Showing 1–16 of 16 results
/ Date/ Name
Mar 12, 2020SPHERE+: Imaging young Jupiters down to the snowlineJul 18, 2018Review of high-contrast imaging systems for current and future ground- and space-based telescopes I. Coronagraph design methods and optical performance metricsDec 16, 2025Why the Northern Hemisphere Needs a 30-40 m Telescope and the Science at Stake. How do Planetary Systems Form?May 16, 2022Towards on-sky adaptive optics control using reinforcement learningJul 15, 2020CS Cha B: A disc-obscured M-type star mimicking a polarised planetary companionMar 24, 2023Implicit electric field Conjugation: Data-driven focal plane controlMar 28, 2018The Single-mode Complex Amplitude Refinement (SCAR) coronagraph: I. Concept, theory and designMar 28, 2018The Single-mode Complex Amplitude Refinement (SCAR) coronagraph: II. Lab verification, and toward the characterization of Proxima bApr 11, 2021Fundamental limit of single-mode integral-field spectroscopyApr 22, 2021The vector-apodizing phase plate coronagraph: design, current performance, and future developmentMar 20, 2025Making the unmodulated pyramid wavefront sensor smart II. First on-sky demonstration of extreme adaptive optics with deep learningJun 4, 2019Two accreting protoplanets around the young star PDS 70Jun 3, 2021A MUSE view of the asymmetric jet from HD 163296Nov 23, 2021Accreting protoplanets: Spectral signatures and magnitude of gas and dust extinction at H alphaNov 16, 2020Searching for proto-planets with MUSEAug 21, 2025Adding colour to the Zernike wavefront sensor: Advantages of including multi-wavelength measurements for wavefront reconstruction