Abstract
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).
Original language | English |
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Journal | VizieR Online Data Catalog |
Volume | 739 |
Publication status | Published - 2009 |
Keywords
- Supernova remnants
- H II regions
- Radio sources
- Morphology