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Multi-epoch, Dual-Frequency VLBI Observations Of PKS 1830-211 From Japan

  • Yoshiaki Hagiwara (a1), K. Fujisawa (a2), P. Edwards (a2), H. Hirabayashi (a2), Y. Murata (a2), H. Kobayashi (a2) and T. Iwata (a3)...

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PKS 1830-211 is a strong, flat-spectrum compact double source with a component spacing of 1 arcsecond. Observations of PKS 1830-211 were made with the Japanese domestic VLBI network at 2.3 GHz and 8.4 GHz bands in sessions between December 1991 and November 1994. The Usuda 64 m (ISAS) and Kashima 34 m (CRL) telescopes were used for all observations, and were used in conjunction with the Mizusawa 10 m (NAO) for observations in 1994. In addition, the total flux was measured with the Usuda 64 m at both bands. Data was recorded using K3 and K4 formatters and recorders, and correlated with NAOCO (the New Advanced One-unit COrrelator of the National Astronomical Observatory).

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Copyright

References

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Fujisawa, K., 1992, , (unpublished).
Hagiwara, Y., 1995, , (unpublished).
Jones, D., et al., 1995, these proceedings.
van Ommen, T.D. et al., 1995, ApJ, 444, 561.

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