The Angular Size Distribution of μJy Radio Sources

We made two new sensitive (rms noise μ Jy beam −1 ) high-resolution ( θ  = 3.″0 and θ  = 0.″66 FWHM) S-band (2 

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Bibliographic Details
Published in:The Astrophysical journal 2018-03, Vol.856 (1), p.67
Main Authors: Cotton, W. D., Condon, J. J., Kellermann, K. I., Lacy, M., Perley, R. A., Matthews, A. M., Vernstrom, T., Scott, Douglas, Wall, J. V.
Format: Article
Language:English
Subjects:
Astrophysics
Diameters
Galaxies
Image detection
Image resolution
Noise sensitivity
Radio
Radio telescopes
Role models
Size distribution
Star & galaxy formation
Star formation
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Description
Summary:We made two new sensitive (rms noise μ Jy beam −1 ) high-resolution ( θ  = 3.″0 and θ  = 0.″66 FWHM) S-band (2 
ISSN:0004-637X
1538-4357
DOI:10.3847/1538-4357/aaaec4