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Table 1:

Specifications of these observations.
No. Date Telescope Number Number Number Bandwidth Number of Ch.width Tot.BW On-source
  (yymmdd) (+conf.) of of of chann. per IF pol.prod. for ima- for ima- time (h)
      antennas $^{{\rm 1}}$ IFs $^{{\rm 2}}$ per IF (MHz) per IF ging (kHz) ging (MHz) $^{{\rm 3}}$  
1 860329 VLA A 11 1 127 3.1 1 98 2.5 4.6
2 860805 VLA B 8 1 127 0.8 1 98 0.7 4.9
3 861226 VLA C 15 1 63 0.8 1 98 0.7 6.2
4 881203 VLA A 22 2 7 1.4 1 195 2.7 5.7
5 890318 VLA B 27 2 7 0.7 1 98 1.4 5.3
6 020930 VLA CnB 22 2 31 3.0 2 98 8.2 5.3
7 050324 WSRT 12 7 128 10.0 4 6328 89 5.3
8 050514 WSRT (21cm) 14 6 64 20.0 4 12813 154 4.6
$^{{\rm 1}}$ This is the nummer of antennas after flagging; $^{{\rm 2}}$ this is the number of IFs after flagging averaged over the RR and LL polarisation products, if both are available; $^{{\rm 3}}$ this is total bandwidth for Stokes I imaging, we added RR and LL bandwidth.

Source LaTeX | All tables | In the text

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