activity
20102023
most citedStellar characterization of CoRoT/Exoplanet fields with MATISSE

39 citations · 78 across the 4 of their papers we have counts for

collaborators

10 papers

astro-ph.GA2020

Gaia Early Data Release 3: Acceleration of the solar system from Gaia astrometry

Gaia Collaboration, S. A. Klioner, F. Mignard +414

Context. Gaia Early Data Release 3 (Gaia EDR3) provides accurate astrometry for about 1.6 million compact (QSO-like) extragalactic sources, 1.2 million of which have the best-quali…

astro-ph.GA202023 cited

The AMBRE Project: Spectrum normalisation influence on Mg abundances in the metal-rich Galactic disc

Pablo Santos-Peral, Alejandra Recio-Blanco, Patrick de Laverny +2

The abundance of α-elements provides an important fossil signature in Galactic archaeology to trace the chemical evolution of the different disc populations. High-precision chemica…

astro-ph.GA2018

Gaia Data Release 2. Summary of the contents and survey properties

Gaia Collaboration, A. G. A. Brown, A. Vallenari +4

We present the second Gaia data release, Gaia DR2, consisting of astrometry, photometry, radial velocities, and information on astrophysical parameters and variability, for sources…

astro-ph.IM2018

Gaia Data Release 2. Short-timescale variability processing and analysis

M. Roelens, L. Eyer, N. Mowlavi +13

The Gaia DR2 sample of short-timescale variable candidates results from the investigation of the first 22 months of Gaia photometry for a subsample of sources at the Gaia faint end…

astro-ph.EP2018

Gaia Data Release 2: Observations of solar system objects

Gaia Collaboration, F. Spoto, P. Tanga +4

The Gaia spacecraft of the European Space Agency (ESA) has been securing observations of solar system objects (SSOs) since the beginning of its operations. Gaia Data Release 2 (DR2…

astro-ph.SR2018

Gaia Data Release 2: first stellar parameters from Apsis

Rene Andrae, Morgan Fouesneau, Orlagh Creevey +13

The second Gaia data release (Gaia-DR2) contains, beyond the astrometry, three-band photometry for 1.38 billion sources. We have used these three broad bands to infer stellar effec…