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      Liger for Next Generation Keck Adaptive Optics: Opto-Mechanical Dewar for Imaging Camera and Slicer

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          Abstract

          Liger is a next generation adaptive optics (AO) fed integral field spectrograph (IFS) and imager for the W. M. Keck Observatory. This new instrument is being designed to take advantage of the upgraded AO system provided by Keck All-Sky Precision Adaptive-optics (KAPA). Liger will provide higher spectral resolving power (R\(\sim\)4,000-10,000), wider wavelength coverage (\(\sim\)0.8-2.4 \(\mu\)m), and larger fields of view than any current IFS. We present the design and analysis for a custom-made dewar chamber for characterizing the Liger opto-mechanical system. This dewar chamber is designed to test and assemble the Liger imaging camera and slicer IFS components while being adaptable for future experiments. The vacuum chamber will operate below \(10^{-5}\) Torr with a cold shield that will be kept below 90 K. The dewar test chamber will be mounted to an optical vibration isolation platform and further isolated from the cryogenic and vacuum systems with bellows. The cold head and vacuums will be mounted to a custom cart that will also house the electronics and computer that interface with the experiment. This test chamber will provide an efficient means of calibrating and characterizing the Liger instrument and performing future experiments.

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          Author and article information

          Journal
          02 April 2021
          Article
          10.1117/12.2563028
          2104.01228
          a06c2365-3150-44c4-bd75-72dc27c76696

          http://creativecommons.org/licenses/by/4.0/

          History
          Custom metadata
          Proc. SPIE 11447, Ground-based and Airborne Instrumentation for Astronomy VIII, 1144758, (December 13, 2020)
          8 pages, 6 figures
          astro-ph.IM

          Instrumentation & Methods for astrophysics
          Instrumentation & Methods for astrophysics

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