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.
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Schedule a callDisclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.
