activity
20152025
most citedDiscovery of a warm, dusty giant planet around HIP65426

205 citations · 1.6k across the 45 of their papers we have counts for

collaborators
Showing 2019Show all

7 papers · 1 filter

astro-ph.EP2019★ 36 cited

A HARPS RV search for planets around young nearby stars

A. Grandjean, A. -M. Lagrange, M. Keppler +9

Young nearby stars are good candidates in the search for planets with both radial velocity (RV) and direct imaging techniques. This, in turn, allows for the computation of the gian…

astro-ph.EP2019★ 84 cited

VLT/SPHERE exploration of the young multiplanetary system PDS70

D. Mesa, M. Keppler, F. Cantalloube +51

Context. PDS 70 is a young (5.4 Myr), nearby (~113 pc) star hosting a known transition disk with a large gap. Recent observations with SPHERE and NACO in the near-infrared (NIR) al…

astro-ph.EP2019★ 9 cited

ODEA: Orbital Dynamics in a complex Evolving Architecture -- Application to the planetary system HD 106906

L. Rodet, H. Beust, M. Bonnefoy +3

Mixed-variable symplectic integrators are widely used in orbital dynamics. However, they have been developed for Solar system-type architectures, and can not handle evolving hierar…

astro-ph.EP2019★ 1 cited

Constraining the properties of HD 206893 B. A combination of radial velocity, direct imaging, and astrometry data

A. Grandjean, A. -M. Lagrange, H. Beust +25

High contrast imaging enables the determination of orbital parameters for substellar companions (planets, brown dwarfs) from the observed relative astrometry and the estimation of…

astro-ph.EP2019★ 16 cited

Two cold belts in the debris disk around the G-type star NZ Lup

A. Boccaletti, P. Thébault, N. Pawellek +36

Planetary systems hold the imprint of the formation and of the evolution of planets especially at young ages, and in particular at the stage when the gas has dissipated leaving mos…

astro-ph.EP2019★ 44 cited

Hint of curvature in the orbital motion of the exoplanet 51 Eridani b using 3 years of VLT/SPHERE monitoring

A. -L. Maire, L. Rodet, F. Cantalloube +49

Context. The 51 Eridani system harbors a complex architecture with its primary star forming a hierarchical system with the binary GJ 3305AB at a projected separation of 2000 au, a…