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MAPPIT: Optical Interferometry with Non-Redundant Masks

Published online by Cambridge University Press:  19 July 2016

T. R. Bedding ,
J. G. Robertson  and
R. G. Marson
T. R. Bedding
Affiliation:
School of Physics, University of Sydney 2006, Australia
J. G. Robertson
Affiliation:
School of Physics, University of Sydney 2006, Australia
R. G. Marson
Affiliation:
School of Physics, University of Sydney 2006, Australia

Extract

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MAPPIT (Masked APerture-Plane Interference Telescope) is an optical interferometer mounted at the coudé focus of the 3.9 m Anglo-Australian Telescope. The instrument, shown schematically in Fig. 1, uses a pupil mask with five apertures of diameter ≲r 0. The apertures are arranged in a linear non-redundant array, with the spacings chosen to optimize the spatial frequency coverage (R. G. Marson, these Proceedings).

Type
Aperture Distributions
Information
Symposium - International Astronomical Union , Volume 158: Very High Angular Resolution Imaging , 1994 , pp. 327 - 330
Copyright
Copyright © Kluwer 1994 

References

Bedding, T. R., Robertson, J. G., Marson, R. G., Gillingham, P. R., Frater, R. H., and O'Sullivan, J. D., 1992, in Proc. of the ESO Conference on High-Resolution Imaging by Interferometry II, edited by Beckers, J. M. and Merkle, F., p. 391, Garching bei München, F.R.G., October 1991.Google Scholar
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