activity
19932023
most citedQuantifying the uncertainties of chemical evolution studies. II. Stellar yields

409 citations · 4.5k across the 115 of their papers we have counts for

collaborators

116 papers

astro-ph.GA2023

Universal Upper End of the Stellar Initial Mass Function in the Young and Compact LEGUS clusters

Dooseok Escher Jung, Daniela Calzetti, Matteo Messa +21

We investigate the variation in the upper end of stellar initial mass function (uIMF) in 375 young and compact star clusters in five nearby galaxies within Mpc. All the yo…

astro-ph.GA2023★ 9 cited

Gas, dust, and the CO-to-molecular gas conversion factor in low-metallicity starbursts

L. K. Hunt, F. Belfiore, F. Lelli +19

The factor relating CO emission to molecular hydrogen column density, XCO, is still subject to uncertainty, in particular at low metallicity. Here, to quantify XCO at two different…

astro-ph.GA2022★ 5 cited

DDO68 C: the actual appearance of a ghost satellite dwarf through adaptive optics at the Large Binocular Telescope

Francesca Annibali, Enrico Pinna, Leslie K. Hunt +12

Through adaptive optics (AO) imaging with the SOUL+LUCI instrument at the Large Binocular Telescope we were able to resolve, for the first time, individual stars in the gas-rich ga…

astro-ph.GA2022★ 21 cited

Fraction of Stars in Clusters for the LEGUS Dwarf Galaxies

D. O. Cook, J. C. Lee, A. Adamo +20

We study the young star cluster populations in 23 dwarf and irregular galaxies observed by the HST Legacy ExtraGalactic Ultraviolet Survey (LEGUS), and examine relationships betwee…

astro-ph.SR2022★ 133 cited

The Gaia-ESO Public Spectroscopic Survey: Motivation, implementation, GIRAFFE data processing, analysis, and final data products

G. Gilmore, S. Randich, C. C. Worley +165

The Gaia-ESO Public Spectroscopic Survey is an ambitious project designed to obtain astrophysical parameters and elemental abundances for 100,000 stars, including large representat…

astro-ph.GA2022★ 6 cited

KMHK 1762: Another star cluster in the Large Magellanic Cloud age gap

M. Gatto, V. Ripepi, M. Bellazzini +11

The star cluster (SC) age distribution of the Large Magellanic Cloud (LMC) exhibits a gap from 4 to 10 Gyr ago, with an almost total absence of SCs. Within this age gap, onl…