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Proceedings Paper

Optical performance of the GHOST fiber cable
Author(s): Ross Zhelem; Vladimir Churilov; Scott Case; Yuriy Kondrat; Kristin Fiegert; Lewis Waller; Jon Lawrence; Tony Farrell; Michael Ireland
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Paper Abstract

The Gemini High-resolution Optical SpecTrograph (GHOST) is fed by an optical cable linking the telescope and environmentally stabilized spectrograph room. Telescope input is injected into integral field units that are translated along the focal surface by positioners. Each integral field unit serves as an image slicer partitioning the seeing limited image with the help of a hexagonal microlens array. An additional microlens array is used to inject light telecentrically into each fiber which maximizes the efficiency of the cable. Spectral measurements of the optical cable throughput are presented for the design wavelength range.

Paper Details

Date Published: 6 January 2020
PDF: 2 pages
Proc. SPIE 11203, Advances in Optical Astronomical Instrumentation 2019, 1120318 (6 January 2020); doi: 10.1117/12.2539924
Show Author Affiliations
Ross Zhelem, Macquarie Univ. (Australia)
Vladimir Churilov, Macquarie Univ. (Australia)
Scott Case, Macquarie Univ. (Australia)
Yuriy Kondrat, Macquarie Univ. (Australia)
Kristin Fiegert, Mount Stromlo Observatory (Australia)
Lewis Waller, Macquarie Univ. (Australia)
Jon Lawrence, Macquarie Univ. (Australia)
Tony Farrell, Macquarie Univ. (Australia)
Michael Ireland, Mount Stromlo Observatory (Australia)


Published in SPIE Proceedings Vol. 11203:
Advances in Optical Astronomical Instrumentation 2019
Simon C. Ellis; Céline d'Orgeville, Editor(s)

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