Launch week offerEnds in00h00m00s

annual Promonthly Pro

Michele Fumagalli

Has grant

Professor

University of Milano-Bicocca

Italy

Research Interests

ApplyKite TwinLearns as you apply

Make your next move.

Prepare your application

Review drafts before you send them.

Explore related searches

Professors in Italy Professors in Astronomy Astronomy professors in Italy

About

Professor Michele Fumagalli is a faculty member at Universita degli Studi di Milano-Bicocca, Italy. His research focuses on astrophysics, particularly the study of star clusters, dwarf galaxies, and the intergalactic medium. Recent articles authored by Professor Fumagalli delve into synthetic photometry, the evolution of metal-enriched gas, and the relationship between gas and galaxies in various cosmic environments.

Recent Grants

Grant: Close

Astronomy at Durham 2020-2023

Open Date: 2020-03-31

Close Date: 2024-03-31

Grant: Close

PATT Linked Grant for the Durham Astrophysics Group 2019-20

Open Date: 2019-01-01

Close Date: 2020-09-29

Grant: Close

Probing an uncharted portion of the distant Universe with the MUSE Ultra Deep Field

Open Date: 2018-06-01

Close Date: 2023-05-01

Grant: Close

A new vantage point on how gas flows regulate the build-up of galaxies in the early universe

Open Date: 2018-02-01

Close Date: 2023-01-31

Grant: Close

Durham Astronomy Consolidated Grant 2017-2020

Open Date: 2017-03-31

Close Date: 2020-03-30

Articles (25)

Year:

2026

Year:

2025

Year:

2025

Year:

2025

Year:

2025

Year:

2025

Year:

2025

Year:

2025

Year:

2025

Year:

2025

Year:

2025

Year:

2025

Year:

2025

Year:

2025

Year:

2025

Year:

2021

Year:

2021

Year:

2021

Year:

2021

Year:

2021

Year:

2021

Year:

2021

Year:

2021

Year:

2021

Year:

2021

Collaborators (93)

John Stott

University of Lancaster

UNITED KINGDOM

Michele Fumagalli

Research Interests

Make your next move.

Explore related searches

About

Recent Grants

Articles (25)

The MUSE Ultra Deep Field (MUDF): VIII. The cool gas distribution surrounding galaxies at redshifts z ≍ 0.5─2

Euclid. I. Overview of the Euclid mission

The MUSE Ultra Deep Field: A 5 Mpc Stretch of the z ≈ 4 Cosmic Web Revealed in Emission

Automated quasar continuum estimation using neural networks

The MUSE Ultra Deep Field (MUDF)

CLUES. III. Do User Choices Impact the Results of SED Fitting? Tests of “Off-the-shelf” Stellar Population and Dust Extinction Models in the CLUES Sample

X-ray view of a massive node of the Cosmic Web at z ∼ 3

A giant disk galaxy two billion years after the Big Bang

Bayesian luminosity function estimation in multi-depth datasets with selection effects: A case study for 3 &lt; z &lt; 5 Lyman α emitters

Modelling Mg II resonance doublet spectra from star-forming galaxies at z ∼ 1

Connecting the growth of galaxies to the large-scale environment in a massive node of the Cosmic Web at z ∼ 3

High-definition imaging of a filamentary connection between a close quasar pair at z = 3

The Qz5 Survey. I. How the H I Mass Density of the Universe Evolves with Cosmic Time

Baryonic Ecosystem IN Galaxies (BEINGMgII): I. Host galaxies of ultra-strong Mg II absorbers in the Subaru Hyper Suprime-Cam Survey

Baryonic Ecosystem IN Galaxies (BEINGMgII): II. Unveiling the nature of galaxies harbouring cool gas reservoirs

The dependence of the hierarchical distribution of star clusters on galactic environment

Synthetic photometry of OB star clusters with stochastically sampled IMFs: analysis of models and HST observations

The Tail of Late-forming Dwarf Galaxies in ΛCDM

Metal-enriched halo gas across galaxy overdensities over the last 10 billion years

Probing the physical properties of the intergalactic medium using blazars

The relationship between gas and galaxies at z &lt; 1 using the Q0107 quasar triplet

Studying the ISM at ∼10 pc scale in NGC 7793 with MUSE

MUSE analysis of gas around galaxies (MAGG) – III. The gas and galaxy environment of z = 3–4.5 quasars

Probing the physical properties of the intergalactic medium using gamma-ray bursts

Sub-damped Lyman α systems in the XQ-100 survey – II. Chemical evolution at 2.4 ≤ z ≤ 4.3

Collaborators (93)

John Stott

Mitchell Revalski

Graham Smith

Max Gronke

Carlton Baugh

Victoria Yankelevich

Sebastien Clesse

Ian Smail

Nelson Nunes

Matteo Calabrese

Ben Dryer

Javier Graciá Carpio

Mikael Granvik

Azadeh Moradinezhad Dizgah

Davide Gerosa

C J A P Martins

Rafael Rebolo

Sotiria Fotopoulou

Isobel Hook

Alejandro Benítez-Llambay

Sergio Di Domizio

Luigi Pilo

Alexandre Refregier

Jorge Carretero

Fabio La Franca

Jussi Valiviita

Nestor Sanchez

Matteo Fossati

Hannu Kurki-Suonio

Ken Osato

chiara mancini

Jacobo Asorey

Santiago Avila

Andrei Lazanu

Jon Loveday

Kimmo Kiiveri

Mike Hudson

Benedict Bahr-Kalus

Mikko Pöntinen

Elizabeth Gonzalez

Frederic Courbin

Lucia F. de la Bella

Marco C Lam

Thomas H. Reiprich

Alvise Raccanelli

Sebastiano Cantalupo

Simon Morris

Bayesian luminosity function estimation in multi-depth datasets with selection effects: A case study for 3 < z < 5 Lyman α emitters

The relationship between gas and galaxies at z < 1 using the Q0107 quasar triplet