activity
20152021
most citedDiscovery of a planetary-mass companion within the gap of the transition disk around PDS 70

700 citations · 1.2k across the 7 of their papers we have counts for

collaborators

7 papers

astro-ph.EP2021★ 17 cited

Investigating point sources in MWC 758 with SPHERE

A. Boccaletti, E. Pantin, F. Ménard +26

Context. Spiral arms in protoplanetary disks could be shown to be the manifestation of density waves launched by protoplanets and propagating in the gaseous component of the disk.…

astro-ph.EP2020★ 230 cited

The SPHERE infrared survey for exoplanets (SHINE). III. The demographics of young giant exoplanets below 300 au with SPHERE

A. Vigan, C. Fontanive, M. Meyer +108

The SHINE project is a 500-star survey performed with SPHERE on the VLT for the purpose of directly detecting new substellar companions and understanding their formation and early…

astro-ph.SR2018★ 16 cited

Mapping of shadows cast on a protoplanetary disk by a close binary system

V. D'Orazi, R. Gratton, S. Desidera +47

For a comprehensive understanding of planetary formation and evolution, we need to investigate the environment in which planets form: circumstellar disks. Here we present high-cont…

astro-ph.EP2018★ 700 cited

Discovery of a planetary-mass companion within the gap of the transition disk around PDS 70

M. Keppler, M. Benisty, A. Müller +123

Young circumstellar disks are of prime interest to understand the physical and chemical conditions under which planet formation takes place. Only very few detections of planet cand…

astro-ph.EP2018★ 1 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.EP2017★ 93 cited

The circumstellar disk HD169142: gas, dust and planets acting in concert?

A. Pohl, M. Benisty, P. Pinilla +33

HD169142 is an excellent target to investigate signs of planet-disk interaction due to the previous evidence of gap structures. We performed J-band (~1.2μm) polarized intensity…