activity
20152018
most citedDiscovery of a warm, dusty giant planet around HIP65426

205 citations · 618 across the 7 of their papers we have counts for

collaborators

7 papers

astro-ph.EP20181 cited

Investigating the young Solar System analog HD95086

G. Chauvin, R. Gratton, M. Bonnefoy +57

HD95086 (A8V, 17Myr) hosts a rare planetary system for which a multi-belt debris disk and a giant planet of 4-5MJup have been directly imaged. Our study aims to characterize the ph…

astro-ph.EP201769 cited

Variable dynamics in the inner disk of HD 135344B revealed with multi-epoch scattered light imaging

Tomas Stolker, Mike Sitko, Bernard Lazareff +12

We present multi-epoch VLT/SPHERE observations of the protoplanetary disk around HD 135344B (SAO 206462). The -band scattered light imagery reveal, with high spatial resolution…

astro-ph.EP201745 cited

The HIP 79977 debris disk in polarized light

N. Engler, H. M. Schmid, Ch. Thalmann +40

We present observations of the known edge-on debris disk around HIP 79977 (HD 146897, F star in Upper Sco, 123 pc), taken with the ZIMPOL differential polarimeter of the SPHERE ins…

astro-ph.SR201770 cited

In-depth study of moderately young but extremely red, very dusty substellar companion HD206893B

P. Delorme, T. Schmidt, M. Bonnefoy +47

The substellar companion HD206893b has recently been discovered by direct imaging of its disc-bearing host star with the SPHERE instrument. We investigate the atypical properties o…

astro-ph.EP2017205 cited

Discovery of a warm, dusty giant planet around HIP65426

G. Chauvin, S. Desidera, A. -M. Lagrange +120

The SHINE program is a large high-contrast near-infrared survey of 600 young, nearby stars. It is aimed at searching for and characterizing new planetary systems using VLT/SPHERE's…

astro-ph.EP2016

Discovery of concentric broken rings at sub-arcsec separations in the HD 141569A gas-rich, debris disk with VLT/SPHERE

C. Perrot, A. Boccaletti, E. Pantin +45

Transition disks correspond to a short stage between the young protoplanetary phase and older debris phase. Along this evolutionary sequence, the gas component disappears leaving r…