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327 MHz Observations of 3C 84, 3C 120 and 1148-001

Published online by Cambridge University Press:  03 August 2017

V. K. Kulkarni  and
S. Ananthakrishnan
V. K. Kulkarni
Affiliation:
Radio Astronomy Centre (TIFR), P.O. Box 8, Udhagamandalam - 643001, India
S. Ananthakrishnan
Affiliation:
Radio Astronomy Centre (TIFR), P.O. Box 8, Udhagamandalam - 643001, India

Extract

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We have made VLBI observations of a mixed sample of bright galaxies and quasars at 327 MHz using the Ooty Radio Telescope in India and the telescopes at Jodrell Bank, Westerbork, Torun, and Crimea in December 1983 and March 1986. MK II recording was used and the data were processed at MPI, Bonn. The preliminary results of the 1983 analysis (Ananthakrishnan and Kulkarni 1986) showed most of the nearby galaxies to be resolved over the longest baselines of 8 million wavelengths. The only seyfert galaxies for which good S/N ratio was available at the longest baselines were 3C84 and 3C120. Although UV coverage was poor we attempted to make maps of these objects. The radio source 1148-001 was used for gain calibration of the telescopes.

Type
Extragalactic
Information
Symposium - International Astronomical Union , Volume 129: The Impact of VLBI on Astrophysics and Geophysics , 1988 , pp. 121 - 122
Copyright
Copyright © Reidel 1988 

References

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