The SPHERE infrared survey for exoplanets (SHINE)-III. The demographics of young giant exoplanets below 300 au with SPHERE
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 …
SPHERE on the Very Large Telescope for the purpose of directly detecting new substellar …
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 …
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 …
[HTML][HTML] The SPHERE infrared survey for exoplanets (SHINE)-I. Sample definition and target characterization
S Desidera, G Chauvin, M Bonavita, S Messina… - Astronomy & …, 2021 - aanda.org
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 …
to derive the frequency and properties of exoplanet populations with separations from~ 5 to …
Impact of a new H/He equation of state on the evolution of massive brown dwarfs-New determination of the hydrogen burning limit
We explored the impact of the latest equation of state (EOS) for dense hydrogen–helium
mixtures, which takes into account the interactions between hydrogen and helium species …
mixtures, which takes into account the interactions between hydrogen and helium species …
On the mass function, multiplicity, and origins of wide-orbit giant planets
A major outstanding question regarding the formation of planetary systems is whether wide-
orbit giant planets form differently than close-in giant planets. We aim to establish constraints …
orbit giant planets form differently than close-in giant planets. We aim to establish constraints …
Direct imaging and spectroscopy of exoplanets with the ELT/HARMONI high-contrast module
Combining high-contrast imaging with medium-resolution spectroscopy has been shown to
significantly boost the direct detection of exoplanets. HARMONI, one of the first-light …
significantly boost the direct detection of exoplanets. HARMONI, one of the first-light …
Detectability of satellites around directly imaged exoplanets and brown dwarfs
C Lazzoni, S Desidera, R Gratton… - Monthly Notices of …, 2022 - academic.oup.com
Satellites around substellar companions are a heterogeneous class of objects with a variety
of different formation histories. Focusing on potentially detectable satellites around …
of different formation histories. Focusing on potentially detectable satellites around …
SCExAO and keck direct imaging discovery of a low-mass companion around the accelerating f5 star HIP 5319
N Swimmer, T Currie, S Steiger, GM Brandt… - The Astronomical …, 2022 - iopscience.iop.org
We present the direct imaging discovery of a low-mass companion to the nearby
accelerating F star, HIP 5319, using SCExAO coupled with the CHARIS, VAMPIRES, and …
accelerating F star, HIP 5319, using SCExAO coupled with the CHARIS, VAMPIRES, and …
Spectral and orbital characterisation of the directly imaged giant planet HIP 65426 b
AC Cheetham, M Samland, SS Brems… - Astronomy & …, 2019 - aanda.org
HIP 65426 b is a recently discovered exoplanet imaged during the course of the SPHERE-
SHINE survey. Here we present new L′ and M′ observations of the planet from the NACO …
SHINE survey. Here we present new L′ and M′ observations of the planet from the NACO …