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 …

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 …

First light of the VLT planet finder SPHERE-III. New spectrophotometry and astrometry of the HR 8799 exoplanetary system

A Zurlo, A Vigan, R Galicher, AL Maire, D Mesa… - Astronomy & …, 2016 - aanda.org
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 …

Spectral and atmospheric characterization of 51 Eridani b using VLT/SPHERE

M Samland, P Mollière, M Bonnefoy, AL Maire… - Astronomy & …, 2017 - aanda.org
Context. 51 Eridani b is an exoplanet around a young (20 Myr) nearby (29.4 pc) F0-type star,
which was recently discovered by direct imaging. It is one of the closest direct imaging …

The infra-red dual imaging and spectrograph for SPHERE: design and performance

K Dohlen, M Langlois, M Saisse, L Hill… - Ground-based and …, 2008 - spiedigitallibrary.org
The SPHERE (Spectro-Polarimetric High-contrast Exoplanet Research) planet finder
instrument for ESO's VLT telescope, scheduled for first light in 2011, aims to detect giant …

Optical vectorial vortex coronagraphs using liquid crystal polymers: theory, manufacturing and laboratory demonstration

D Mawet, E Serabyn, K Liewer, C Hanot… - Optics …, 2009 - opg.optica.org
In this paper, after briefly reviewing the theory of vectorial vortices, we describe our
technological approach to generating the necessary phase helix, and report results obtained …

Apodized phase mask coronagraphs for arbitrary apertures-ii. comprehensive review of solutions for the vortex coronagraph

A Carlotti, L Pueyo, D Mawet - Astronomy & Astrophysics, 2014 - aanda.org
Context. With a clear circular aperture, the vortex coronagraph perfectly cancels an on-axis
point source and offers a 0.9 or 1.75λ/D inner working angle for topological charge 2 or 4 …

Performance of the VLT Planet Finder SPHERE-II. Data analysis and results for IFS in laboratory

D Mesa, R Gratton, A Zurlo, A Vigan, RU Claudi… - Astronomy & …, 2015 - aanda.org
Aims. We present the performance of the Integral Field Spectrograph (IFS) of SPHERE, the
high-contrast imager for the ESO VLT telescope designed to perform imaging and …

Imaging exoplanets with coronagraphic instruments

R Galicher, J Mazoyer - Comptes …, 2023 - comptes-rendus.academie-sciences …
L'exoplanétologie est un domaine très actif de l'astronomie moderne avec des questions
encore ouvertes: comment les systèmes planétaires se forment-ils et évoluent-ils; pourquoi …

The Gemini NICI Planet-Finding Campaign: The frequency of giant planets around young B and A stars

EL Nielsen, MC Liu, Z Wahhaj, BA Biller… - The Astrophysical …, 2013 - iopscience.iop.org
We have carried out high contrast imaging of 70 young, nearby B and A stars to search for
brown dwarf and planetary companions as part of the Gemini NICI Planet-Finding …