activity
20132022
most citedThe Wide Field Infrared Survey Telescope: 100 Hubbles for the 2020s

178 citations · 1.2k across the 39 of their papers we have counts for

collaborators

56 papers

astro-ph.SR202215 cited

The HST large programme on NGC 6752 -- IV. The White Dwarf Sequence

L. R. Bedin, M. Salaris, J. Anderson +13

We present our final study of the white dwarf cooling sequence (WD CS) in the globular cluster NGC 6752. The investigation is the main goal of a dedicated Hubble Space Telescope la…

astro-ph.SR202228 cited

Survey of multiple populations in globular clusters among very low-mass stars

E. Dondoglio, A. P. Milone, A. Renzini +14

Recent work has shown that NIR Hubble Space Telescope (HST) photometry allows us to disentangle multiple populations (MPs) among M dwarfs of globular clusters (GCs) and investigate…

astro-ph.SR202126 cited

The HST large programme on omega Centauri -- IV. catalogue of two external fields

M. Scalco, A. Bellini, L. R. Bedin +10

In the fourth paper of this series, we present -- and publicly release -- the state-of-the-art catalogue and atlases for the two remaining parallel fields observed with the Hubble…

astro-ph.GA2021

3D core kinematics of NGC6362: central rotation in a dynamically evolved globular cluster

E. Dalessandro, S. Raso, S. Kamann +4

We present a detailed 3D kinematic analysis of the central regions () of the low-mass and dynamically evolved galactic globular cluster NGC 6362. The study is based on data…

astro-ph.GA202120 cited

Hunting for intermediate-mass black holes in globular clusters: an astrometric study of NGC 6441

Maximilian Häberle, Mattia Libralato, Andrea Bellini +6

We present an astrometric study of the proper motions (PMs) in the core of the globular cluster NGC 6441. The core of this cluster has a high density and observations with current…

astro-ph.GA20216 cited

The wide upper main sequence and main sequence turnoff of the ~ 800 Myr old star cluster NGC1831

Matteo Correnti, Paul Goudfrooij, Andrea Bellini +1

We present the analysis of the colour-magnitude diagram (CMD) morphology of the ~ 800 Myr old star cluster NGC1831 in the Large Magellanic Cloud, exploiting deep, high-resolution p…