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The NRAO VLA Sky Survey

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Condon, J. J., Cotton, W. D., Greisen, E. W., Yin, Q. F., Perley, R. A., Taylor, G. B., Broderick, J. J.·1998·The Astronomical Journal

Abstract

The NRAO VLA Sky Survey (NVSS) covers the sky north of J2000.0 δ = -40° (82% of the celestial sphere) at 1.4 GHz. The principal data products are (1) a set of 2326 4° × 4° continuum "cubes" with three planes containing Stokes I , Q , and U images plus (2) a catalog of almost 2 × 10 6 discrete sources stronger than S ≈ 2.5 mJy. The images all have θ = 45'' FWHM resolution and nearly uniform sensitivity. Their rms brightness fluctuations are σ ≈ 0.45 mJy beam -1 ≈ 0.14 K (Stokes I ) and σ ≈ 0.29 mJy beam -1 ≈ 0.09 K (Stokes Q and U ). The rms uncertainties in right ascension and declination vary from ≲1'' for the N ≈ 4 × 10 5 sources stronger than 15 mJy to 7'' at the survey limit. The NVSS was made as a service to the astronomical community. All data products, user software, and updates are being released via the World Wide Web as soon as they are produced and verified.

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Metadata

Authors
Condon, J. J., Cotton, W. D., Greisen, E. W., Yin, Q. F., Perley, R. A., Taylor, G. B., & Broderick, J. J.
Venue
The Astronomical Journal
Published
1998-05
Volume
115
Issue
5
Pages
1693-1716
ISSN
0004-6256 (ISSN-L)
OpenAlex
W1966667130
Cited by
5,760
References
0
FWCI
97.51
Type
journal article
Language
en
Open access
bronze

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CoChat. (2026). Citation check: The NRAO VLA Sky Survey. https://app.cochat.ai/papers/10.1086/300337
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Condon, J. J., Cotton, W. D., Greisen, E. W., Yin, Q. F., Perley, R. A., Taylor, G. B., & Broderick, J. J. (1998). The NRAO VLA Sky Survey. The Astronomical Journal. https://doi.org/10.1086/300337

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