RESOLVING THE RADIO SOURCE BACKGROUND: DEEPER UNDERSTANDING THROUGH CONFUSION

@article{Condon2012RESOLVINGTR,
  title={RESOLVING THE RADIO SOURCE BACKGROUND: DEEPER UNDERSTANDING THROUGH CONFUSION},
  author={James J. Condon and William D. Cotton and Edward B. Fomalont and Kenneth I. Kellermann and Neil A. Miller and Richard A. Perley and Douglas Scott and T. Vernstrom and Jasper V. Wall},
  journal={The Astrophysical Journal},
  year={2012},
  volume={758}
}
We used the Karl G. Jansky Very Large Array to image one primary beam area at 3 GHz with 8″ FWHM resolution and 1.0 μJy beam−1 rms noise near the pointing center. The P(D) distribution from the central 10 arcmin of this confusion-limited image constrains the count of discrete sources in the 1 < S(μJy) < 10 range. At this level, the brightness-weighted differential count S2n(S) is converging rapidly, as predicted by evolutionary models in which the faintest radio sources are star-forming… 

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