009 The smaller object to the southwest is a star (SDSS). 020 The smaller object to the west is a star (SDSS). 021 The radio emission is displaced northwest of the optical center. It is 021 extended to the east and is associated with a faint optical galaxy. 027 The extended radio source is about 8" south of a group of bright galaxies. 027 It is unidentified, but faint background optical emission lies near the 027 radio emission. 032 The radio source is well displaced from the galactic nucleus. There is a 032 spur of optical emission near the radio centroid. 050 The main part of the radio emission is associated with a 23rd magnitude 050 galaxy. There is radio emission extending to the galaxies to the east and 050 west. 053 The extended radio emission is associated with a close binary system. 069 This extended radio source is identified with a symmetric galaxy. The 069 contour plot of the entire radio source (Fig. 8 below) shows a morphology 069 closer to FR I than FR II (lobes are diffuse with no hot spot). 091 The radio source is displaced 3" west of the galaxy nucleus. It may be a 091 background unidentified source, or it may be associated with a faint spur 091 toward the west from the galaxy. 096 The radio source is identified with a faint galaxy. There is extended radio 096 emission connected to another galaxy about 7" to the south. 101 One radio component is associated with the nucleus of the galaxy. A second 101 radio component (101B) is located 2" north, roughly in the direction of the 101 extended optical core. 104 The radio source is located at the nucleus of the southern galaxy of a close 104 pair. Source 105 is to the north. The circular object to the west is a 104 star (SDSS). 105 The radio source is located at the nucleus of the northern galaxy of a close 105 pair. Source 104 is to the south. 109 Most of the radio emission is associated with the southern galaxy. The 109 object about 3" to the northwest is a star (SDSS), with a hint of faint 109 radio emission. 112 The object 4" to the west is a star (SDSS). 122 The radio source lies in the middle of a group of galaxies but is considered 122 unidentified, since there is no optical emission coincident with the 122 radio source. 141 The identification is uncertain. 143 The main radio emission is associated with a 23rd magnitude galaxy. There 143 are indications of extended emission associated with two nearby galaxies. 156 The radio source is located near a bright star (SDSS) that is saturated on 156 the image. Source 158 is at the lower left border of the frame. 158 The radio emission is located within the glare of a bright star (SDSS). 159 The identification is uncertain. 169 The radio source is associated with a blue stellar object (SDSS). 169 It could be a quasar. 171 The identification is uncertain. 175 The large-scale radio emission is associated with several galaxies. 177 The identification is uncertain. 183 The optical object 3" to the west is a star (SDSS). 185 Three objects show radio emission. However, the northernmost radio source 185 (185C) is a slightly red stellar object (SDSS), while components 185A and 185 185B are associated with individual galaxies. 188 The radio emission associated with the elliptical galaxy is complex. 188 A bright star is located about 10" northeast. 195 The radio emission lies between a circular galaxy to the north and a fainter 195 galaxy to the southwest (morphology unknown). 201 Two of the three galaxies have radio emission (components 201A and 201B). 201 They are cataloged as one radio source, since the galaxies appear to be 201 interacting. 212 The radio contours here just show the radio core of an extended active 212 galaxy with lobes 38" to the south and 45" to the north (see the contour 212 plot of the entire source in Fig. 8). This source has a classic FR II 212 morphology. 229 The radio source is lost in the glare of a bright star (SDSS). 234 The identification is uncertain. 236 The bright object to the northeast is a star (SDSS). 239 The fainter object to the southwest is a star (SDSS). 244 The brighter radio source is identified with a 20mag, slightly red stellar 244 object (SDSS). The weaker component 3" to the southwest is unidentified. 244 Perhaps it is a background galaxy that is obscured. 254 Unidentified. This and source 255 could be a pair of radio lobes associated 254 with the galaxy located between them. 255 Unidentified. This and source 254 could be a pair of radio lobes associated 255 with the galaxy located between them. 257 Extended radio emission has a similar orientation to the optical galaxy. 257 This source is 10" west of No. 263. 263 The orientation of the radio emission is similar to the optical light of the 263 galaxy and points to a fainter binary component. This source is 10" east 263 of No. 257 and is assumed to be an independent source. 264 Most of the radio emission is offset from the nucleus of the galaxy but 264 coincident with a faint optical feature. It is classified as a binary. 266 There is extended radio emission along the minor axis of the galaxy. 266 It could be an extended AGN. 267 The identification is uncertain. 268 The main radio component (268A) is near the galaxy center. Two fainter arms 268 of radio emission are also present. 275 The identification is uncertain. 280 The major component is offset 2" southwest of a galaxy. A brighter galaxy 280 with faint emission lies about 7" to the north. 294 The relationship of the radio emission and the faint galaxies within 2" is 294 unclear. 295 The small-diameter radio source is significantly displaced from the center 295 of an elliptical galaxy. There is a star (SDSS) located 8" to the northeast 299 The optical object is a red stellar object (SDSS). 304 This is an extended active galaxy with an intermediate FR I-II morphology 304 (see contour plot in Fig. 8). 314 Most of the extended radio emission is located in the center of a bright 314 galaxy; however, there is extended radio emission toward a faint companion 314 to the west. 315 A group of galaxies contains radio emission associated with two of the 315 galaxies. There is additional extended radio emission. 319 The radio emission is displaced southwest of the core of the galaxy. The 319 relationship to the bright galaxy 8" to the northeast is unclear. 330 This is a complicated group of galaxies. Two have significant radio emission 330 (330A, 330B). Source 335 lies southeast of this region. 335 This is a line of three galaxies, with the southern two having radio 335 emission. The radio sources are 15" southeast of the complex of sources 335 comprising No. 330. 340 The radio source is in the glare of the 10th magnitude star. 346 The radio emission contains two components, each probably identified with a 346 faint galaxy. It is classified as a binary but could be considered as two 346 independent identifications. 350 The radio source is close to the 10th magnitude star. 353 The radio emission is relatively weak and extended. This is cataloged as one 353 source with two components, the southern one identified with a galaxy and 353 the more extended northern component leading toward a fainter galaxy to the 353 northeast. However, the source is weak and this association is uncertain. 359 The radio source is identified with a faint galaxy. There is an elliptical 359 galaxy 2" to the west, and it is unknown whether there is a physical 359 connection between these two optical objects. 360 The radio source is too close to a 10th magnitude star to be identified. 385 The two radio components are identified with two galaxies in a crowded group 385 of galaxies. The bright object to the southeast is stellar. 386 The radio source is unidentified. Source 391, which is 6" northwest, is also 386 unidentified. It is possible that sources 386 and 391 are radio lobes of 386 the galaxy lying roughly between them, but there is no detection of a 386 radio core. 390 The object north of the radio identification is stellar (SDSS). 391 The radio source is unidentified. Source 386, which is 6" southeast, is also 391 unidentified. It is possible that sources 386 and 391 are radio lobes 391 associated with the galaxy between them. 400 The redshift is 0.322 (Fomalont et al., 2002, Cat. ). 403 The optical object is a blue stellar object (SDSS). It is a quasar with a 403 redshift of 2.561 (Fomalont et al., 2002, Cat. ). 407 The radio source is associated with a faint, diffuse object that is 2" east 407 of a brighter galaxy. The two galaxies may be part of a binary. 409 The peak emission of the radio source lies 1.5" southwest of the center of 409 the galaxy and may be associated with an optical spur to the southwest. 412 The optical object is a red stellar object (SDSS). 413 The radio emission is associated with a galaxy. The bright object is stellar 413 (SDSS). The low surface brightness of the extended optical emission 413 is puzzling. 416 The optical object is a blue stellar object (SDSS). It is probably a quasar. 418 The extended radio source is identified with a faint object at the edge of 418 the image of a bright star (SDSS). 419 The optical object is a blue stellar object (SDSS). It is probably a quasar. 431 The nature of this radio source is puzzling. One radio component (B) is 431 associated with faint emission southeast of the nucleus of the brighter 431 object. The brighter radio source is northwest of the bright galaxy, 431 although it could be associated with a faint spur (or an unrelated faint 431 background object) to the northwest. These components could also be radio 431 lobes associated with the bright galaxy, with no detectable core emission 431 from the nucleus. However, the near-coincidence of this possible radio lobe 431 to the southeast with optical emission argues somewhat against a twin-lobed 431 radio source. The 8 GHz radio image (source 29, or J131219 423608 in the 431 8GHz catalog) at lower resolution blends these two radio components with 431 no indication of emission from the galaxy nucleus (Fomalont et al., 2002, 431 Cat. ). 434 The identification is uncertain. 435 This is a complex region of radio and optical emission. The peak of the 435 radio emission is near a faint spur from the most southern galaxy. 438 The redshift is 0.302 (Fomalont et al., 2002, Cat. ). 442 The redshift is 0.180 (Fomalont et al., 2002, Cat. ). 443 The bright radio component lies near the center of the galaxy. There is also 443 a faint radio component (443B) 4" to the east. It is unknown whether this 443 is related to the galaxy or associated with a faint background object. 446 The peak of the radio emission is coincident with a circular galaxy. Radio 446 jets emanate north and south of the core for 5", and the source has been 446 classified as an FR I galaxy. (See contour plot in Fig. 8.) 449 The optical object northeast of the radio source is stellar (SDSS). 449 The identification is uncertain. 450 The radio source is centered on a blue stellar object (SDSS), a quasar with 450 redshift 2.561 (Fomalont et al., 2002, Cat. ). 453 The object northeast of the radio source is a red stellar object (SDSS). 453 Hence, it is unlikely to be part of a binary system. 457 The redshifts of both galaxies are 0.401 (Fomalont et al., 2002, 457 Cat. ). 461 Some of the radio emission extends from the center of the fainter galaxy 461 toward the brighter galaxy. 462 The radio emission is extended and may be associated with three closely 462 grouped galaxies. 466 This is the fainter extended member of a close, weak pair. Source 471, 466 about 3" to the northeast, is more compact. Both sources are unidentified 466 and not in the complete catalog. 469 The brighter radio source lies near the center of a galaxy. The fainter 469 radio source (469B) is associated with another galaxy to the east. These 469 two objects have been cataloged as one source because the galaxies appear 469 to be interacting. 471 This is the brighter compact member of a close, weak pair. Source 466, 471 about 3" to the southwest, is more extended. Both sources are unidentified 471 and not in the complete catalog. 477 There is faint extended radio emission from the optical identification 477 toward another galaxy 8" to the north. 483 The radio source is identified with an elliptical galaxy that is near a 483 bright red stellar object (SDSS). 490 The radio source is coincident with a galaxy that is about 2" south of a 490 stellar object (SDSS). 503 This is an extended active galaxy with a morphology closer to FR I than to 503 FR II (see contour plot in Fig. 8). 504 The radio source is coincident with a galaxy that lies near two bright 504 stars (SDSS). 507 This radio source is north of the northern lobe of the extended active 507 galaxy No. 503 (Fig. 8). It is identified with a faint galaxy and probably 507 not part of source 503. 515 The main radio source is located 1" east of a bright red stellar object 515 (SDSS). This identification is classified as stellar but may be a compact 515 red galaxy. There may be extended, faint radio emission along the galaxy's 515 north-south line. 535 The radio emission lies on a galaxy to the north of a bright star (SDSS). 549 The strong radio core and the emission to the west and east are associated 549 with an extended active galaxy. It could be an FR II source, but the lobes 549 are too weak to be certain. (See Fig. 8.) 563 The radio source is coincident with a faint optical object that is 5" east 563 of a bright circular galaxy. We have classified this as a binary system. 566 The compact radio emission is located 3" west of a bright galaxy, perhaps 566 identified with a faint optical object. A faint radio extension toward the 566 bright galaxy suggests that the compact radio emission is associated with 566 the bright galaxy. 567 The two radio components have been classified as a binary; however, they may 567 be independent sources. 569 The nucleus of this bright galaxy has a slightly extended radio source. 569 Source 578 is located 10" to the northwest. 575 The slightly extended radio source is identified with a faint galaxy. 575 The bright object to the west is stellar (SDSS). 582 The radio source is associated with a faint binary visible above the glare 582 of the nearby bright star. 589 The identification is uncertain. 594 Most of the radio emission comes from an optical spur to the northeast of 594 the galaxy nucleus. Some extended emission covers the other spur and the 594 galactic nucleus. 601 The radio emission is located at the western edge of a 25th magnitude galaxy 601 that is probably in a binary pair. 611 The radio source is centered on a faint object between two brighter objects. 621 The extended radio emission is an asymmetric FR I source (see Fig. 8). 626 The radio source is clearly displaced from the galaxy. The probability that 626 this is a random association is about 10%. 634 The radio emission is coincident with a galaxy that is located in the glare 634 of the bright star. 654 This region, near the plate edge, has poor optical sensitivity. The western 654 component might be identified with a faint galaxy; the eastern is not. 654 Classified as unidentified. 660 The radio emission lies on an optical bridge between two galaxies. 668 A large diffuse radio source with two extended components is associated 668 with a group of galaxies. 676 The radio component is clearly displaced from a galaxy core and not 676 associated with an optical feature. It is unlikely to be associated with 676 another, invisible background galaxy. The probability that this source is 676 unrelated to the bright galaxy is less than 10%. The source to the east 676 is No. 680. 680 The radio source is coincident with a compact galaxy that is 7" east of a 680 brighter galaxy. Source 676 lies to the west. 685 The radio source is associated with a faint galaxy near the edge of the 685 image of a bright star (SDSS). The identification is uncertain. 711 The two galaxies in this binary have radio emission that is oriented along 711 each galaxy's major axis. They could be considered as two independent 711 sources, although the optical objects appear to be interacting. 715 The identification is uncertain. 721 The identification with a very faint optical object has only a 50% 721 probability. Faint extended radio emission to the east may be associated 721 with another galaxy 3" to the east. 738 The radio emission is extended and covers several galaxies. 740 The unresolved radio emission peak is located between two 23rd magnitude 740 galaxies. It is considered as unidentified, although it may be associated 740 with one or both of the nearby galaxies. Source 741 can be seen at upper 740 left and is assumed to be unrelated to this source. 748 This is a bright source at the edge of the z-band image, with reduced 748 optical sensitivity and some distortion. The identification is uncertain. 753 The radio emission is extended and may be associated with several galaxies 753 in this group. 754 The radio source is close to a 26th magnitude object that is 1" north of a 754 brighter galaxy. The identification is uncertain. 771 The radio source is extended and located between the galaxy nucleus and an 771 optically brightened region about 1" to the east. 779 The probability of identification of this radio source with the faint object 779 that is 2" north of a binary system is 80%. It is unknown if the faint 779 optical emission is associated with the brighter binary. 790 The radio source lies 1" north of a 24th magnitude galaxy. It could be 790 associated with this galaxy but may also be identified with a faint optical 790 object. It is tentatively considered as unidentified. 792 The extended radio source is coincident with a faint galaxy that is 8" 792 southwest of a much brighter galaxy. We assume that the faint galaxy is a 792 background object. 800 The radio source is associated with faint diffuse emission that is 3" north 800 of a brighter galaxy. There is also faint radio emission near the bright 800 galaxy. 806 The extended radio source is centered on a faint object that lies between 806 two binary systems. The radio emission extends to the northern galaxy of a 806 binary system to the northwest.