NVSS J010619-325713 Narrow-angle tail source with partially detached tails 
NVSS J010619-325713  (e.g. similar morphology to J1324-3138 in the Abell cluster
NVSS J010619-325713  A3556; Venturi et al., 1998MNRAS.298.1113V). The optical 
NVSS J010619-325713  counterpart is located at the centroid of the cluster 
NVSS J010619-325713  EDCC 0523 (Lumsden et al., 1992, Cat. <VII/175>); using 
NVSS J010619-325713  data from the 2dF Galaxy Redshift Survey (2dFGRS; 
NVSS J010619-325713  Colless et al., 2001, Cat. <VII/250>), De Propris et al. 
NVSS J010619-325713  (2002, Cat. <J/MNRAS/329/87>) determined the cluster 
NVSS J010619-325713  centroid to be located at RA=01:06:20s28, DE=-32:57:32.7 
NVSS J010619-325713  with a redshift of z=0.146+/-0.002. The 2dFGRS redshift of 
NVSS J010619-325713  the optical counterpart is z=0.1433+/-0.0002.
NVSS J014353-331041 Wide-angle tail source with a clear optical identification. 
NVSS J014353-331041  The 2dFGRS redshift of the optical counterpart is 
NVSS J014353-331041  z=0.1756+/-0.0003.
NVSS J015745-310557 Two independent, closely spaced doubles. While the 408, 843 
NVSS J015745-310557  and 1400MHz flux densities are blended, both doubles are 
NVSS J015745-310557  still HzRG candidates: {alpha}^2368^_1384_=-1.50+/-0.12 for
NVSS J015745-310557  the north double, and {alpha}^2368^_1384_=-1.57+/-0.12 for 
NVSS J015745-310557  the south double.
NVSS J020828-342520 See NVSS J020827-342635
NVSS J020827-342635 + NVSS J020828-342520. This source has a complex, diffuse, 
NVSS J020827-342635  multicomponent morphology. There are a number of faint 
NVSS J020827-342635  confusing sources at 1384MHz that are not resolved in NVSS
NVSS J020827-342635  (these are included in the total 1384MHz flux density in 
NVSS J020827-342635  Table 3). Both the southern lobe and most of the confusing 
NVSS J020827-342635  sources are either marginally detected or not detected at 
NVSS J020827-342635  2368MHz, implying that they have very steep spectra. The 
NVSS J020827-342635  2dFGRS redshift of the optical counterpart is 
NVSS J020827-342635  z=0.3044+/-0.0003.
NVSS J111921-363139 This single-component source is also in the MRC-PMN USS 
NVSS J111921-363139  sample, with spectral index {alpha}^4850^_408_=-1.24+/-0.05
NVSS J111921-363139  (De Breuck et al., 2000, Cat. <J/A+AS/143/303>). It was 
NVSS J111921-363139  observed with the ATCA at 1420MHz by De Breuck et al. 
NVSS J111921-363139  (2000, Cat. <J/A+AS/143/303>), who obtained a flux density 
NVSS J111921-363139  of S1420=542+/-54mJy. This is consistent with our 
NVSS J111921-363139  1384 MHz flux density of S1384=509.2+/-15.8mJy.
NVSS J120839-340307 Double source that is also in the Molonglo Southern 4Jy 
NVSS J120839-340307  sample (MS4; Burgess & Hunstead, 2006, Cat. <J/AJ/131/100>,
NVSS J120839-340307  Cat. <J/AJ/131/114>) and the MRC-PMN USS sample (spectral 
NVSS J120839-340307  index {alpha}^4850^_408_=-1.28+/-0.04; De Breuck et al.,
NVSS J120839-340307  2000, Cat. <J/A+AS/143/303>). Burgess & Hunstead (2006, 
NVSS J120839-340307  Cat. <J/AJ/131/114>) used the Anglo-Australian Telescope 
NVSS J120839-340307  (AAT) to detect an optical counterpart between the lobes at
NVSS J120839-340307  RA=12:08:39.68, DE=-34:03:10.6 with R=22.9+/-0.5mag. The 
NVSS J120839-340307  SuperCOSMOS BJ magnitude of the optical counterpart is 
NVSS J120839-340307  >22.5mag.
NVSS J215547-344614 Two independent, closely spaced wide-angle tail (north) and 
NVSS J215547-344614  head-tail (south) sources that are potentially members of 
NVSS J215547-344614  the same distant cluster (e.g. similar morphology to 
NVSS J215547-344614  MRC B1610-605 + MRC B1610-608 in Jones &McAdam 1992, Cat. 
NVSS J215547-344614  <J/ApJS/80/137>); {alpha}^2368^_1384_=-1.28+/-0.14 for the 
NVSS J215547-344614  wide-angle tail source, and 
NVSS J215547-344614  {alpha}^2368^_1384_=-0.90+/-0.12 for the head-tail source.