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A pulse calibration system for the VLBA

Published online by Cambridge University Press:  12 April 2016

A.R. Thompson
Affiliation:
National Radio Astronomy Observatory, Edgemont Road, Charlottesville, VA
D.S. Bagri
Affiliation:
National Radio Astronomy Observatory, Socorro, NM

Abstract

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In pulse calibration of an interferometer a series of short pulses is inserted into the receiver input to produce a spectrum of equi-spaced lines. The use of these for calibration, and the proposed system for the VLBA, are described.

Type
Hardware for Interferometry
Copyright
Copyright © Astronomical Society of the Pacific 1991

References

Clark, T.A., et al. 1985, Precision Geodesy Using the Mark-III Very-Long-Baseline Interferometer System, IEEE Trans. Geosci. Remote Sensing, GE-23, 438449.CrossRefGoogle Scholar
Kellermann, K.I. and Thompson, A.R. 1985, The Very Long Baseline Array, Science, 229, 123130.CrossRefGoogle ScholarPubMed
Swarup, G. and Yang, K.S. 1961, Phase Adjustment of Large Antennas, IEEE Trans. Antennas Propag., AP-9, 7581.CrossRefGoogle Scholar
Thompson, A.R. and Bagri, D.S. 1988, A Pulse Calibration Scheme for the VLBA, VLB Array Memo. No. 622.Google Scholar
Whitney, A.R., et al. 1976, A Very-Long-Baseline Interferometer System for Geodetic Applications, Radio Science, 11, 421432.CrossRefGoogle Scholar