Near Infrared (1To5 µm) Multichannel Speckle Interferameter

M J Selby; K Jason; D Xin; C Sanchez

doi:10.1117/12.966132

9 January 1984 Near Infrared (1To5 µm) Multichannel Speckle Interferameter

M J Selby, K Jason, D Xin, C Sanchez

Proceedings Volume 0445, Instrumentation in Astronomy V; (1984) https://doi.org/10.1117/12.966132
Event: 1983 Astronomy Conferences, 1983, London, United Kingdom

Abstract

Speckle interferometry was first introduced by Labeyrie (1970) in the visible as a method of restoring diffraction-limited information from large telescopes despite the presence of a turbulent atmosphere. It has been extensively used in the visible to resolve small sources and measure binary separations (Bonneau and Foy, 1980; McAllister and Hendry, 1982; Beddoes et al, 1976; Morgan et al, 1978).

Citation Download Citation

M J Selby, K Jason, D Xin, and C Sanchez "Near Infrared (1To5 µm) Multichannel Speckle Interferameter", Proc. SPIE 0445, Instrumentation in Astronomy V, (9 January 1984); https://doi.org/10.1117/12.966132

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