A receiver system for a very-long-baseline radio interferometer

Details A receiver system for a very-long-baseline radio interferometer A receiver system for a very-long-baseline radio interferometer

Aug 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976pazh....2..410m&link_type=abstract

(Pis'ma v Astronomicheskii Zhurnal, vol. 2, Aug. 1976, p. 410-415.) Soviet Astronomy Letters, vol. 2, July-Aug. 1976, p. 159-161

Astronomy and Astrophysics

Astronomy

2

Radio Astronomy, Radio Interferometers, Radio Receivers, Frequency Stability, Radio Sources (Astronomy), Signal Reception

Scientific paper

A VLBI receiver capable of independent signal recording at a wavelength of 1.35 cm has been developed. The system noise temperature at the zenith is approximately 70 K. The local-oscillator signal is supplied by a hydrogen frequency standard with a stability better than approximately 10 to the -13th power. Spectra of the radio sources W49 and Orion A have been recorded at 15-kHz resolution.

Affiliated with

Also associated with

No associations

Rating

A receiver system for a very-long-baseline radio interferometer does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with A receiver system for a very-long-baseline radio interferometer, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and A receiver system for a very-long-baseline radio interferometer will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1873315