posted on 2024-07-12, 22:11authored byEmil Lenc, Mike Garrett, Olaf Wucknitz, James Anderson, Steven Tingay
We report on a recent 90 cm wide-field VLBI survey of two 3.1 deg2 fields using the VLBA, Westerbork and Jodrell Bank telescopes. In-beam calibration was used to calibrate each field, the process was simplified by imaging the calibrators in DIFMAP and transferring the calibration solutions to AIPS using the newly developed DIFMAP task - cordump. We detected and imaged 13 out of the 141 sources originally detected by the low resolution (54′′) WENSS survey of the same two fields. The sources were detected at 7−12 sigma levels above the image noise, had total flux densities ranging between 85−1640 mJy and were between 16′−58′ from the phase centre of each field. This is the first systematic (and non-biased), deep, high resolution survey of the low frequency radio sky. These initial results suggest that new instruments such as LOFAR should detect many compact radio sources and that plans to extend these arrays to baselines of several thousand kilometres are warranted.
science: 8th European VLBI Network Symposium, Torun, Poland, 26-29 September 2006 / Willem Baan, Rafael Bachiller, Roy Booth, Patrick Charlot, Phil Diamond, Mike Garrett, Xiaoyu Hong, Justin Jonas, Andrzej Kus, Franco Mantovani, Andrzej Marecki, Hans Olofsson, Wolfgang Schlueter, Merja Tornikoski, Na Wang and Anton Zensus (eds.)
Conference name
science: 8th European VLBI Network Symposium, Torun, Poland, 26-29 September 2006 / Willem Baan, Rafael Bachiller, Roy Booth, Patrick Charlot, Phil Diamond, Mike Garrett, Xiaoyu Hong, Justin Jonas, Andrzej Kus, Franco Mantovani, Andrzej Marecki, Hans Olofsson, Wolfgang Schlueter, Merja Tornikoski, Na Wang and Anton Zensus eds.