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Microarcsecond scintillation-induced variability (MASIV) survey of the northern sky
Authors:
D. L. Jauncey a;
J. E. J. Lovell a;
C. Senkbeil b;
S. Shabala c;
H. E. Bignall d;
T. Pursimo e;
R. Ojha f;
M. Dutka f;
J. -P. Macquart g;
B. J. Rickett h;
L. Kedziora-Chudczer i
| Affiliations: | a Australia Telescope National Facility, Epping, NSW, Australia |
| b School of Mathematics and Physics, University of Tasmania, Hobart, Australia | |
| c Cavendish Laboratory, Cambridge, UK | |
| d Joint Institute for VLBI in Europe, Dwingeloo, AA, The Netherlands | |
| e Nordic Optical Telescope, Sta Cruz de La Palma, Tenerife, Spain | |
| f US Naval Observatory, Washington DC, USA | |
| g NRAO Jansky Fellow, Department of Astronomy, California Institute of Technology, Pasadena, CA, USA | |
| h Department of Electrical and Computer Engineering, University of California, San Diego, La Jolla, CA, USA | |
| i School of Physics, University of Sydney, NSW, Australia |
DOI:
10.1080/10556790701596846
Publication Frequency:
6 issues per year
Published in:
Astronomical & Astrophysical Transactions,
Volume
26,
Issue
6
December
2007
, pages 575
- 583
Astronomical & Astrophysical Transactions,
Volume
26,
Issue
6
December
2007
, pages 575
- 583
Subjects:
Astrophysics;
Space Science;
Formats available:
HTML
(English)
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PDF
(English)
The circumstances under which this title is published have changed:
Reason for change: Changed Publisher
Date of change: 2008
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Abstract
We present the results of a large-scale 5-GHz Very Large Array (VLA) survey of the northern sky searching for sources that exhibit intraday variability (IDV). The observations were made over four epochs, each of 3 days in January, May and September 2002 and January 2003. The objective is to obtain a large sample of IDV sources in order to derive reliable statistics of the microarcsecond properties of the source population and the scattering properties of the interstellar medium.
|
| Keywords: IDV; Interstellar medium; VLA survey |
| view references (19) |
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