activity
20072026
most citedShadows and spirals in the protoplanetary disk HD 100453

213 citations · 405 across the 4 of their papers we have counts for

collaborators

6 papers

astro-ph.SR2026

SPHERE/ZIMPOL observations of the symbiotic system R Aquarii. II. Dynamics of the dust in the Mira wind and the Halpha gas in the jet

H. M. Schmid, E. Lagadec, J. Milli +17

R Aqr is a resolved symbiotic Mira binary and a prototype target for the study of complex hydrodynamic processes including dust-driven mass loss, mass transfer, accretion, and jet…

astro-ph.EP2025★ 64 cited

A temperate super-Jupiter imaged with JWST in the mid-infrared

E. C. Matthews, A. L. Carter, P. Pathak +16

Of the ~25 directly imaged planets to date, all are younger than 500Myr and all but 6 are younger than 100Myr. Eps Ind A (HD209100, HIP108870) is a K5V star of roughly solar age (r…

astro-ph.IM2023

Exoplanet imaging with ELTs: exploring a second-stage AO with a Zernike wavefront sensor on the ESO/GHOST testbed

Mamadou N'Diaye, Arthur Vigan, Byron Engler +6

We propose to explore a cascade extreme Adaptive optics (ExAO) approach with a second stage based on a Zernike wavefront sensor (ZWFS) for exoplanet imaging and spectroscopy. Most…

astro-ph.EP2016★ 213 cited

Shadows and spirals in the protoplanetary disk HD 100453

M. Benisty, T. Stolker, A. Pohl +46

Understanding the diversity of planets requires to study the morphology and the physical conditions in the protoplanetary disks in which they form. We observed and spatially resolv…

astro-ph.IM2013★ 47 cited

Speckle temporal stability in XAO coronagraphic images II. Refine model for quasi-static speckle temporal evolution for VLT/SPHERE

P. Martinez, M. Kasper, A. Costille +4

Observing sequences have shown that the major noise source limitation in high-contrast imaging is due to the presence of quasi-static speckles. The timescale on which quasi-static…

astro-ph2007★ 81 cited

A Survey for Massive Giant Planets in Debris Disks with Evacuated Inner Cavities

D. Apai, M. Janson, A. Moro-Martin +9

The commonality of collisionally replenished debris around main sequence stars suggests that minor bodies are frequent around Sun-like stars. Whether or not debris disks in general…