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The Sydney University Stellar Interferometer (SUSI)

Published online by Cambridge University Press:  19 July 2016

J. Davis
J. Davis*
Affiliation:
Chatterton Astronomy Department, School of Physics, University of Sydney

Abstract

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The Sydney University Stellar Interferometer has been designed and constructed as a two aperture, single ro, long baseline, optical interferometer with wavefront-tilt compensation and dynamic optical path length compensation. Initially it will operate in the blue part of the visual spectrum but provision has been made for the addition of an additional beam-combining system for a second spectral band. The rationale behind the choice of instrumental parameters, the potential developments which have been taken into account in its construction, and the current status of SUSI are outlined.

Keywords

opticalstellarinterferometer
Type
Optical and Infrared Interferometers and Arrays
Information
Symposium - International Astronomical Union , Volume 158: Very High Angular Resolution Imaging , 1994 , pp. 135 - 142
Copyright
Copyright © Kluwer 1994 

References

Bedding, T.R., Robertson, J.G. & Marson, R.G.: 1993, ‘Non-redundant masking with MAPPIT at the Anglo-Australian Telescope’, In these proceedings. Google Scholar
Davis, J.: 1979, ‘The Application of High Angular Resolution Interferometry to the Study of Single Objects in the Visual Region of the Spectrum’, in Proc. I.A.U. Colloquium No. 50: High Angular Resolution Interferometry, ed. Davis, J. & Tango, W.J., Chatterton Astronomy Dept., University of Sydney, 1–1 to 1–27 Google Scholar
Davis, J.: 1992, ‘SUSI's Potential for Binary Star Studies’, in Proc. I.A.U. Colloquium No. 135: Complementary Approaches to Double and Multiple Star Research, ed. McAlister, H.A. & Hartkopf, W.I., Astron. Soc. Pacific. Conference Series, 32, 521–526.Google Scholar
Davis, J. & Tango, W.J.: 1985, ‘The Sydney University 11.4 Metre Stellar Interferometer’, Proc. A.S.A., 6, 34–38.Google Scholar
Davis, J. & Tango, W.J.: 1985, ‘A New Very High Angular Resolution Stellar Interferometer’, Proc. A. S. A., 6, 38–43.Google Scholar
Davis, J. & Tango, W.J.: 1986, ‘New Determination of the Angular Diameter of Sirius’, Nature, 323, 234–235.Google Scholar
Hanbury Brown, R., Davis, J. & Allen, L.R.: 1974, ‘The Angular Diameters of 32 Stars’, Mon. Not. R. astr. Soc., 167, 121–136.Google Scholar
Lawson, P.R. & Booth, A.J.: 1993, ‘The Fringe Tracking Servo in SUSI’, In these proceedings. Google Scholar
McAlister, H.A.: 1979, ‘High Angular Resolution Binary Star Interferometry’, in Proc. I.A.U. Colloquium No. 50: High Angular Resolution Interferometry, ed. Davis, J. & Tango, W.J., Chatterton Astronomy Dept., University of Sydney, 3–1 to 3–16.Google Scholar
McAlister, H.A.: 1985, ‘High Angular Resolution Measurement of Stellar Properties’ in Ann. Rev. Astron. Astrophys., 23, 59–87.Google Scholar
Minard, R.A., Booth, A.J., Tango, W.J. & ten Brummelaar, T.: 1993, ‘An Overview of the SUSI Control System’, In these proceedings. Google Scholar
Shao, M.: 1993, ‘Fringe Visibility and Phase Measurements’, In these proceedings. Google Scholar
Tango, W.J.: 1990, ‘Dispersion in Stellar Interferometry’, Applied Optics, 29, 516–521.Google Scholar
Tango, W.J. and Twiss, R.Q.: 1980, ‘Michelson Stellar Interferometry’, Progress in Optics, XVII, 241–277.Google Scholar
ten Brummelaar, T., Tango, W.J., Davis, J. & Shobbrook, R.R.: 1993, ‘Preliminary Seeing Measurements with SUSI’, In these proceedings. Google Scholar