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Science and technology progress at the Sydney University Stellar Interferometer

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Authors

Robertson, James G
Tango, W J
Tuthill, Peter G
Warrington, B A
Kok, Y
Rizzuto, Aaron C.
Cheetham, Anthony
Jacob, A P
Ireland, Michael

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SPIE - The International Society for Optical Engineering

Abstract

This paper presents an overview of recent progress at the Sydney University Stellar Interferometer (SUSI). Development of the third-generation PAVO beam combiner has continued. The MUSCA beam combiner for high-precision differential astrometry using visible light phase referencing is under active development and will be the subject of a separate paper. Because SUSI was one of the pioneering interferometric instruments, some of its original systems are old and have become difficult to maintain. We are undertaking a campaign of modernization of systems: (1) an upgrade of the Optical Path Length Compensator IR laser metrology counter electronics from a custom system which uses an obsolete single-board computer to a modern one based on an FPGA interfaced to a Linux computer - in addition to improving maintainability, this upgrade should allow smoother motion and higher carriage speeds; (2) the replacement of the aged single-board computer local controllers for the siderostats and the longitudinal dispersion compensator has been completed; (3) the large beam reducing telescope has been replaced with a pair of smaller units with separate accessible foci. Examples of scientific results are also included.

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Proceedings of SPIE - The International Society for Optical Engineering

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Restricted until

2037-12-31