Michele Fumagalli
University of Milan
257 Papers
2.4K Citations
Michele Fumagalli is an academic researcher from University of Milan. The author has contributed to research in topics: Galaxy & Redshift. The author has an hindex of 59, co-authored 227 publications. Previous affiliations of Michele Fumagalli include Princeton University & Leiden University.
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Papers
Metal-enriched, subkiloparsec gas clumps in the circumgalactic medium of a faint z = 2.5 galaxy
Neil H. M. Crighton,Joseph F. Hennawi,Robert A. Simcoe,Kathy L. Cooksey,Michael T. Murphy,Michele Fumagalli,Michele Fumagalli,J. Xavier Prochaska,Tom Shanks +8 more
TL;DR: In this paper, a 0.2 L*, Lyα emitting galaxy at redshift 2.5 at an impact parameter of 50 kpc from a bright background QSO sightline was detected.
The brightest young star clusters in ngc 5253
Daniela Calzetti,K. E. Johnson,Angela Adamo,John S. Gallagher,Jennifer E. Andrews,Linda J. Smith,Geoffrey C. Clayton,J. C. Lee,J. C. Lee,Elena Sabbi,Leonardo Ubeda,Hwihyun Kim,Hwihyun Kim,J. E. Ryon,David A. Thilker,S. N. Bright,Erik Zackrisson,Robert C. Kennicutt,S. E. de Mink,B. C. Whitmore,Alessandra Aloisi,Rupali Chandar,Michele Cignoni,David O. Cook,Daniel A. Dale,Bruce G. Elmegreen,Debra Meloy Elmegreen,Aaron S. Evans,Aaron S. Evans,Michele Fumagalli,Dimitrios A. Gouliermis,Dimitrios A. Gouliermis,Kathryn Grasha,Eva K. Grebel,Mark R. Krumholz,Rene A. M. Walterbos,Aida Wofford,Thomas M. Brown,Carol Christian,Clare Dobbs,A. Herrero,A. Herrero,L. Kahre,Matteo Messa,P. Nair,Antonella Nota,Göran Östlin,Anne Pellerin,Elena Sacchi,Daniel Schaerer,Monica Tosi +50 more
TL;DR: In this article, the role of the radio nebula in the starburst energetics was investigated by combining new and archival Hubble Space Telescope images of NGC 5253 with wavelength coverage from 1500 A to 1.9 μm in 13 filters.
Directly imaging damped Lyman α galaxies at z>2 - I. Methodology and first results
TL;DR: In this article, the authors presented the methodology for, and the first results from, a new imaging programme aimed at identifying and characterizing the host galaxies of damped Lyman α absorbers (DLAs) at z ≳ 2.69 DLA towards J073149+285449, a galaxy with impact parameter b = 1.54 arcsec = 11.89 h − 1 72 kpc and an implied star formation rate (SFR) of ∼5 h − 2 72 M ⊙ yr − 1.
Towards ultra metal-poor DLAs: linking the chemistry of the most metal-poor DLA to the first stars
TL;DR: In this paper , the authors presented new Keck/HIRES data of the most metal-poor damped Lyα (DLA) system currently known, and they used the chemistry of this DLA combined with a stochastic chemical enrichment model to probe its enrichment history.
The MUSE Ultra Deep Field (MUDF). II. Survey design and the gaseous properties of galaxy groups at 0.5 < z < 1.5
Matteo Fossati,Michele Fumagalli,Michele Fumagalli,Emma K. Lofthouse,Valentina D'Odorico,Elisabeta Lusso,Elisabeta Lusso,Sebastiano Cantalupo,Ryan Cooke,Stefano Cristiani,Francesco Haardt,Francesco Haardt,Simon L. Morris,Celine Peroux,Celine Peroux,L. J. Prichard,Marc Rafelski,Marc Rafelski,Ian Smail,Tom Theuns +19 more
TL;DR: The results of the MUDF survey as discussed by the authors show that the galaxy environment and gaseous properties of seven groups detected at redshifts 0.5 < z < 1.5, spanning a large dynamic range in halo mass, log(Mh/M⊙)≈11−13.