During April and May 1993, hours of observations were scheduled. To achieve a flux density limit of 1 mJy (), each field was observed for minutes. The data were taken in spectral-line mode using two 25 MHz bandpasses, each divided into seven 3 MHz channels in two polarizations. The field centers are distributed in the sky in a variable hexagonal grid with an average spacing of 26 arcmin between nearest neighbors. A total of fields were observed in a narrow declination strip 2.75° wide passing through the NGP and spanning in RA.