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Opacity at the Owens Valley Millimeter Array

Published online by Cambridge University Press:  12 April 2016

Stephen L. Scott  and
David P. Woody
Stephen L. Scott
Affiliation:
Owens Valley Radio Observatory, California Institute of Technology, PO Box 968, Big Pine, Ca 93513
David P. Woody
Affiliation:
Owens Valley Radio Observatory, California Institute of Technology, PO Box 968, Big Pine, Ca 93513

Abstract

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We have measured the opacity at the Owens Valley Millimeter Array with tip curves at frequencies from 95 to 248GHz. These measurements have been interpreted using a model and then scaled to a standard frequency of 100GHz. The unique aspect of this data is the wide range of frequencies covered and the use of receivers with different sideband gain ratios.

Type
Seeing
Information
International Astronomical Union Colloquium , Volume 131: Radio Interferometry: Theory, Techniques, and Applications , 1991 , pp. 119 - 123
Copyright
Copyright © Astronomical Society of the Pacific 1991

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