Title | The VLA Low-Frequency Sky Survey |
Authors | Cohen, A. S.; Lane, W. M.; Cotton, W. D.; Kassim, N. E.; Lazio, T. J. W.; Perley, R. A.; C ... |
Bibcode | 2007AJ....134.1245C Search ADS ↗ |
Abstract | The VLA Low-frequency Sky Survey (VLSS) has imaged 95% of the 3π sr of sky north of δ = -30° at a frequency of 74 MHz (4 m wavelength). The resolution is 80″ (FWHM) throughout, and the typical rms noise level is langσrang approx 0.1 Jy beam-1. The typical point-source detection limit is 0.7 Jy beam-1, and so far nearly 70,000 sources have been cataloged. This survey used the 74 MHz system ... |
Objects | 68310 Objects Search NED ↙ |