activity
20032021
most citedImproved constraints on the expansion rate of the Universe up to z~1.1 from the spectroscopic evolution of cosmic chronometers

1k citations · 8.2k across the 90 of their papers we have counts for

collaborators

89 papers

astro-ph.GA2021★ 47 cited

CLASH-VLT: Abell~S1063. Cluster assembly history and spectroscopic catalogue

A. Mercurio, P. Rosati, A. Biviano +31

Using the CLASH-VLT survey, we assembled an unprecedented sample of 1234 spectroscopically confirmed members in Abell~S1063, finding a dynamically complex structure at z_cl=0.3457…

astro-ph.GA2021★ 92 cited

The VANDELS ESO public spectroscopic survey: final Data Release of 2087 spectra and spectroscopic measurements

B. Garilli, R. McLure, L. Pentericci +94

VANDELS is an ESO Public Spectroscopic Survey designed to build a sample of high signal to noise, medium resolution spectra of galaxies at redshift between 1 and 6.5. Here we prese…

astro-ph.GA2020★ 78 cited

The MUSE Deep Lensed Field on the Hubble Frontier Field MACS~J0416

E. Vanzella, G. B. Caminha, P. Rosati +21

Context: A census of faint and tiny star forming complexes at high redshift is key to improving our understanding of reionizing sources, galaxy growth and the formation of globular…

astro-ph.GA2020★ 58 cited

Candidate Population III stellar complex at z=6.629 in the MUSE Deep Lensed Field

E. Vanzella, M. Meneghetti, G. B. Caminha +20

We discovered a strongly lensed (μ>40) Lya emission at z=6.629 (S/N~18) in the MUSE Deep Lensed Field (MDLF) targeting the Hubble Frontier Field galaxy cluster MACS~J0416. Dedicate…

astro-ph.GA2019★ 94 cited

Strong lensing models of eight CLASH clusters from extensive spectroscopy: accurate total mass reconstructions in the cores

G. B. Caminha, P. Rosati, C. Grillo +19

We carry out a detailed strong lensing analysis of a sub-sample of eight galaxy clusters of the CLASH survey, in the redshift range of , using exten…

astro-ph.GA2018★ 26 cited

Quantifying the suppression of the (un)-obscured star formation in galaxy cluster cores at 0.20.9

L. Rodríguez-Muñoz, G. Rodighiero, C. Mancini +21

We quantify the star formation (SF) in the inner cores (/0.3) of 24 massive galaxy clusters at 0.20.9 observed by the …