Surveys of large stellar samples are the prime means through which the prevalence of exoplanets can be derived, and crucial constraints to planet formation models can be set.
SPHERE
SPHERE’s Debris Disk Gallery: Tell-tale Signs Of Dust And Small Bodies In Distant Solar Systems
Observations with the instrument SPHERE at ESO’s Very Large Telescope have produced an unprecedented gallery of “debris disks” in exoplanetary systems. Gaël Chauvin (Max Planck Institute for Astronomy), project scientist […]
A Newborn Planet Observed Sculpting The Dust Around It
Astronomers may have caught a still-forming planet in action, carving out an intricate pattern in the gas and dust that surrounds its young host star.
High-Contrast Imaging: Hide and Seek with Exoplanets
So far, most of the about 5,700 exoplanets have been discovered mainly with radial velocity and transit methods. These techniques are sensitive to planets in close orbits, not being able […]
RISTRETTO: A VLT XAO Design To Reach Proxima Cen b In The Visible
RISTRETTO is the evolution of the original idea of coupling the VLT instruments SPHERE and ESPRESSO lovis_2016a, aiming at High Dispersion Coronagraphy. RISTRETTO is a visitor instrument that should enable […]
The High-contrast Performance of the Keck Planet Imager and Characterizer
The Keck Planet Imager and Characterizer (KPIC), a series of upgrades to the Keck II Adaptive Optics System and Instrument Suite, aims to demonstrate high-resolution spectroscopy of faint exoplanets that […]
Groundbreaking Survey Reveals Secrets Of Planet Birth Around Dozens Of StarsESOGroundbreaking Survey Reveals Secrets Of Planet Birth Around Dozens Of Stars
In a series of studies, a team of astronomers has shed new light on the fascinating and complex process of planet formation. The stunning images, captured using the European Southern […]
First Light of VLT/HiRISE: High-resolution Spectroscopy Of Young Giant Exoplanets
A major endeavor of this decade is the direct characterization of young giant exoplanets at high spectral resolution to determine the composition of their atmosphere and infer their formation processes […]
Compositional Mapping of Europa Using MCMC Modelling of Near-IR VLT/SPHERE and Galileo/NIMS Observations
We present maps of surface composition of Europa’s anti-jovian hemisphere acquired using high spatial resolution IFU multi-spectral data from the SPHERE instrument on the Very Large Telescope (0.95 to 1.65μm) […]
