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The VSOP project: Space VLBI Imaging of AGN at 1.6 and 5 GHz

Published online by Cambridge University Press:  13 May 2016

Y. Murata
Affiliation:
Institute of Space and Astronautical Science, 3-1-1 Yoshinodai, Sagamihara, Kanagawa 229-8510, Japan
H. Hirabayashi
Affiliation:
Institute of Space and Astronautical Science, 3-1-1 Yoshinodai, Sagamihara, Kanagawa 229-8510, Japan
P.G. Edwards
Affiliation:
Institute of Space and Astronautical Science, 3-1-1 Yoshinodai, Sagamihara, Kanagawa 229-8510, Japan

Abstract

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The VLBI Space Observatory Programme (VSOP) combines an orbiting radiotelescope with arrays of ground radio telescopes to extend the Very Long Baseline Interferometry (VLBI) technique to baselines up to almost three Earth diameters. In this paper, we present results from VSOP observations of active galactic nuclei (AGN) at 1.6 and 5 GHz from the first 3.5 years of the mission.

Type
The Inner Regions of Galaxies
Copyright
Copyright © Astronomical Society of the Pacific 2001 

References

N.B. APRSV2000 denotes Astrophysical Phenomena Revealed by Space VLBI, ed. Hirabayashi, H., Edwards, P. G. & Murphy, D. W. (Sagamihara: ISAS).Google Scholar
Asada, K., Kameno, S., Inoue, M. et al. 2000, in APRSV2000 p. 51.Google Scholar
Bower, G.C. & Backer, D.C. 1998, ApJ, 507, L117.Google Scholar
Edwards, P.G., Giovannini, G., Cotton, W.D. et al. 2000, PASJ, 52, in press.Google Scholar
Gabuzda, D. 1999, New Astronomy Reviews, 43, 691.CrossRefGoogle Scholar
Gurvits, L.I., Frey, S., Schilizzi, R.T. et al. 2000, Adv. Space Res., 26, 719.Google Scholar
Hirabayashi, H., Hirosawa, H., Kobayashi, H., et al. 1998, Science, 281, 1825 and erratum 282, 1995.CrossRefGoogle Scholar
Hirabayashi, H., Hirosawa, H., Kobayashi, H. et al. 2000a, PASJ, 52, in press.Google Scholar
Hirabayashi, H., Fomalont, E.B., Horiuchi, S., et al. 2000b, PASJ, 52, in press.Google Scholar
Jones, D.L., Wehrle, A.E., Piner, B.G. et al. 2000, in APRSV2000, p. 71.Google Scholar
Junor, W., Biretta, J.A., Owen, F.N. & Begelman, M.C. 2000, in APRSV2000 p. 13.Google Scholar
Kameno, S., Sawada-Satoh, S., Shibata, K. et al. 2000a, in APRSV2000, p. 87.Google Scholar
Kameno, S., Horiuchi, S., Shen, Z.-Q., Inoue, M., et al. 2000b, PASJ, 52, 209.Google Scholar
Kellermann, K.I. & Pauliny-Toth, I.I.K. 1969, ApJ, 155, L71.CrossRefGoogle Scholar
Kemball, A., Flatters, C., Gabuzda, D., et al. 2000, PASJ, 52, in press.Google Scholar
Kobayashi, H., Wajima, K., Hirabayashi, H. et al. 2000 PASJ, 52, in press.Google Scholar
Lovell, J.E.J., Tingay, S.J., Piner, B.G. et al. 2000, in APRSV2000, p. 215.Google Scholar
Murata, Y., Hirabayashi, H., Kobayashi, H., et al. 2000, in Radio Telescopes, ed. Butcher, H.R., Proc. of SPIE Vol 4015, p. 204.CrossRefGoogle Scholar
Murphy, D.W., Preston, R.A., Polatidis, A. et al. 2000, in APRSV2000, p. 47.Google Scholar
Piner, B.G., Edwards, P.G., Wehrle, A.E. et al. 2000, ApJ, 537, 91.Google Scholar
Preston, R.A., Lister, M.L., Tingay, S.J. et al. 2000, in APRSV2000, p. 199.Google Scholar
Reid, M. et al. 2000, in preparation.Google Scholar
Schwartz, D.A. et al. 2000, ApJ, 540, L69.CrossRefGoogle Scholar
Shen, Z.-Q., Edwards, P.G., Lovell, J.E.J. et al. 1999, PASJ, 51, 513.Google Scholar
Snellen, I., Tschager, W., Schilizzi, R. et al. 2000, in APRSV2000, p. 79.Google Scholar
Sudou, H., Taniguchi, Y., Ohyama, Y. et al. 2000, PASJ, 52, in press.Google Scholar
Tingay, S.J., Jauncey, D.L., Reynolds, J.E. et al. 2000, Adv. Sp. Res., 26, 677.CrossRefGoogle Scholar