| Name (m) --- | Note --- |
|---|---|
| WN J0043+4719 | The source 18" north of the NVSS position is not detected in |
| WN J0043+4719 | the NVSS. This is therefore not a real USS source because the |
| WN J0043+4719 | NVSS flux density was underestimated. |
| WN J0048+4137 | Our VLA map probably doesn't go deep enough to detect all the |
| WN J0048+4137 | flux of this source. |
| WN J0727+3020 | The higher resolution FIRST map shows that both components of |
| WN J0727+3020 | this object are indeed identified on the POSS, even though the |
| WN J0727+3020 | NVSS position is too far off to satisfy our identification |
| WN J0727+3020 | criterion. |
| WN J0717+4611 | Optical and near-IR spectroscopy revealed this object as a red |
| WN J0717+4611 | quasar at z=1.462 (De Breuck et al., 1998AJ....116...13D). |
| WN J0725+4123 | The extended POSS identification suggest this source is |
| WN J0725+4123 | located in a galaxy cluster. |
| WN J0829+3834 | The NVSS position of this unresolved source is 7" (3{sigma}) |
| WN J0829+3834 | from the FIRST position, which itself is only at 2" from the |
| WN J0829+3834 | WENSS position. |
| WN J0850+4830 | The difference with the NVSS position indicates that our VLA |
| WN J0850+4830 | observations are not deep enough to detect a probable |
| WN J0850+4830 | north-eastern component. |
| WN J0901+6547 | This 38" large source is over-resolved in our VLA |
| WN J0901+6547 | observations, and probably even misses flux in the NVSS, and |
| WN J0901+6547 | is therefore not a real USS source. |
| WN J1012+3334 | The bend morphology and bright optical sources to the east |
| WN J1012+3334 | indicate this object is probably located in a galaxy cluster. |
| WN J1101+3520 | The faint FIRST component 20" north of the brighter Southern |
| WN J1101+3520 | component is not listed in the FIRST catalog, but is within |
| WN J1101+3520 | 1" of a faint optical object. This might be the core |
| WN J1101+3520 | of a 70" triple source. |
| WN J1152+3732 | The distorted radio morphology and bright, extended POSS |
| WN J1152+3732 | identification suggest this source is located in a |
| WN J1152+3732 | galaxy cluster. |
| WN J1232+4621 | This optically identified and diffuse radio source suggest |
| WN J1232+4621 | this source is located in a galaxy cluster. |
| WN J1314+3515 | The diffuse radio source appears marginally detected on the |
| WN J1314+3515 | POSS. |
| WN J1329+3046 A,B | and WN J1330+3037, WN J1332+3009 & WN J1333+3037 : The noise |
| WN J1329+3046 A,B | in the FIRST image is almost ten times higher than average due |
| WN J1329+3046 A,B | to the proximity of the S1400=15Jy source 3C 286. |
| WN J1330+3037 | See WN J1329+3046A,B |
| WN J1332+3009 | See WN J1329+3046A,B |
| WN J1333+3037 | See WN J1329+3046A,B |
| WN J1330+5344 | The difference with the NVSS position indicates that our VLA |
| WN J1330+5344 | observations are not deep enough to detect a probable |
| WN J1330+5344 | south-eastern component. |
| WN J1335+3222 | Although the source appears much like the hotspot of a larger |
| WN J1335+3222 | source with the core 90" to the east, no other hotspot is |
| WN J1335+3222 | detected in the FIRST within 5'. |
| WN J1359+7446 | The extended POSS identification suggests this source is |
| WN J1359+7446 | located in a galaxy cluster. |
| WN J1440+3707 | The equally bright galaxy 30" south of the POSS identification |
| WN J1440+3707 | suggests that this source is located in a galaxy cluster. |
| WN J1509+5905 | The difference with the NVSS position indicates that our VLA |
| WN J1509+5905 | observations are not deep enough to detect a probable western |
| WN J1509+5905 | component. |
| WN J1628+3932 | This is the well studied galaxy NGC 6166 in the galaxy cluster |
| WN J1628+3932 | Abell 2199 (e.g. Zabludoff et al., 1993, Cat. <J/AJ/106/1273>) |
| WN J1509+5905 | The difference with the NVSS position indicates that our VLA |
| WN J1509+5905 | observations are not deep enough to detect a probable |
| WN J1509+5905 | west-south-western component. |
| WN J1821+3601 | The source 35" south-west of the NVSS position is not detected |
| WN J1821+3601 | in the NVSS. This is therefore not a real USS source because |
| WN J1821+3601 | the NVSS flux density was underestimated. |
| WN J1832+5354 | The source 19" north-east of the NVSS position is not detected |
| WN J1832+5354 | in the NVSS. This is therefore not a real USS source because |
| WN J1832+5354 | the NVSS flux density was underestimated. |
| WN J1852+5711 | The extended POSS identification suggests this source is |
| WN J1852+5711 | located in a galaxy cluster. |
| WN J2313+3842 | The extended POSS identification suggests this source is |
| WN J2313+3842 | located in a galaxy cluster. |
| TN J0233+2349 | This is probably the north-western hotspot of a 35" source, |
| TN J0233+2349 | with the south-eastern component barely detected in our |
| TN J0233+2349 | VLA map. |
| TN J0309-2425 | We have classified. this source as a 13" double, but the |
| TN J0309-2425 | western component might also be the core of a 45" source, with |
| TN J0309-2425 | the other hotspot around RA=3h9m10s, DE=-24{deg}25'50". |
| TN J0349-1207 | The core-dominated structure is reminiscent of the |
| TN J0349-1207 | red quasar WN J0717+4611. |
| TN J0352-0355 | This is probably the south-western hotspot of a 30" source. |
| TN J0837-1053 | Given the 10" difference between the positions of the NVSS and |
| TN J0837-1053 | diffuse VLA source, this is probably the northern component |
| TN J0837-1053 | of a larger source. |
| TN J0408-2418 | This is the z=2.44 source MRC 0406244 (McCarthy et al., 1996, |
| TN J0408-2418 | Cat. <J/ApJS/107/19>). The bright object on the POSS is a |
| TN J0408-2418 | foreground star to the north-east of the R=22.7 galaxy. |
| TN J0443-1212 | Using the higher resolution VLA image, we can identify this |
| TN J0443-1212 | radio source with a faint object on the POSS. |
| TN J2106-2405 | This is the z=2.491 source MRC 2104-242 (McCarthy et al., |
| TN J2106-2405 | 1996, Cat. <J/ApJS/107/19>). The identification is an R=22.7 |
| TN J2106-2405 | object, not the star to the north-north-west of the |
| TN J2106-2405 | NVSS position. |