activity
20132025
most citedAsymmetric features in the protoplanetary disk MWC758

318 citations · 754 across the 9 of their papers we have counts for

collaborators

9 papers

astro-ph.EP2025★ 12 cited

MIRI-LRS spectrum of a cold exoplanet around a white dwarf: water, ammonia, and methane measurements

Maël Voyer, Quentin Changeat, Pierre-Olivier Lagage +21

The study of the atmosphere of exoplanets orbiting white dwarfs is a largely unexplored field. With WD\,0806-661\,b, we present the first deep dive into the atmospheric physics and…

astro-ph.EP2024★ 10 cited

SO as shock tracer in protoplanetary disks: the AB Aurigae case

A. Dutrey, E. Chapillon, S. Guilloteau +9

{Sulfur Monoxide is known to be a good shock tracer in molecular clouds and protostar environments, but its abundance is difficult to reproduce even using state-of-the-art astroche…

astro-ph.IM2022

Upgrading the high contrast imaging facility SPHERE: science drivers and instrument choices

A. Boccaletti, G. Chauvin, F. Wildi +71

SPHERE+ is a proposed upgrade of the SPHERE instrument at the VLT, which is intended to boost the current performances of detection and characterization for exoplanets and disks. S…

astro-ph.EP2018★ 58 cited

Post conjunction detection of Pictoris b with VLT/SPHERE

A. -M. Lagrange, A. Boccaletti, M. Langlois +102

With an orbital distance comparable to that of Saturn in the solar system, \bpic b is the closest (semi-major axis \,9\,au) exoplanet that has been imaged to orbit a star.…

astro-ph.SR2017★ 54 cited

SPHERE / ZIMPOL observations of the symbiotic system R Aqr. I. Imaging of the stellar binary and the innermost jet clouds

H. M. Schmid, A. Bazzon, J. Milli +40

R Aqr is a symbiotic binary system consisting of a mira variable, a hot companion with a spectacular jet outflow, and an extended emission line nebula. We have used R Aqr as test t…

astro-ph.EP2015★ 146 cited

First light of the VLT planet finder SPHERE. IV. Physical and chemical properties of the planets around HR8799

M. Bonnefoy, A. Zurlo, J. L. Baudino +63

The system of four planets around HR8799 offers a unique opportunity to probe the physics and chemistry at play in the atmospheres of self-luminous young (~30 Myr) planets. We rece…