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Radio Observations of the γ-Ray Blazar 0528+134

Published online by Cambridge University Press:  25 May 2016

M. Pohl ,
W. Reich ,
T. P. Krichbaum ,
K. Standke ,
S. Britzen ,
H. P. Reuter ,
P. Reich ,
R. Schlickeiser ,
H. Ungerechts  and
R. L. Fiedler
...Show all authors
M. Pohl
Affiliation:
1 MPE, Postfach 1603, 85740 Garching, Germany
W. Reich
Affiliation:
2 MPIfR, Postfach 2024, 53010 Bonn, Germany
T. P. Krichbaum
Affiliation:
2 MPIfR, Postfach 2024, 53010 Bonn, Germany
K. Standke
Affiliation:
2 MPIfR, Postfach 2024, 53010 Bonn, Germany
S. Britzen
Affiliation:
2 MPIfR, Postfach 2024, 53010 Bonn, Germany
H. P. Reuter
Affiliation:
2 MPIfR, Postfach 2024, 53010 Bonn, Germany
P. Reich
Affiliation:
2 MPIfR, Postfach 2024, 53010 Bonn, Germany
R. Schlickeiser
Affiliation:
2 MPIfR, Postfach 2024, 53010 Bonn, Germany
H. Ungerechts
Affiliation:
4 IRAM, Ave. Divina Pastora 7, 18012 Granada, Spain
R. L. Fiedler
Affiliation:
5 NRL, Code 7210, Washington, DC 20375-5351, USA
E. B. Waltman
Affiliation:
5 NRL, Code 7210, Washington, DC 20375-5351, USA
K. J. Johnston
Affiliation:
6 US Naval Obs., Washington, DC 20392-5420, USA
F. D. Ghigo
Affiliation:
7 NRAO, P.O. Box 2, Green Bank, WV 24944, USA

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We report multifrequency observations of the γ-ray blazar 0528+134 with the Effelsberg 100-m telescope, the IRAM 30-m telescope at Pico Veleta and the NRL Green Bank Interferometer. The observing methods are described elsewhere (Reich et al., 1993; Pohl et al., 1995). The radio lightcurves are given in Fig.1 in comparison to the status of 0528+134 in the EGRET energy range. The uncertainties in the flux densities quoted there are less than 5% at 10.55 GHz and lower frequencies, while slightly exceeding this value at 32 GHz and 86 GHz.

Type
Properties of Radio Sources
Information
Symposium - International Astronomical Union , Volume 175: Extragalactic Radio Sources , 1996 , pp. 14 - 16
Copyright
Copyright © Kluwer 1996 

References

Krichbaum, T.P., Britzen, S., Standke, K.J. et al.: 1995, in Quasars and AGN: High Resolution Radio Imaging , Eds. Cohen, M. and Kellermann, K., Proc. Nat. Acad. Sci. USA, in press Google Scholar
McNaron-Brown, K., Johnson, W.N., Jung, G.V. et al., 1995, ApJ 451,575 CrossRefGoogle Scholar
Mücke, A., Pohl, M., Reich, P. et al., 1996, Proceedings of the 3rd Compton Symposium , A&AS submitted Google Scholar
Pohl, M., Reich, W., Krichbaum, T.P. et al., 1995, A&A 303, 383 Google Scholar
Reich, W., Steppe, H., Schlickeiser, R. et al., 1993, A&A 273, 65 Google Scholar
Valtaoja, E., Teräsranta, H., 1995, A&A 297, L13 Google Scholar
Zhang, Y.F., Marscher, A.P., Aller, H.D. et al., 1995, ApJ 432, 91 CrossRefGoogle Scholar