Liger for Next Generation Keck AO: Filter Wheel and Pupil Design
Maren Cosens (1, 2), Shelley A. Wright (1, 2), Pauline Arriaga, (3, 4), Aaron Brown (2), Michael Fitzgerald (3), Tucker Jones (5), Marc, Kassis (6), Evan Kress (3), Renate Kupke (7), James E. Larkin (3), Jim Lyke, (6), Eric Wang (3), James Wiley (1, 2)

TL;DR
Liger is a versatile next-generation near-infrared imager and spectrograph for Keck Observatory, featuring upgradeable filter wheels and pupil masks to optimize adaptive optics observations over a broad wavelength range.
Contribution
This paper presents the innovative design of filter wheels and pupil masks for Liger, enabling future upgrades and optimized performance in adaptive optics imaging and spectroscopy.
Findings
Design allows for future filter upgrades.
Pupil masks can be added or changed easily.
Fixed masks offer near-ideal performance with simpler mechanics.
Abstract
Liger is a next-generation near-infrared imager and integral field spectrograph (IFS) for the W.M. Keck Observatory designed to take advantage of the Keck All-Sky Precision Adaptive Optics (KAPA) upgrade. Liger will operate at spectral resolving powers between R4,000 - 10,000 over a wavelength range of 0.8-2.4m. Liger takes advantage of a sequential imager and spectrograph design that allows for simultaneous observations between the two channels using the same filter wheel and cold pupil stop. We present the design for the filter wheels and pupil mask and their location and tolerances in the optical design. The filter mechanism is a multi-wheel design drawing from the heritage of the current Keck/OSIRIS imager single wheel design. The Liger multi-wheel configuration is designed to allow future upgrades to the number and range of filters throughout the life of the instrument.…
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