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For refcode 1996MNRAS.282..779W:
Retrieve 5548 NED objects in this reference.
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Copyright by Royal Astronomical Society. 1996MNRAS.282..779W The 7C survey of radio sources at 151 MHz - a region covering RA 9^h^ to 16^h^ and Dec. 20^deg^ to 35^deg^ E. M. Waldram, J. A. Yates, J. M. Riley and P. J. Warner Mullard Radio Astronomy Observatory, Cavendish Laboratory, Madingley Road, Cambridge CB3 OHE Accepted 1996 May 1. Received 1996 April 30; in original form 1995 October 31 ABSTRACT The Cambridge Low Frequency Synthesis Telescope has been used at 151 MHz to survey a region of 1393 deg^2^, in the range RA 9^h^-16^h^, Dec. 20^deg^-35^deg^, with an angular resolution of 108 x 108 cosec {delta} arcsec^2^. The rms noise on the maps is, in general, ~35-55 mJy beam^- 1^, but varies considerably and exceeds this in some areas. We have extracted sources with a signal-to-noise ratio > 5.5, totaling 5526, and present a catalogue of their position and flux densities. Key words: catalogues - surveys - radio continuum: general. ======================================================================== 1997MNRAS.284.1007W Erratum: The 7C survey of radio sources at 151 MHz - a region covering RA 9^h^ to 16^h^ and Dec. 20^deg^ to 35^deg^ by E. M. Waldram, J. A. Yates, J. M. Riley and P. J. Warner Key words: catalogues - surveys - radio continuum: general. The paper `The 7C survey of radio sources at 151 MHz - a region covering RA 9^h^ to 16^h^ and Dec. 20^deg^ to 35^deg^ was published in Mon. Not. R. Astron. Soc. 282, 779-787 (1996). Owing to a publishing error the specimen sample of the survey referred to in Section 7 was not included in Appendix A. Presented here is Table A1, the specimen section of the final list. See Journal. On microfiche 282/1 there is a typographical error in the text describing the column entries. Columns 3 and 4 are both mistakenly referred to as column 3. The correct text is (3) RA of the centroid position (B1950); (4) Dec. of the centroid position (B1950). See Journal.
Retrieve 5548 NED objects in this reference.
Please click here for ADS abstract

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