Abstract

The Cambridge Low Frequency Synthesis Telescope has been used at 151 MHz to survey three regions centred at RA 10h05m, Dec. 53°54′, RA 10h42m, Dec. 57°36′ and RA 13h32m, Dec. 38°10′, each of area 7.3×7.3 cosec δ deg2. The resolution is 70×70 cosec δ arcsec2, and the rms noise on the maps is typically 15 mJy beam−1. We present positions and flux densities for 2381 sources which have signal-to-noise ratios >5.5.

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