Poster + Presentation
13 December 2020 Design of a precision calibration unit for Keck NIRC2 AO instrument
Author Affiliations +
Conference Poster
Abstract
High-precision astrometry has the potential to address questions in planet formation, black hole science, Galactic structure, and more. However, in order to achieve a precision of sub-milli arcseconds (mas), we need a calibration method better than the current techniques such as on-sky calibration using calibrated stellar or stellar cluster systems, which have a precision of $sim$ 1 mas. Precision calibration unit with a regular grid of photo-lithographically manufactured pinholes combined with self-calibration techniques, on the other hand, is a new and innovative way to potentially achieve a precision of sub-mas over the entire field of view. This technique is beneficial to adaptive optic (AO) instruments for future telescopes like the Thirty Meter Telescope (TMT). In this work, we present our design for a new astrometric calibration unit to feed the NIRC2 AO instrument at the W. M. Keck Observatory. It allows calibration over a large field of view of $47^{''} times 47^{''}$, spat
Conference Presentation
© (2020) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Zeren Lin, Tarun Kumar, Xun Chen, Jessica Lu, Peter Wizinowich, Scott Lilley, Ed Wetherell, and Nicholas McConnell "Design of a precision calibration unit for Keck NIRC2 AO instrument", Proc. SPIE 11448, Adaptive Optics Systems VII, 1144879 (13 December 2020); https://doi.org/10.1117/12.2561958
Advertisement
Advertisement
RIGHTS & PERMISSIONS
Get copyright permission  Get copyright permission on Copyright Marketplace
KEYWORDS
Adaptive optics

Calibration

Telescopes

Thirty Meter Telescope

Distortion

Keck Observatory

Manufacturing

RELATED CONTENT

NFIRAOS the optical design of an adaptive optics system...
Proceedings of SPIE (September 17 2009)
Exoearth study with TMT
Proceedings of SPIE (July 07 2004)

Back to Top