Context. The wind-driven halo is a feature that is observed in images that were delivered by
the latest generation of ground-based instruments that are equipped with an extreme …

We report the results of a∼ 4 yr direct imaging survey of 104 stars to resolve and
characterize circumstellar debris disks in scattered light as part of the Gemini Planet Imager …

We know little about the outermost exoplanets in planetary systems because our detection
methods are insensitive to moderate-mass planets on wide orbits. However, debris discs …

Context. Direct imaging of extrasolar giant planets demands the highest possible contrasts
(ΔH≳ 10 mag) at the smallest angular separations (∼ 0.1 ″) from the star. We present an …

Characterizing 51 Eri b from 1 to 5 μm: A Partly Cloudy Exoplanet - IOPscience This site uses
cookies. By continuing to use this site you agree to our use of cookies. To find out more, see …

Spatially resolved images of debris discs are necessary to determine disc morphological
properties and the scattering phase function (SPF) thatantifies the brightness of scattered …

Aims. We aim to detect planetary companions to young stars with debris disks via the radial
velocity method. Methods. We observed HD 114082 during April 2018–August 2022 as one …

Aims. Uncovering the ingredients and the architecture of planetary systems is a very active
field of research that has fuelled many new theories on giant planet formation, migration …

Aims. We present new optical and near-infrared images of the debris disk around the F-type
star HD 114082 in the Scorpius-Centaurus OB association. We obtained direct imaging …

Context. The occurrence rate of long-period (a≳ 50 au) giant planets around young stars is
highly uncertain since it is not only governed by the protoplanetary disc structure and planet …