Paper
21 February 2003 Status of the SUSI program
Author Affiliations +
Abstract
SUSI -- the Sydney University Stellar Interferometer -- currently operates with a maximum baseline of 160 m. A major upgrade which will see the sensitivity of the instrument increased by a factor of 50 is nearly complete, and first fringes have been obtained with the new red beam-combining system.
© (2003) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
William J. Tango "Status of the SUSI program", Proc. SPIE 4838, Interferometry for Optical Astronomy II, (21 February 2003); https://doi.org/10.1117/12.459975
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Cited by 2 scholarly publications.
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KEYWORDS
Mirrors

Interferometers

Beam splitters

Sensors

Telescopes

Adaptive optics

Avalanche photodetectors

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