activity
20012016
most citedThe PLATO 2.0 Mission

1.3k citations · 2.9k across the 8 of their papers we have counts for

collaborators

8 papers

astro-ph.SR2016★ 514 cited

The Radial Velocity Experiment (RAVE): Fifth Data Release

Andrea Kunder, Georges Kordopatis, Matthias Steinmetz +51

Data Release 5 (DR5) of the Radial Velocity Experiment (RAVE) is the fifth data release from a magnitude-limited (9< I < 12) survey of stars randomly selected in the southern hemis…

astro-ph.GA2015★ 16 cited

The Gaia-ESO Survey: Separating disk chemical substructures with cluster models

A. Rojas-Arriagada, A. Recio-Blanco, P. de Laverny +24

(Abridged) Recent spectroscopic surveys have begun to explore the Galactic disk system outside the solar neighborhood on the basis of large data samples. In this way, they provide…

astro-ph.GA2015★ 51 cited

The Gaia-ESO Survey: New constraints on the Galactic disc velocity dispersion and its chemical dependencies

G. Guiglion, A. Recio-Blanco, P. de Laverny +27

Understanding the history and the evolution of the Milky Way disc is one of the main goals of modern astrophysics. We study the velocity dispersion behaviour of Galactic disc stars…

astro-ph.GA2015★ 43 cited

A new method for estimating the pattern speed of spiral structure in the Milky Way

T. C. Junqueira, C. Chiappini, J. R. D. Lépine +2

In the last few decades many efforts have been made to understand the effect of spiral arms on the gas and stellar dynamics in the Milky Way disc. One of the fundamental parameters…

astro-ph.EP2013★ 1.3k cited

The PLATO 2.0 Mission

H. Rauer, C. Catala, C. Aerts +159

PLATO 2.0 has recently been selected for ESA's M3 launch opportunity (2022/24). Providing accurate key planet parameters (radius, mass, density and age) in statistical numbers, it…

astro-ph.CO2009★ 1 cited

The Mass-Metallicity relation in galaxies of different morphological types

F. Calura, A. Pipino, C. Chiappini +4

By means of chemical evolution models of different morphological types, we study the mass-metallicity (MZ) relation and its evolution with redshift. Our aim is to understand the ro…