Poster + Paper
29 August 2022 The Large Fiber Array Spectroscopic Telescope: fiber feed and spectrometer conceptual design
Chad F. Bender, J. Roger Angel, Joel Berkson, Peter Gray, Samuel Halverson, Hyukmo Kang, Daewood Kim, Andy Monson, Chang Jin Oh, Matthew Rademacher, Christian Schwab, Andrew Young, Dennis Zaritsky
Author Affiliations +
Conference Poster
Abstract
The Large Fiber Array Spectroscopic Telescope, LFAST, will use optical fibers to combine light from thousands of small telescopes at centrally located high-resolution spectrometers. LFAST aims to use mass replication of small, self-contained telescope systems to provide ELT sized collecting area and spectroscopic capabilities at a drastically reduced price. However, fundamental constraints such as étendue, fiber modal noise, and focal-plane sampling that affect the size and complexity of spectrometers for single telescope ELTs also impact LFAST. We are carrying out a three year study to tackle these challenges. In this paper, we describe the conceptual designs for the fiber feed assemblies that carry light from the individual telescopes to a centralized location, and the high-resolution spectrometer that accepts this light.
© (2022) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Chad F. Bender, J. Roger Angel, Joel Berkson, Peter Gray, Samuel Halverson, Hyukmo Kang, Daewood Kim, Andy Monson, Chang Jin Oh, Matthew Rademacher, Christian Schwab, Andrew Young, and Dennis Zaritsky "The Large Fiber Array Spectroscopic Telescope: fiber feed and spectrometer conceptual design", Proc. SPIE 12184, Ground-based and Airborne Instrumentation for Astronomy IX, 121844J (29 August 2022); https://doi.org/10.1117/12.2628710
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KEYWORDS
Telescopes

Spectroscopy

Optical instrument design

Mirrors

Prototyping

Relays

Spectrometer engineering

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