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Proceedings Paper

Beam combiner studies for the Magdalena Ridge Observatory Interferometer
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Paper Abstract

We present four alternative designs for a near-infrared science beam combiner for the Magdalena Ridge Observatory Interferometer. The candidate designs considered are: (1) a four way pupil-plane combiner, fed by a "fast switchyard" that would be reconfigured at a few minute intervals to select different subsets of six input beams; (2) a four way image-plane combiner, fed by a similar fast switchyard; (3) an eight way pupil plane combiner; and (4) a six way image plane combiner. The criteria by which fully-optimised versions of the designs will be compared include: realistic signal-to-noise and imaging speed, stability and ease of alignment and calibration, cost (including detector costs), and technical and schedule risk to the MROI project.

Paper Details

Date Published: 28 June 2006
PDF: 12 pages
Proc. SPIE 6268, Advances in Stellar Interferometry, 62681R (28 June 2006); doi: 10.1117/12.671174
Show Author Affiliations
Fabien Baron, Cavendish Lab. (United Kingdom)
David F. Buscher, Cavendish Lab. (United Kingdom)
Julien Coyne, Cavendish Lab. (United Kingdom)
Michelle J. Creech-Eakman, New Mexico Institute of Mining and Technology (United States)
Chris A. Haniff, Cavendish Lab. (United Kingdom)
Colby A. Jurgenson, New Mexico Institute of Mining and Technology (United States)
John S. Young, Cavendish Lab. (United Kingdom)


Published in SPIE Proceedings Vol. 6268:
Advances in Stellar Interferometry
John D. Monnier; Markus Schöller; William C. Danchi, Editor(s)

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