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

Published online by Cambridge University Press:  25 May 2016

Yoshiaki Hagiwara
Affiliation:
The Graduate University for Advanced Studies, Nobeyama Radio Observatory, Nagano 384-13, Japan
K. Fujisawa
Affiliation:
The Institute of Space and Astronautical Science, 3–1–1 Yoshinodai, Sagamihara, Kanagawa 229, Japan
P. Edwards
Affiliation:
The Institute of Space and Astronautical Science, 3–1–1 Yoshinodai, Sagamihara, Kanagawa 229, Japan
H. Hirabayashi
Affiliation:
The Institute of Space and Astronautical Science, 3–1–1 Yoshinodai, Sagamihara, Kanagawa 229, Japan
Y. Murata
Affiliation:
The Institute of Space and Astronautical Science, 3–1–1 Yoshinodai, Sagamihara, Kanagawa 229, Japan
H. Kobayashi
Affiliation:
The Institute of Space and Astronautical Science, 3–1–1 Yoshinodai, Sagamihara, Kanagawa 229, Japan
T. Iwata
Affiliation:
Communications Research Laboratory, Kashima Space Research Center, Ibaraki 314, Japan

Extract

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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).

Type
Chapter 9: Observational Developments
Copyright
Copyright © Kluwer 1996 

References

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