Bibliography #
Paper directly linked to the project #
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(Bugatti et al 2024) The RISTRETTO simulator: exoplanet reflected spectra
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(Motte et al 2024) High-performance AO systems: impact of the chromatic pupil shift in the case of RISTRETTO
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(Lovis et al 2024) RISTRETTO: reflected-light exoplanet spectroscopy at the diffraction limit of the VLT
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(Restori and Blind et al 2024) RISTRETTO: the PIAA Nuller in the prototyping phase
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(Blind et al 2024 RISTRETTO: a VLT XAO for characterising Proxima b in the visible
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(Shinde et al 2024) RISTRETTO: a comparative performance analysis of the unmodulated Pyramid wavefront sensor (PyWFS) and the Zernike wavefront sensor (ZWFS)
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(Shinde et al 2024) Characterizing the performance of C-RED One cameras for implementation in RISTRETTO and SAXO+ projects
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(Chazelas et al 2024); RISTRETTO: Manufacturing of a single-mode visible high resolution spectrograph
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(Lovis et al 2023); RISTRETTO at the VLT: A pathfinder for ELT-ANDES and ELT-PCS
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(Blind et al 2023); RISTRETTO: reaching 1E-4 fiber contrast at 2lbd/D in the visible
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(Shinde et al 2023); Linearizing the unmodulated pyramid wavefront sensor
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(Lovis et al 2022); RISTRETTO: high-resolution spectroscopy at the diffraction limit of the VLT, 2022
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(Blind et al 2022); RISTRETTO: coronagraph and AO designs enabling High Dispersion Coronagraphy at 2 λ/D
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(Chazelas et al 2022); RISTRETTO: Seven Spaxels Single Mode Spectrograph Design
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(Chazelas et al 2020); RISTRETTO: a pathfinder instrument for exoplanet atmosphere characterization, 2020.
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(Lovis 2019), Reflected-light spectroscopy of nearby expoplanets with RISTRETTO at the VLT, The Very Large Telescope in 2030.
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(Lovis, C. et al 2017); Atmospheric characterization of Proxima b by coupling the SPHERE high-contrast imager to the ESPRESSO spectrograph
Scientific paper of interest for this project #
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(Haffert et al 2019); Two accreting protoplanets around the young star PDS 70.
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(Por et al 2018)The Single-mode Complex Amplitude Refinement (SCAR) coronagraph: I. Concept, theory and design
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(Guyon et al 2003) Phase-Induced Amplitude Apodization of Telescope Pupils for Extrasolar Terrestrial Planet Imaging