The SpHere INfrared Exoplanet (SHINE) project is a 500-star survey performed with
SPHERE on the Very Large Telescope for the purpose of directly detecting new substellar …

Abstract We present JWST Early Release Science coronagraphic observations of the super-
Jupiter exoplanet, HIP 65426b, with the Near-Infrared Camera (NIRCam) from 2 to 5 μm …

The orbital eccentricities of directly imaged exoplanets and brown dwarf companions
provide clues about their formation and dynamical histories. We combine new high-contrast …

Young exoplanets are snapshots of the planetary evolution process. Planets that orbit stars
in young associations are particularly important because the age of the planetary system is …

The direct characterization of exoplanetary systems with high-contrast imaging is among the
highest priorities for the broader exoplanet community. As large space missions will be …

Context. In recent decades, direct imaging has confirmed the existence of substellar
companions (exoplanets or brown dwarfs) on wide orbits (> 10 au) around their host stars. In …

Context. Large surveys with new-generation high-contrast imaging instruments are needed
to derive the frequency and properties of exoplanet populations with separations from~ 5 to …

Even though tens of directly imaged companions have been discovered in the past decades,
the number of directly confirmed multiplanet systems is still small. Dynamical analysis of …

Medium-resolution integral-field spectrographs (IFS) coupled with adaptive-optics such as
Keck/OSIRIS, VLT/MUSE, or SINFONI are appearing as a new avenue for enhancing the …

Context. Directly imaged planets and substellar companions are key targets for the
characterization of self-luminous atmospheres. Their photometric appearance at 4–5 μm is …