The VLA Low-Frequency Sky Survey (VLSS) is a 74 MHz continuum survey
covering the entire sky north of -30 degrees declination. Using the
VLA in BnA and B-configurations, it will map the entire survey region
at a resolution of 80" and with an average rms noise of 0.1 Jy/beam.
This version include the data from the VLSS redux which increased the coverage
region slightly and substantially improved the data reduction. Details are in the
Lane et al. (2012) reference. Provenance: VLSS Team: R.A. Perley, J.J. Condon, W.D. Cotton (NRAO);
A.S. Cohen, W.M. Lane (NRC/NRL),
N.E. Kassim, T.J.W. Lazio (NRL),
W.C. Erickson (UMd). This is a service of NASA HEASARC.
