#Table: J/A+AS/143/303/notes.dat (http://cdsarc.cds.unistra.fr) ------------------------------------------------------------------------------------------ |m_N| Name |ame|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. ) 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. ). 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. ). 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. ------------------------------------------------------------------------------------------