Poster
19 July 2024 Liger at W.M. Keck Observatory: assembly, integration, and testing
Aaron M. Brown, Shelley Wright, James Wiley, Maren Cosens, Renate Kupke, Marc Kassis, Rosalie McGurk, Sherry Yeh, James Larkin, Michael Fitzgerald, Eric Wang, Evan Kress, Ken Magnone, Chris Johnson, Tucker Jones
Author Affiliations +
Conference Poster
Abstract
Liger is an adaptive optics (AO)-fed imager and integral field spectrograph (IFS) designed for W.M. Keck Observatory. This paper will discuss the assembly, integration, and testing (AIT) of the Liger instrument. The project is currently in the first of two-fabrication phases where we are manufacturing, assembling, and testing the complete imager system, the IFS camera TMA, grating turret mechanism, and the IFS re-imaging optics mechanisms. The second fabrication phase will include the final fabrication and assembly of the IFS and science cryostat. An integration phase will follow where the full instrument is assembled and integrated into the science cryostat. Once complete the Liger will be shipped to Hawaii for final assembly, integration, and verification at W.M. Keck Observatory.
© (2024) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Aaron M. Brown, Shelley Wright, James Wiley, Maren Cosens, Renate Kupke, Marc Kassis, Rosalie McGurk, Sherry Yeh, James Larkin, Michael Fitzgerald, Eric Wang, Evan Kress, Ken Magnone, Chris Johnson, and Tucker Jones "Liger at W.M. Keck Observatory: assembly, integration, and testing", Proc. SPIE 13096, Ground-based and Airborne Instrumentation for Astronomy X, 130967I (19 July 2024); https://doi.org/10.1117/12.3020784
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