TGN109Z024 See TGN109Z025 below.
TGN109Z025 This galaxy and TGN 109Z024 lie in the same cluster. There is a 
TGN109Z025  complex radio structure (see Figure) with peaks close to both these 
TGN109Z025  galaxies. For now, we assume that both are radio sources. 
TGN109Z025  Higher-resolution radio observations would be valuable.
TGN110Z073 Interacting galaxy pair.
TGN124Z197 uoted radio ux density is the sum of three NVSS components.
TGN135Z197 This galaxy is within 30 arcsec of the 15.2mag galaxy NGC5039. Some 
TGN135Z197  or all of the radio emission probably arises from NGC5039 (which is 
TGN135Z197  also an IRAS source with a 60{mu}m flux density of 0.353Jy) rather 
TGN135Z197  than TGN135Z197.
TGN137Z043 Identified as an ultraluminous IRAS galaxy by Clowes et al. 
TGN137Z043  (1995MNRAS.275..819C), who note that it has a Seyfert 2 optical 
TGN137Z043  spectrum.
TGN149Z091 Quoted radio ux density is the sum of two NVSS components.
TGN156Z046 Galaxy with Galactic star superimposed, redshift remeasured 
TGN156Z046  from 2dF spectrum.
TGN165Z119 Seyfert 1 galaxy (broad Balmer emission lines).
TGN165Z189 Interacting galaxy pair.
TGN171Z312 Quoted ux density is the sum of five NVSS components.
TGN207Z146 This is a QSO at redshift 3.0.
TGN284Z051 Quoted ux density is the sum of two NVSS components.
TGN286Z081 Interacting galaxy pair.
TGN299Z119 Another faint galaxy is closer to the radio centroid.
TGN304Z086 Redshift is from repeat 2dFGRS spectrum taken in Dec 1999.
TGN306Z194 Paired with TGN306Z196, which is also detected by NVSS.
TGN306Z196 Paired with TGN306Z194, which is also detected by NVSS.
TGN307Z092 See TGN307Z090 below
TGN307Z090 Unusuale very diffuse source. TGN307Z092 is more likely ID. 
TGN307Z090  Quoted flux density is the sum of four NVSS components.
TGN314Z018 ROSAT X-ray detection.
TGN318Z080 Quoted radio ux density is the sum of three NVSS components.
TGN348Z183 Quoted radio ux density is the sum of two NVSS components.
TGN401Z254 ROSAT X-ray detection. Quoted radio ux density is the sum of four 
TGN401Z254  NVSS components.
TGN402Z029 See TGN402Z030.
TGN402Z030 With TGN402Z029, interacting galaxy pair Arp 240 (NGC 5257/5258) - 
TGN402Z030  total IRAS ux density at 60{mu}m is 9.297Jy. We have assumed that 
TGN402Z030  half of this comes from each galaxy.
TGN422Z122 Quoted radio ux density is the sum of three NVSS components.
TGS119Z122 This source has a flux density of only 11.7mJy in the NVSS catalogue,
TGS119Z122  but the Parkes catalogue lists it as 230mJy at 2.7GHz. The Parkes 
TGS119Z122  source may be very diffuse and largely resolved out by the NVSS, or 
TGS119Z122  possibly time-varying. Further investigation is needed.
TGS184Z238 Quoted radio ux density is the sum of three NVSS components.
TGS190Z081 Quoted radio ux density is the sum of three NVSS components.
TGS190Z106 The radio source is a lobe of PKS2317-27, and the correct optical ID 
TGS190Z106  is the galaxy TGS190Z105 at z=0.1730.
TGS192Z053 Quoted radio ux density is the sum of two NVSS components.
TGS193Z242 Interacting pair of galaxies.
TGS209Z078 The original 2dFGRS position corresponds to a blob in the spiral arm 
TGS209Z078  of the bright spiral ESO411-011. The position and magnitude given 
TGS209Z078  here are for ESO411-011.
TGS210Z106 Radio emission extends to south and overlaps spiral companion 
TGS210Z106  TGS210Z108 (z=0.0401).
TGS221Z095 Starburst galaxy with unusual optical tail.
TGS223Z232 Quoted radio ux density is the sum of three NVSS components.
TGS232Z027 The original 2dFGRS position corresponds to a knot in the spiral arm 
TGS232Z027  of the bright spiral IC 1826. The position and magnitude given here 
TGS232Z027  are for IC 1826.
TGS234Z274 Another (faint) galaxy is closer to the radio centroid.
TGS235Z101 Radio overlay comfirms that this galaxy is the correct ID in spite 
TGS235Z101  of 11.1 arcsec offset.
TGS246Z061 Radio overlay suggests that the correct ID is the 18th magnitude 
TGS246Z061  galaxy TGS246Z062 at z=0.1723. 
TGS312Z171 There is another, fainter galaxy closer to the radio centroid.
TGS326Z047 Seyfert 1 galaxy (broad Balmer emission lines). ROSAT X-ray detection
TGS397Z016 Strong, broad emission lines.
TGS407Z205 Seyfert 1 galaxy, broad Balmer wings. ROSAT X-ray detection.