RISTRETTO: reflected-light exoplanet spectroscopy at the diffraction limit of the VLT
Christophe Lovis, Nicolas Blind, Bruno Chazelas, Muskan Shinde,, Maddalena Bugatti, Nathana\"el Restori, Isaac Dinis, Ludovic Genolet, Ian, Hughes, Micha\"el Sordet, Robin Schnell, Samuel Rihs, Adrien Crausaz, Martin, Turbet, Nicolas Billot, Thierry Fusco, Benoit Neichel

TL;DR
RISTRETTO is a high-resolution spectrograph designed for the VLT to detect and analyze exoplanets in reflected light, enabling new atmospheric and surface studies of nearby celestial objects.
Contribution
It introduces a novel combination of high-contrast adaptive optics with a high-resolution spectrograph and a specialized coronagraphic IFU, advancing exoplanet characterization capabilities.
Findings
Design phase completed for the spectrograph subsystem.
Preliminary AO front-end design underway.
Innovative coronagraphic IFU with PIAA and 3D-printed microlenses developed.
Abstract
RISTRETTO is a visible high-resolution spectrograph fed by an extreme adaptive optics (AO) system, to be proposed as a visitor instrument on ESO VLT. The main science goal of RISTRETTO is to pioneer the detection and atmospheric characterisation of exoplanets in reflected light, in particular the temperate rocky planet Proxima b. RISTRETTO will be able to measure albedos and detect atmospheric features in a number of exoplanets orbiting nearby stars for the first time. It will do so by combining a high-contrast AO system working at the diffraction limit of the telescope to a high-resolution spectrograph, via a 7-spaxel integral-field unit (IFU) feeding single-mode fibers. Further science cases for RISTRETTO include the study of accreting protoplanets such as PDS70b/c through spectrally-resolved H-alpha emission, and spatially-resolved studies of Solar System objects such as icy moons…
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