Table 2: Map parameters of the MERLIN-detected sources. Column 1: source name; Col. 2: spectral class from Ho et al. (1997a); Col. 3: restoring beam; Col. 4: position angle of the beam; Col. 5: rms noise level of the image.
  Spectral Beamsize PA rms
Galaxy Class (mas2) (deg) (mJy/beam)
(1) (2) (3) (4) (5)
N 2768 L2 130 $\times$ 68 - 7.07 0.10
N 3169 L2 178 $\times$ 56 -45.27 0.09
N 3226 L1.9 153 $\times$ 48 -51.23 0.07
N 3414 L2 153 $\times$ 49 -49.53 0.06
N 3718 L1.9 161 $\times$ 130 +54.66 0.06
N 3884a L1.9 86 $\times$ 58 -79.10 0.05
N 4143 L1.9 71 $\times$ 41 +50.37 0.06
N 4203 L1.9 126 $\times$ 47 -28.85 0.06
N 4293 L2 159 $\times$ 55 -18.22 0.06
N 4321 T2 174 $\times$ 55 -15.41 0.06
N 4450 L1.9 177 $\times$ 57 -14.73 0.06
N 5077a L1.9 145 $\times$ 47 +12.02 0.08
N 5297a L2 71 $\times$ 42 +29.53 0.06
N 5353 L2 73 $\times$ 44 +23.66 0.06
N 5363 L2/T2: 100 $\times$ 46 +24.83 0.11
$\textstyle \parbox{8cm}{ $^a$\space New subarcsecond-scale radio detection.}$

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