Published October 2009
| Published
Journal Article
Open
Filling in the Gaps in the 4.85 GHz Sky
Chicago
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Abstract
We describe a 4.85 GHz survey of bright, flat-spectrum radio sources conducted with the Effelsberg 100 m telescope in an attempt to improve the completeness of existing surveys, such as CRATES. We report the results of these observations and of follow-up 8.4 GHz observations with the VLA of a subset of the sample. We comment on the connection to the Wilkinson Microwave Anisotropy Probe point source catalog and on the survey's effectiveness at supplementing the CRATES sky coverage.
Additional Information
© 2009 The American Astronomical Society. Received 2009 April 7; accepted 2009 July 2; published 2009 August 26. Data in this paper are based on observations with the 100 m telescope of the MPIfR (Max-Planck-Institut fur Radioastronomie) at Effelsberg. The National Radio Astronomy Observatory is operated by Associated Universities, Inc., under cooperative agreement with the National Science Foundation. S.E.H. was supported by SLAC under DOE contract DE-AC03-76SF00515.Attached Files
Published - Healey2009p5976Astron_J.pdf
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Additional details
- Eprint ID
- 16140
- Resolver ID
- CaltechAUTHORS:20091001-092815973
- NSF
- Department of Energy (DOE)
- DE-AC03-76SF00515
- Stanford Linear Accelerator Center
- Created
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2009-10-06Created from EPrint's datestamp field
- Updated
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2021-11-08Created from EPrint's last_modified field