activity
20022025
most citedChemical abundance analysis of the Open Clusters Cr110, NGC2099 (M37), NGC2420, NGC7789 and M67 (NGC2682)

210 citations · 927 across the 14 of their papers we have counts for

collaborators

14 papers

astro-ph.GA2025★ 8 cited

The Missing Globular Cluster Survey. I. Survey overview and the first precise age estimate for ESO452-11 and 2MASS-GC01

D. Massari, M. Bellazzini, M. Libralato +17

We present the Missing Globular Cluster Survey (MGCS), a Treasury Program dedicated to the observation of all kinematically confirmed Milky Wa…

astro-ph.GA2024★ 31 cited

OCCASO V. Chemical-abundance trends with Galactocentric distance and age

J. Carbajo-Hijarrubia, L. Casamiquela, R. Carrera +12

Context. Open clusters provide valuable information on stellar nucleosynthesis and the chemical evolution of the Galactic disc, as their age and distances can be measured more prec…

astro-ph.GA2024★ 9 cited

SpectroTranslator: a deep-neural network algorithm to homogenize spectroscopic parameters

G. F. Thomas, G. Battaglia, F. Gran +8

The emergence of large spectroscopic surveys requires homogenising on the same scale the quantities they measure in order to increase their scientific legacy. We developed the Spec…

astro-ph.GA2021★ 75 cited

Survey of Surveys I: The largest catalogue of radial velocities for the Galaxy

M. Tsantaki, E. Pancino, P. Marrese +8

In the present-day panorama of large spectroscopic surveys, the amount, diversity, and complexity of the available data continuously increase. We present a comprehensive catalogue,…

astro-ph.GA2019★ 51 cited

OCCASO III. Iron peak and elements of 18 open clusters. Comparison with chemical evolution models and field stars

L. Casamiquela, S. Blanco-Cuaresma, R. Carrera +10

The study of open-cluster chemical abundances provides insights on stellar nucleosynthesis processes and on Galactic chemo-dynamical evolution. In this paper we present an extended…

astro-ph.GA2017★ 22 cited

NGC 6705 a young -enhanced Open Cluster from OCCASO data

L. Casamiquela, R. Carrera, L. Balaguer-Núñez +12

The stellar [/Fe] abundance is sometimes used as a proxy for stellar age, following standard chemical evolution models for the Galaxy, as seen by different observational results…