activity
20042025
most citedSpectroscopic parameters for 451 stars in the HARPS GTO planet search program. Stellar [Fe/H] and the frequency of exo-Neptunes

596 citations · 7.4k across the 86 of their papers we have counts for

collaborators
Showing 2019Show all

14 papers · 1 filter

astro-ph.EP2019★ 109 cited

Measuring precise radial velocities on individual spectral lines : II. Dependance of stellar activity signal on line depth

M. Cretignier, X. Dumusque, R. Allart +2

Context. Although the new generation of radial-velocity (RV) instruments such as ESPRESSO are expected to reach the long-term precision required to find other earths, the RV measur…

astro-ph.EP2019★ 51 cited

The SOPHIE search for northern extrasolar planets. XVI. HD 158259: A compact planetary system in a near-3:2 mean motion resonance chain

N. C. Hara, F. Bouchy, M. Stalport +32

Since 2011, the SOPHIE spectrograph has been used to search for Neptunes and super-Earths in the Northern Hemisphere. As part of this observational program, 290 radial velocity mea…

astro-ph.SR2019★ 65 cited

The detection and characterisation of 54 massive companions with the SOPHIE spectrograph -- 7 new brown dwarfs and constraints on the BD desert

F. Kiefer, G. Hébrard, J. Sahlmann +35

Brown-dwarfs are substellar objects with masses intermediate between planets and stars within about 13-80Mjup. While isolated BDs are most likely produced by gravitational collapse…

astro-ph.EP2019★ 63 cited

Catalog for the ESPRESSO blind radial velocity exoplanet survey

S. Hojjatpanah, P. Figueira, N. C. Santos +19

One of the main scientific drivers for ESPRESSO,Échelle SPectrograph, is the detection and characterization of Earth-class exoplanets. With this goal in mind, the ESPRESSO Guarante…

astro-ph.EP2019★ 10 cited

ISPY -- NaCo Imaging Survey for Planets around Young stars. Discovery of an M dwarf in the gap between HD 193571 and its debris ring

Arianna Musso Barcucci, Ralf Launhardt, Grant M. Kennedy +19

Context. The interaction between low-mass companions and the debris discs they reside in is still not fully understood. A debris disc can evolve due to self-stirring, a process in…

astro-ph.EP2019★ 77 cited

Characterization of the L 98-59 multi-planetary system with HARPS: two confirmed terrestrial planets and a mass upper limit on the third

R. Cloutier, N. Astudillo-Defru, X. Bonfils +33

L 98-59 (TIC 307210830, TOI-175) is a nearby M3 dwarf around which TESS revealed three terrestrial-sized transiting planets (0.80, 1.35, 1.57 Earth radii) in a compact configuratio…