activity
20162018
most citedDiscovery of a warm, dusty giant planet around HIP65426

205 citations · 342 across the 5 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.EP201776 cited

Investigation of the inner structures around HD169142 with VLT/SPHERE

R. Ligi, A. Vigan, R. Gratton +47

We present observations of the Herbig Ae star HD169142 with VLT/SPHERE instruments InfraRed Dual-band Imager and Spectrograph (IRDIS) ( and bands) and the Integral Fie…

astro-ph.EP201719 cited

Orbiting a binary: SPHERE characterisation of the HD 284149 system

Mariangela Bonavita, V. D'Orazi, D. Mesa +52

In this paper we present the results of the SPHERE observation of the HD 284149 system, aimed at a more detailed characterisation of both the primary and its brown dwarf companion.…

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.EP201741 cited

New constraints on the disk characteristics and companion candidates around T Cha with VLT/SPHERE

A. Pohl, E. Sissa, M. Langlois +34

The transition disk around the T Tauri star T Cha possesses a large gap, making it a prime target for high-resolution imaging in the context of planet formation. We aim to find sig…

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…