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The 7C survey of radio sources at 151 MHz - 33 regions in the range RA 7-17 h, Dec. 30-58 deg
The Cambridge Low Frequency Synthesis Telescope has been used at 151 MHz to survey 33 regions. The resolution is 70 x 70 cosec delta sq arcsec, and the rms noise is typically 25 mJy/beam. We present positions and flux densities for about 15000 sources that have signal-to-noise ratios above 5.5. Thes...
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Published in: | Monthly notices of the Royal Astronomical Society 1999-06, Vol.306 (1), p.31-34 |
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container_title | Monthly notices of the Royal Astronomical Society |
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creator | Riley, J M W Waldram, E M Riley, J M |
description | The Cambridge Low Frequency Synthesis Telescope has been used at 151 MHz to survey 33 regions. The resolution is 70 x 70 cosec delta sq arcsec, and the rms noise is typically 25 mJy/beam. We present positions and flux densities for about 15000 sources that have signal-to-noise ratios above 5.5. These observations almost complete the coverage by 7C of the region. (Author) |
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The resolution is 70 x 70 cosec delta sq arcsec, and the rms noise is typically 25 mJy/beam. We present positions and flux densities for about 15000 sources that have signal-to-noise ratios above 5.5. These observations almost complete the coverage by 7C of the region. (Author)</abstract></addata></record> |
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ispartof | Monthly notices of the Royal Astronomical Society, 1999-06, Vol.306 (1), p.31-34 |
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language | eng |
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source | Oxford University Press Open Access; EZB Electronic Journals Library |
title | The 7C survey of radio sources at 151 MHz - 33 regions in the range RA 7-17 h, Dec. 30-58 deg |
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