RISTRETTO: a VLT XAO design to reach Proxima Cen b in the visible
N. Blind, M. Shinde, I. Dinis, N. Restori, B. Chazelas, T. Fusco, O., Guyon, J. Kuehn, C. Lovis, P. Martinez, M. Motte, J.-F. Sauvage, A. Spang

TL;DR
The paper presents the design and simulation results of RISTRETTO, a high-contrast, high-resolution spectrograph for the VLT aimed at characterizing nearby exoplanets like Proxima Centauri b in reflected light.
Contribution
It introduces a novel adaptive optics architecture and demonstrates through simulations that RISTRETTO can achieve the required contrast and stability for exoplanet atmospheric characterization.
Findings
Achieves contrast down to 5×10^{-5} at 2λ/D in visible light.
Demonstrates stable closed-loop operation with combined wavefront sensors.
Validates performance with end-to-end simulations including atmospheric effects.
Abstract
RISTRETTO is the evolution of the original idea of coupling the VLT instruments SPHERE and ESPRESSO \cite{lovis_2016a}, aiming at High Dispersion Coronagraphy. RISTRETTO is a visitor instrument that should enable the characterization of the atmospheres of nearby exoplanets in reflected light, by using the technique of high-contrast, high-resolution spectroscopy. Its goal is to observe Prox Cen b and other planets placed at about 35mas from their star, i.e. at =750nm. The instrument is composed of an extreme adaptive optics, a coronagraphic Integral Field Unit, and a diffraction-limited spectrograph (R=140.000, 620-840 nm). We present the RISTRETTO XAO architecture that reach the specification, providing contrasts down to at 2 from the star in the visible, in the presence of atmosphere and low wind effect. This performance is…
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