AF Lep b: The lowest-mass planet detected by coupling astrometric and direct imaging data
Aims. Using the direct-imaging technique, we searched for low-mass companions around
the star AF Lep, which presents a significant proper-motion anomaly (PMa) signal obtained …
the star AF Lep, which presents a significant proper-motion anomaly (PMa) signal obtained …
SPHERE: the exoplanet imager for the Very Large Telescope
Observations of circumstellar environments that look for the direct signal of exoplanets and
the scattered light from disks have significant instrumental implications. In the past 15 years …
the scattered light from disks have significant instrumental implications. In the past 15 years …
SPHERE: a planet finder instrument for the VLT
JL Beuzit, M Feldt, K Dohlen, D Mouillet… - Ground-based and …, 2008 - spiedigitallibrary.org
Direct detection and spectral characterization of extra-solar planets is one of the most
exciting but also one of the most challenging areas in modern astronomy. The challenge …
exciting but also one of the most challenging areas in modern astronomy. The challenge …
Astrometric accelerations as dynamical beacons: discovery and characterization of HIP 21152 B, the first T-dwarf companion in the Hyades
K Franson, BP Bowler, M Bonavita… - The Astronomical …, 2023 - iopscience.iop.org
Benchmark brown dwarf companions with well-determined ages and model-independent
masses are powerful tools to test substellar evolutionary models and probe the formation of …
masses are powerful tools to test substellar evolutionary models and probe the formation of …
The SPHERE infrared survey for exoplanets (SHINE)-II. Observations, data reduction and analysis, detection performances, and initial results
M Langlois, R Gratton, AM Lagrange… - Astronomy & …, 2021 - aanda.org
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 …
companions (exoplanets or brown dwarfs) on wide orbits (> 10 au) around their host stars. In …
Reference-star differential imaging on SPHERE/IRDIS
Context. Reference-star differential imaging (RDI) is a promising technique in high-contrast
imaging that is thought to be more sensitive to exoplanets and disks than angular differential …
imaging that is thought to be more sensitive to exoplanets and disks than angular differential …
First light of the VLT planet finder SPHERE-III. New spectrophotometry and astrometry of the HR 8799 exoplanetary system
Context. The planetary system discovered around the young A-type HR 8799 provides a
unique laboratory to: a) test planet formation theories; b) probe the diversity of system …
unique laboratory to: a) test planet formation theories; b) probe the diversity of system …
Astrophotonics: astronomy and modern optics
S Minardi, RJ Harris, L Labadie - The Astronomy and Astrophysics Review, 2021 - Springer
Much of the progress in astronomy has been driven by instrumental developments, from the
first telescopes to fiber fed spectrographs. In this review, we describe the field of …
first telescopes to fiber fed spectrographs. In this review, we describe the field of …
Perturbers: SPHERE detection limits to planetary-mass companions in protoplanetary disks
R Asensio-Torres, T Henning, F Cantalloube… - Astronomy & …, 2021 - aanda.org
The detection of a wide range of substructures such as rings, cavities, and spirals has
become a common outcome of high spatial resolution imaging of protoplanetary disks, both …
become a common outcome of high spatial resolution imaging of protoplanetary disks, both …
Near-infrared scattered light properties of the HR 4796 A dust ring-A measured scattering phase function from 13.6° to 166.6°
Context. HR 4796 A is surrounded by a debris disc, observed in scattered light as an
inclined ring with a high surface brightness. Past observations have raised several …
inclined ring with a high surface brightness. Past observations have raised several …