EISD  3 In the EIS I-band catalogue the two central objects erroneously appear 
EISD  3  as a single entry at RA = 09 50 31.32, DE = -21 02 44.4  with a 
EISD  3  magnitude of 20.15. In the other two bands they appear as two separate 
EISD  3  objects. The optical position was taken from the V-band data, and the 
EISD  3  I-band magnitude was re-determined. 
EISD  6 Two potential optical counterparts are found to this extended radio 
EISD  6  source. These have similar likelihood ratios, with the brighter galaxy 
EISD  6  to the north marginally favoured.
EISD 16 Although there is a weak radio feature towards the centre of this radio 
EISD 16  source, it is not clear if this is a core. A likelihood analysis 
EISD 16  treating the source as an extended source picks out the unresolved 
EISD 16  object associated with a radio structure to the north as the most 
EISD 16  likely optical counterpart.
EISD 38 The I~19 galaxy lying exactly on the south-eastern radio component is 
EISD 38  selected as a potential host galaxy.
EISD 41 There are two optical objects identified between the radio lobes, but 
EISD 41  neither achieves a likelihood ratio in excess of the cut-off.
EISD 47 This candidate should be considered very tentative, owing to the 
EISD 47  extremely faint I-band magnitude.
EISD 60 The faint optical object associated with the western radio component is 
EISD 60  kept as a potential id.
EISD 87 There are many optical galaxies close to the radio position, but none 
EISD 87  achieves a likelihood ratio above the cut-off value.
EISD 91 The two optical objects near the centre of the radio source are blended 
EISD 91  into a single object in the I-band catalogue. In the other two bands 
EISD 91  they appear as two separate objects. The optical position was taken 
EISD 91  from the V-band data, and the I-band magnitude was re-determined.
EISD102 The luminous galaxy coincident with the southern radio component is 
EISD102  retained as a likely optical counterpart.
EISD110 Strangely, this bright optical galaxy is not found within the EIS I-band
EISD110  catalogue, although it is in the V- and B-band catalogues. Its I-band 
EISD110  magnitude was measured directly from the image.
EISD120 The faint extended emission seen in the I-band overlay is not catalogued
EISD120  within the EIS catalogue, but appears convincingly on the image and so 
EISD120  its magnitude and position have been determined.
EISD123 This bright saturated galaxy is excluded from the EIS catalogue, but is 
EISD123  clearly the optical counterpart to the radio source. The optical image 
EISD123  shows it to be part of a merging system, with numerous bright tidal 
EISD123  features, including a long tidal tail stretching to the north.
EISD148 The I~19 object coincident with the eastern radio component is 
EISD148  considered a likely optical id.
EISD155 There is a bright galaxy overlying the northern radio component, which 
EISD155  is identified as a likely counterpart.
EISD162 The likely radio source counterpart is a fainter object close to a 
EISD162  brighter star. Although clearly distinct, these two objects are not 
EISD162  separated in any of the three catalogues. In the I-band the position 
EISD162  and an estimate of the magnitude of the source were determined from 
EISD162  the image.
EISD163 This very bright saturated galaxy is not included in the optical 
EISD163  catalogue. Also known as ESO 566-G 014, it has a redshift of 0.01559 
EISD163  in the NASA/IPAC Extragalactic Data base (NED). Its magnitudes quoted 
EISD163  there are B=14.9+/-0.1, R=14.0+/-0.1 and I=13.7+/-0.1.
EISD171 Two plausible optical counterparts are picked out by the likelihood 
EISD171  analysis, although in fact there are several I-band objects close to 
EISD171  the radio lobes, the majority of which (including the two selected 
EISD171  candidates) appear to be unresolved. It is not clear whether either of 
EISD171  these is really a good candidate.
EISD178 The galaxy close to the south-western radio lobe is retained as a 
EISD178  plausible optical host.
EISD181 This candidate should be considered very tentative, owing to the 
EISD181  extremely faint I-band magnitude.
EISD191 This very bright nearby spiral galaxy has a redshift of z=0.02935 in 
EISD191  NED, but in the EIS imaging is saturated and excluded from the 
EISD191  catalogue. The galaxy is also known as ESO 566-G 018, and has colours 
EISD191  from NED of B=14.1+/-0.1, R=13.1+/-0.1 and I=12.7+/-0.1.