Orateur
Mlle
Lauren Schatz
(University of Arizona)
Summary
Adaptive optics systems correct atmospheric turbulence in real time. Most adaptive optics
systems used routinely correct in the near infrared, at wavelengths greater than 1$\mu$m. MagAO-X is a new extreme adaptive optics (ExAO) instrument that will offer corrections at visible-to-near-IR wavelengths. MagAO-X will achieve Strehl ratios greater than 70% at H%\alpha$ when running the 2040 actuator deformable mirror at 3.6 kHz. A visible pyramid wavefront sensor (PWFS) optimized for sensing at 600-1000 nm wavelengths will provide the high-order wavefront sensing on MagAO- X. We present the optical design and an update on the alignment of the MagAO-X pyramid wavefront sensor.
Auteur principal
Mlle
Lauren Schatz
(University of Arizona)
Co-auteurs
Alexander Hedglen
(University of Arizona College of Optical Sciences)
Alexander Rodack
(University of Arizona College of Optical Sciences)
Chris Bohlman
(University of Arizona)
Dr
Jared Males
(Unviersity of Arizona Steward Observatory)
Jennifer Lumbres
(University of Arizona College of Optical Sciences)
Joseph Long
(University of Arizona Steward Observatory)
Justin Knight
(University of Arizona College of Optical Sciences)
Kelsey Miller
(University of Arizona College of Optical Sciences)
Kyle Van Gorkom
(University of Arizona College of Optical Sciences)
Prof.
Laird Close
(University of Arizona Steward Observatory)
Madison Jean
(University of Arizona College of Optical Sciences)
Maggie Kautz
(University of Arizona College of Optical Sciences)
Prof.
Michael Hart
(University of Arizona College of Optical Sciences)
Olivier Durney
(University of Arizona Steward Observatory)
Prof.
Olivier Guyon
(Subaru Telescope / University of Arizona)
