activity
20152024
most citedMusE GAs FLOw and Wind (MEGAFLOW) II. A study of gas accretion around star-forming galaxies with background quasars

131 citations · 787 across the 19 of their papers we have counts for

collaborators

31 papers

astro-ph.GA20212 cited

Implications of a spatially resolved main sequence for the size evolution of star forming galaxies

Gabriele Pezzulli

Two currently debated problems in galaxy evolution, the fundamentally local or global nature of the main sequence of star formation and the evolution of the mass-size relation of s…

astro-ph.GA202146 cited

A tight angular-momentum plane for disc galaxies

Pavel E. Mancera Piña, Lorenzo Posti, Gabriele Pezzulli +4

The relations between the specific angular momenta () and masses () of galaxies are often used as a benchmark in analytic models and hydrodynamical simulations as they are co…

astro-ph.GA202113 cited

The MUSE-Wide survey: Three-dimensional clustering analysis of Lyman- emitters at

Y. Herrero Alonso, M. Krumpe, L. Wisotzki +12

We present an analysis of the spatial clustering of 695 Ly-emitting galaxies (LAE) in the MUSE-Wide survey. All objects have spectroscopically confirmed redshifts in the range $…

astro-ph.GA202116 cited

Constraining the cosmic UV background at z>3 with MUSE Lyman-α emission observations

Sofia G. Gallego, Sebastiano Cantalupo, Saeed Sarpas +10

The intensity of the Cosmic UV background (UVB), coming from all sources of ionising photons such as star-forming galaxies and quasars, determines the thermal evolution and ionizat…

astro-ph.GA2021

The X-SHOOTER Lyman- survey at z=2 (XLS-z2) I: What makes a galaxy a Lyman- emitter?

Jorryt Matthee, David Sobral, Matthew Hayes +9

We present the first results from the X-SHOOTER Lyman- survey at (XLS-). XLS- is a deep spectroscopic survey of 35 Lyman- emitters (LAEs) utilising

astro-ph.GA202021 cited

Most of the cool CGM of star-forming galaxies is not produced by supernova feedback

Andrea Afruni, Filippo Fraternali, Gabriele Pezzulli

The characterization of the large amount of gas residing in the galaxy halos, the so called circumgalactic medium (CGM), is crucial to understand galaxy evolution across cosmic tim…