Physics
Scientific paper
Jun 2009
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009ycat..73911384f&link_type=abstract
VizieR On-line Data Catalog: J/MNRAS/391/1384. Originally published in: 2008MNRAS.391.1384F
Physics
Supernova Remnants, H Ii Regions, Radio Sources, Morphology
Scientific paper
The 2002 deep integration was obtained using six of the MERLIN antennas, including the Cambridge telescope. The observing strategy and correlator configuration replicated those used in the 1992 5-GHz observations presented by Muxlow et al. (1994MNRAS.266..455M). The 2002 observations were undertaken between the April 1 and 28 at a frequency of 4.994GHz using both left-left (LL) and right-right (RR) polarizations and with a bandwidth of 15MHz divided into 15 channels. The total on source integration time was over 175h.
(1 data file).
Argo Megan K.
Beswick Rob J.
Fenech D. M.
Muxlow Thomas W. B.
Pedlar Alan
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