Filling in the Gaps in the 4.85 GHz Sky
arXiv:0907.0788 · doi:10.1088/0004-6256/138/4/1032
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 WMAP point source catalog and on the survey's effectiveness at supplementing the CRATES sky coverage.
13 pages, 3 figures, 2 tables. Accepted for publication in the Astronomical Journal. Tables available in electronic form: http://astro.stanford.edu/gaps/
References in corpus (6)
- Three-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Temperature Analysis
- CRATES: An All-Sky Survey of Flat-Spectrum Radio Sources
- Bright AGN Source List from the First Three Months of the Fermi Large Area Telescope All-Sky Survey
- CGRaBS: An All-Sky Survey of Gamma-Ray Blazar Candidates
- The Wilkinson Microwave Anisotropy Probe (WMAP) Source Catalog
- Multi-frequency measurements of the NVSS foreground sources in the Cosmic Background Imager fields. I. Data release
Cited by in corpus (8)
- Nine-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Final Maps and Results
- The Second Catalog of Active Galactic Nuclei Detected by the Fermi Large Area Telescope
- The Fourth Catalog of Active Galactic Nuclei Detected by the Fermi Large Area Telescope
- The C-Band All-Sky Survey (C-BASS): Constraining diffuse Galactic radio emission in the North Celestial Pole region
- A powerful (and likely young) radio-loud quasar at z=5.3
- One Centimetre Receiver Array-prototype observations of the CRATES sources at 30 GHz
- The C-Band All-Sky Survey (C-BASS): Total intensity point-source detection over the northern sky
- Simulations and Observations of the Microwave Universe