A Single-Sideband, Double-Sideband Interferometer Receiver for Radio Astronomy

Details A Single-Sideband, Double-Sideband Interferometer Receiver for Radio Astronomy A Single-Sideband, Double-Sideband Interferometer Receiver for Radio Astronomy

Mar 1967

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1967itap...15..332w&link_type=abstract

IEEE Transactions on Antennas and Propagation, vol. 15, issue 2, pp. 332-333

Astronomy and Astrophysics

Astronomy

1

Scientific paper

At present, two principal types of receivers for interferometers in radio astronomy are in use. The first and older type is the so-called single-sideband (SSB) receiver, in which input noise in one of the two passbands of a mixer receiver is suppressed by an image filter. The second type is the double-sideband (DSB) receiver. It is essentially a mixer type receiver, but now without image suppression. The special character of this type of receiver for interferometry and its inherent simplicity were first discovered at Caltech. [1][2]

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