activity
20002026
most citedThe ACS Virgo Cluster Survey. XII. The Luminosity Function of Globular Clusters in Early Type Galaxies

337 citations · 4.6k across the 80 of their papers we have counts for

collaborators

79 papers

astro-ph.SR2026

Euclid: The convective-transition gap of 47 Tuc

M. Libralato, M. Griggio, R. Gerasimov +140

We report the first detection of the `convective-transition gap' (also known as `M-dwarf gap') in the globular cluster 47 Tuc (NGC 104) thanks to Euclid data. This feature, linked…

astro-ph.GA2023★ 16 cited

Intracluster light in the core of z~2 galaxy proto-clusters

S. V. Werner, N. A. Hatch, J. Matharu +5

Intracluster light is thought to originate from stars that were ripped away from their parent galaxies by gravitational tides and galaxy interactions during the build up of the clu…

astro-ph.IM2023

Gender and Precarity in Astronomy

N. A. Webb, C. Bot, S. Charpinet +6

Following the survey Well-being in astrophysics that was sent out in March 2021, to establish how astrophysics researchers, primarily in France, experience their career, some of th…

astro-ph.CO2023★ 19 cited

YOLO-CL: Galaxy cluster detection in the SDSS with deep machine learning

Kirill Grishin, Simona Mei, Stéphane Ilic

(Abridged) Galaxy clusters are a powerful probe of cosmological models. Next generation large-scale optical and infrared surveys will reach unprecedented depths over large areas an…

astro-ph.GA2022★ 22 cited

The galaxy mass-size relation in CARLA clusters and proto-clusters at 1.4 < z < 2.8: larger cluster galaxy sizes

Anton V. Afanasiev, Simona Mei, Hao Fu +12

(Abridged) We study the galaxy mass-size relation in CARLA spectroscopically confirmed clusters at , which span a total stellar mass $11.3<\mathrm{log}(M^c_*/M_{\odot})<…

astro-ph.GA2022

Morphology-density Relation, Quenching, and Mergers in CARLA Clusters and Proto-Clusters at

Simona Mei, Nina A. Hatch, Stefania Amodeo +11

(Abridged) To understand if the morphology-density and passive-density relations are already established at z>1.5, we study galaxies in 16 confirmed clusters at from th…