activity
20102024
most citedThe PLATO 2.0 Mission

1.3k citations · 1.4k across the 9 of their papers we have counts for

collaborators

9 papers

astro-ph.IM2024★ 13 cited

The PLATO Mission

Heike Rauer, Conny Aerts, Juan Cabrera +842

PLATO (PLAnetary Transits and Oscillations of stars) is ESA's M3 mission designed to detect and characterise extrasolar planets and perform asteroseismic monitoring of a large numb…

astro-ph.SR2023

Near-IR and optical radial velocities of the active M dwarf star Gl 388 (AD Leo) with SPIRou at CFHT and SOPHIE at OHP: A 2.23 day rotation period and no evidence for a corotating planet

A. Carmona, X. Delfosse, S. Bellotti +36

Context: The search for extrasolar planets around the nearest M dwarfs is a crucial step towards identifying the nearest Earth-like planets. One of the main challenges in this sear…

astro-ph.EP2018★ 8 cited

Reconciling the predictions of microlensing analysis with radial velocity measurements for OGLE-2011-BLG-0417

E. Bachelet, J. -P. Beaulieu, I. Boisse +2

Microlensing is able to reveal multiple body systems located several kilo-parsec away from the Earth. Since it does not require the measurement of light from the lens, microlensing…

astro-ph.EP2018★ 23 cited

SOPHIE velocimetry of Kepler transit candidates XVIII. Radial velocity confirmation, absolute masses and radii, and origin of the Kepler-419 multiplanetary system

J. M. Almenara, R. F. Díaz, G. Hébrard +14

Kepler-419 is a planetary system discovered by the Kepler photometry which is known to harbour two massive giant planets: [...] Here we present new radial velocity (RV) measurement…

astro-ph.EP2015★ 1 cited

PASTIS: Bayesian extrasolar planet validation II. Constraining exoplanet blend scenarios using spectroscopic diagnoses

A. Santerne, R. F. Díaz, J. -M. Almenara +7

The statistical validation of transiting exoplanets proved to be an efficient technique to secure the nature of small exoplanet signals which cannot be established by purely spectr…

astro-ph.EP2015★ 48 cited

One of the closest exoplanet pairs to the 3:2 Mean Motion Resonance: K2-19b \& c

David J. Armstrong, Alexandre Santerne, Dimitri Veras +25

The K2 mission has recently begun to discover new and diverse planetary systems. In December 2014 Campaign 1 data from the mission was released, providing high-precision photometry…