Showing 21–40 of 79 results
/ Date/ Name
Jul 18, 2018Review of high-contrast imaging systems for current and future ground-based and space-based telescopes III. Technology opportunities and pathwaysOct 28, 2021High contrast imaging wavefront sensor referencing from coronagraphic imagesOct 28, 2021On-sky validation of image-based adaptive optics wavefront sensor referencingJul 2, 2021Phase Retrieval and Design with Automatic DifferentiationMay 12, 20213D-M3: High-spatial resolution spectroscopy with extreme AO and 3D printed micro-lensletsJun 1, 2021Achromatic photonic tricouplers for application in nulling interferometryJan 16, 2023High-angular resolution and high-contrast VLTI observations from Y to L band with the Asgard instrumental suiteAug 3, 2022High Contrast Imaging at the Photon Noise Limit with WFS-based PSF CalibrationSep 11, 2024Spectroscopy using a visible photonic lantern at the Subaru telescope: Laboratory characterization and first on-sky demonstration on Ikiiki (α Leo) and `Aua (α Ori)Jul 9, 2014Gemini Planet imager Observational Calibrations X: Non-Redundant Masking on GPIAug 2, 2018Multiplexed Holographic Aperture Masking with liquid-crystal geometric phase masksAug 10, 2021Full characterization of the instrumental polarization effects of the spectropolarimetric mode of SCExAO-CHARISSep 27, 2021SCExAO, a testbed for developing high-contrast imaging technologies for ELTsAug 3, 2022A Visible-light Lyot Coronagraph for SCExAO/VAMPIRESJul 12, 2019Astro2020: Astrophotonics White PaperDec 1, 2020Calibration of the instrumental polarization effects of SCExAO-CHARIS' spectropolarimetric modeDec 20, 2023Real-time experimental demonstrations of a photonic lantern wavefront sensorJul 22, 2024Visible Photonic Lantern integration, characterization and on-sky testing on Subaru/SCExAOSep 10, 2024Design, scientific goals, and performance of the SCExAO survey for planets around accelerating starsMar 31, 2025Implicit Electric Field Conjugation with the Photonic Lantern Nuller