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The VSOP 5 GHz Active Galactic Nucleus Survey. II. Data Calibration and Imaging

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Authors
Lovell, J.
Moellenbrock, G.
Horiuchi, S.
Fomalont, E.
Scott, W.
Hirabayashi, H.
Dodson, R.
Dougherty, S.
Edwards, P.
Frey, S.
Gurvits, L.
Lister, M.
Murphy, D.
Paragi, Z.
Piner, B.
Shen, Z.
Taylor, A.
Tingay, Steven
Asaki, Y.
Moffett, D.
Murata, Y.
Date
2004
Type
Journal Article
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Abstract

The VLBI Space Observatory Programme (VSOP) mission is a Japanese-led project to study radio sources with sub-milliarcsecond angular resolution using an orbiting 8 m telescope, HALCA, and global arrays of Earth-based telescopes. Approximately 25% of the observing time has been devoted to a survey of compact active galactic nuclei (AGNs) at 5 GHz that are stronger than 1 Jy-the VSOP AGN Survey. This paper, the second in a series, describes the data calibration, source detection, self-calibration, imaging, and modeling and gives examples illustrating the problems specific to space VLBI. The VSOP Survey Web site, which contains all results and calibrated data, is described.

Citation
Lovell, J and Moellenbrock, G and Horiuchi, S and Fomalont, E and Scott, W and Hirabayashi, H and Dodson, R et al. 2004. The VSOP 5 GHz Active Galactic Nucleus Survey. II. Data Calibration and Imaging. The Astrophysical Journal. 155 (1): pp. 27-31.
Source Title
The Astrophysical Journal
URI
DOI
Faculty
Faculty of Science and Engineering
Curtin Institute of Radio Astronomy
Remarks

Copyright © 2004 The American Astronomical Society ("AAS")-[The Astrophysical Journal (ApJ) Lovell, 2004 ApJS 155 (1), 27-31.]

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