activity
19972026
most citedGaia Data Release 2. Summary of the contents and survey properties

8.6k citations · 28.3k across the 161 of their papers we have counts for

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Showing 2019Show all

8 papers · 1 filter

astro-ph.SR2019★ 3 cited

Stellar population astrophysics (SPA) with the TNG. Characterization of the young open cluster ASCC 123

A. Frasca, J. Alonso-Santiago, G. Catanzaro +10

Star clusters are key to understand the stellar and Galactic evolution. ASCC 123 is a little-studied, nearby and very sparse open cluster. We performed the first high-resolution sp…

astro-ph.IM2019★ 8 cited

Voyage 2050 White Paper: All-Sky Visible and Near Infrared Space Astrometry

David Hobbs, Anthony Brown, Erik Høg +27

A new all-sky visible and Near-InfraRed (NIR) space astrometry mission with a wavelength cutoff in the K-band is not just focused on a single or small number of key science cases.…

astro-ph.GA2019★ 64 cited

The Gaia-ESO survey: Calibrating a relationship between Age and the [C/N] abundance ratio with open clusters

G. Casali, L. Magrini, E. Tognelli +51

In the era of large high-resolution spectroscopic surveys, high-quality spectra can contribute to our understanding of the Galactic chemical evolution, providing chemical abundance…

astro-ph.SR2019★ 18 cited

The Gaia-ESO Survey: The inner disc, intermediate-age open cluster Pismis 18

D. Hatzidimitriou, E. V. Held, E. Tognelli +34

Pismis 18 is a moderately populated, intermediate-age open cluster located within the solar circle at a Galactocentric distance of about 7 kpc. Few open clusters have been studied…

astro-ph.SR2019★ 59 cited

New light on the Gaia DR2 parallax zero-point: influence of the asteroseismic approach, in and beyond the Kepler field

Saniya Khan, Andrea Miglio, Benoît Mosser +15

The importance of studying the Gaia DR2 parallax zero-point by external means was underlined by Lindegren et al. (2018), and initiated by several works making use of Cepheids, ecli…

astro-ph.SR2019★ 69 cited

The extended halo of NGC 2682 (M 67) from Gaia DR2

R. Carrera, M. Pasquato, A. Vallenari +8

Context: NGC 2682 is a nearby open cluster, approximately 3.5 Gyr old. Dynamically, most open clusters should dissolve on shorter timescales, of ~ 1 Gyr. Having survived until now,…