articles (20)

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2025

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2020

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2020

Collaborators (18)

Francesca RIZZO

Associate professor

University of Bologna

ITALY

Michele Ginolfi

Research Interests

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Articles (20)

Temporarily Quiescent Galaxies at Cosmic Dawn: Probing Bursty Star Formation

Classifying spectra of emission-line regions with neural networks

Assessing the Dark Matter Content of Two Quasar Host Galaxies at z ∼ 6 through Gas Kinematics

Machine learning the gap between real and simulated nebulae

Inferring redshift and galaxy properties via a multi-task neural net with probabilistic outputs

ALMA reveals a dust-obscured galaxy merger at cosmic noon

Evaluating the effectiveness of sonification in science education using Edukoi

Carbon envelopes around merging galaxies at z ∼ 4.5

Metallicity calibrations based on auroral lines from PHANGS–MUSE data

Datacube segmentation via deep spectral clustering

The assembly of dusty galaxies at z ≥ 4: the build-up of stellar mass and its scaling relations with hints from early JWST data

MusE GAs FLOw and Wind (MEGAFLOW) IX. The impact of gas flows on the relations between the mass, star formation rate, and metallicity of galaxies

A solar metallicity galaxy at z &gt; 7? Possible detection of the [N ii] 122 μm and [O iii] 52 μm lines

ALPINE: A Large Survey to Understand Teenage Galaxies

A dusty compact object bridging galaxies and quasars at cosmic dawn

A new look at the infrared properties of z ∼ 5 galaxies

Detection of companion galaxies around hot dust-obscured hyper-luminous galaxy W0410-0913

The alpine-Alma [c ii] survey: Kinematic diversity and rotation in massive star-forming galaxies at z ~ 4.4-5.9

The ALPINE-ALMA [C II] Survey: [C II] 158 μm Emission Line Luminosity Functions at z ∼ 4–6

The ALPINE-ALMA [CII] survey

Collaborators (18)

Francesca RIZZO

Charlotte Mason

Joop Schaye

Vivienne Wild

Martin Wendt

Raffaella Schneider

Andreas Faisst

Massimo Grassi

Johan Richard

Mélanie Chevance

John Silverman

Johannes Zabl

Jonathan Freundlich

Francesco Valentino

Stefania SALVADORI

Marianne Vestergaard

Seiji Fujimoto

Luca Graziani

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A solar metallicity galaxy at z > 7? Possible detection of the [N ii] 122 μm and [O iii] 52 μm lines