UCM0001+2255  UGC 14, Sc as in RC3 (de Vaucouleurs et al., 1991). 
UCM0001+2255  Asymmetric arm at the north and various HII regions.
UCM0003+2200  KUG0003+220 from the UV excess Kiso survey (Takase & 
UCM0003+2200  Miyauchi-Isobe, 1993). High inclination galaxy, with a possible 
UCM0003+2200  emitting knot at the east side of the nucleus. All the criteria 
UCM0003+2200  points to a late type galaxy.
UCM0013+1944  Sc, no obvious signs of interaction with the eastern ZWG 456.050.
UCM0014+1829  Low luminosity Sa galaxy. A field star contaminates the profile.
UCM0014+1748  UGC 164, SBbc in RC3. Very bright nucleus, southwest arm more
UCM0014+1748  prominent and a knot at the northeastern arm.
UCM0015+2212  Mrk 1141, compact in Mazzarella & Balzano (1986). More probably
UCM0015+2212  a Sa type galaxy.
UCM0017+1942  KARA72004A = Arak 7 = MCG+3-02-002. Almost edge-on Sc galaxy,
UCM0017+1942  very distorted, without obvious signs of interaction with the
UCM0017+1942  northeast neighbor barred UGC 188 (both at the same z).
UCM0018+2216  Very compact (D24 = 8 kpc), almost face-on and with typical 
UCM0018+2216  parameters of a Sb galaxy.
UCM0019+2201  Sc galaxy, without emitting knots outside the nucleus.
UCM0022+2049  ZWG 457.013, northeastern arm more developed. More probably 
UCM0022+2049  Sb type.
UCM0038+2259  More probably a Sa galaxy placed to the south of two stars
UCM0038+2259  and an ELG at 37" NW of the UCM.
UCM0040+0257  Mrk 1144, pair with Mk 1143 (Mazzarella & Balzano, 1986).
UCM0040+0257  Also UM 61 in the University of Michigan survey of ELGs in the 
UCM0040+0257  blue (MacAlpine et al., 1977a). Signs of interaction between
UCM0040+0257  the two galaxies and a low luminosity galaxy  (the three at
UCM0040+0257  the same z) located 14" SE from the UCM Sc type galaxy.
UCM0040+0220  UM 63 (MacAlpine et al., 1977a). Low luminosity galaxy, almost
UCM0040+0220  face-on, disk dominated profile, with photometric parameters 
UCM0040+0220  more typical of a Sb type.
UCM0043+2440  Very bright nucleus, Sa type.
UCM0044+2246  MG+04-03-003, asymmetrical Sb spiral, northern arm more extended.
UCM0045+2256  Without B+D decomposition, profile with FWHM equal to the PSF
UCM0045+2256  seeing, with anomalous photometric parameters for a galaxy.
UCM0045+2256  Possible star.
UCM0047+2051  Only known as IRAS00472+2051 source. Photometric parameters
UCM0047+2051  proper for a Sc galaxy.
UCM0047-0213  UM 280 (MacAlpine et al., 1977b), bulge component very prominent,
UCM0047-0213  photometric trend to Sa type.
UCM0047+2413  MCG+04-03-011, more probably a Sa type with a bar at 
UCM0047+2413  PA=45 degrees, and an emitting knot at west.
UCM0049-0006  UM 282 (MacAlpine et al., 1977b), compact (D24 = 7.7 kpc)
UCM0049-0006  and low luminosity object (Mr = -18.6), candidate to BCD.
UCM0049+0017  UM 283 (MacAlpine et al., 1977b), probably small Sc.
UCM0050+0005  UM 290 (MacAlpine et al., 1977b), eastern arm more prominent,
UCM0050+0005  trend to Sa type galaxy.
UCM0050+2114  Mrk 349, compact in Mazzarella & Balzano (1986), but clearly
UCM0050+2114  spiral in our r image, probably Sa.
UCM0056+0044  UM 295 (MacAlpine et al., 1977b), all the criteria point to
UCM0056+0044  Irr morphology.
UCM0056+0043  UM 296 (MacAlpine et al., 1977b), probably small Sc.
UCM0119+2156  Only known as IRAS01196+2156 source. High luminosity
UCM0119+2156  (Mr = -22.5) Sc galaxy and Sy 2 (Gallego et al., 1995).
UCM0121+2137  MCG+04-04-010, catalogued as S ring, although the ring
UCM0121+2137  is not visible in our r image. Sc type with a knot located 8"
UCM0121+2137  west of the nucleus.
UCM0130+2505  Compact and with ambiguous classification. Although it
UCM0130+2505  presents stellar appearance, it could be a Sb.
UCM0135+2242  Its parameters point to S0 type.
UCM0141+2220  More probably a Sb type.
UCM0142+2137  MCG+04-05-004. High luminosity (Mr = -22.6) SBb galaxy
UCM0142+2137  and Sy 2 (Gallego et al., 1995).
UCM0145+2519  MCG+04-05-010, SBr in RC3. We appreciate an excess of light
UCM0145+2519  between 8" and 16" in the profile, maybe due to the ring,
UCM0145+2519  and with parameters typical of SB(r)c.
UCM0147+2309  More probably a Sa type.
UCM0148+2124  Compact (D24 = 7.2 kpc) and low luminosity (Mr = -18.9),
UCM0148+2124  candidate to BCD galaxy.
UCM0150+2032  High inclination (i= 65 degrees) Sc with an emitting knot at SW.
UCM0150+2056  Its prominent bulge component points to Sa type.
UCM0152+2039  Its ambiguous morphological classification and FWHM equal
UCM0152+2039  to PSF point to stellar nature.
UCM0155+2507  UGC 1451, SBb type as in RC3 with the bar at PA = 132+/-2 degrees.
UCM0155+2223  More probably a small Sb type galaxy.
UCM0156+2410  ZWG 482.035, disk dominated profile, Sc type.
UCM0157+2324  NGC 776, SBb with the bar at PA = 137+/-5 degrees and 
UCM0157+2324  northern arm less prominent.
UCM0157+2413  UGC 1479, almost edge-on Sc spiral and Sy 2 (Gallego et
UCM0157+2413  al., 1995).
UCM0157+2102  UGC 1490, previously catalogued as S pec. It presents an emitting
UCM0157+2102  knot near the nucleus, and shows parameters more typical of a Sb.
UCM0158+2354  Prominent bulge component, Sa type.
UCM0159+2327  ZWG 482.050, without type in RC3, Sc according our criteria.
UCM0206+2300N Only known as IRAS02063+2300, Sc galaxy located between
UCM0206+2300  a northern star and the southern galaxy UCM0206+2300S; possible
UCM0206+2300  interaction pair.
UCM0206+2300S Almost face-on Sb galaxy; interaction pair with the northern
UCM0206+2300  companion galaxy.
UCM0206+2330  Disk dominated profile, Sc galaxy.
UCM0214+2404  Previuosly unknown, in spite of its mr = 14.41. Spiral whose
UCM0214+2404  nuclear burst would retard the type to S0-Sa.
UCM0218+2322  UGC 1808, very luminous (Mr = -22.9) Sb galaxy, almost face- on,
UCM0218+2322  with an emitting knot located 16" SE.
UCM1247+2701  KUG1247+270, raindrop aspect, Sc in the Coma cluster (van 
UCM1247+2701  Haarlem et al., 1993).
UCM1253+2926  Compact. Its ambiguous morphological classification and FWHM 
UCM1253+2926  equal to PSF point to stellar nature.
UCM1253+2756  Mrk 53 = KUG1253+279 and CG 930 in the blue objects survey of
UCM1253+2756  Sanduleak & Pesch (1990). Sa in Coma with a bright knot 
UCM1253+2756  to the south.
UCM1254+2932  UV excess object A2-213 (Barbieri & Rosino, 1972; Berger et 
UCM1254+2932  al., 1991). Its ambiguous morphological classification and 
UCM1254+2932  FWHM equal to PSF point to stellar nature.
UCM1254+2741  Sb in Coma, no visible emitting regions outside the nucleus.
UCM1254+2853  Sb in Coma, no visible emitting regions outside the nucleus.
UCM1254+2802  Sc in Coma, disk dominated profile.
UCM1254+2740  Largest component of the Mrk 55 pair in Coma, with properties
UCM1254+2740  of Sa type, no strong interaction signs.
UCM1255+2819  MCG+05-031-035 in Coma, Sb with a knot near the nucleus.
UCM1255+3125  MCG+05-31-33 in Coma and Was 64 in Bothun et al. (1989);
UCM1255+3125  these authors only fit an exponential law to the profile and
UCM1255+3125  observe serious deviations from it in the central regions;
UCM1255+3125  in fact, our B+D decomposition offers an important bulge
UCM1255+3125  contribution, proper for Sa type.
UCM1255+2734  KUG1255+275, Irr in Coma cluster.
UCM1256+2732  Mrk 56 and KUG1256+275, with a knot near the nucleus and 
UCM1256+2732  parameters typical of S0 type, according to Mazzarella
UCM1256+2732  & Balzano (1986). 
UCM1256+2701  Irr in Coma with various emitting knots.
UCM1256+2910  Almost face-on Sb in Coma.
UCM1256+2823  NGC 4858, SBb in Coma (Bothun & Dressler, 1986); parameters
UCM1256+2823  typical of Sb type, but we do not see the bar in our r image;
UCM1256+2823  no apparent conexion with the elliptic NGC 4860 placed 38" NE 
UCM1256+2823  from the UCM object.
UCM1256+2754  Mrk 58, SBa in Coma (Mazzarella & Balzano, 1986); B+D
UCM1256+2754  decomposition profile dominated by the nuclear emission,
UCM1256+2754  but the other parameters point to Sa type, and we do not 
UCM1256+2754  appreciate bar structure.
UCM1256+2722  Sc in Coma with a disk dominated brightness profile.
UCM1257+2754  Although it appears like a face-on galaxy, the disparity between
UCM1257+2754  the five criteria points to its stellar nature; in fact it is 
UCM1257+2754  the planetary nebula H 4-1, 11.87 kpc away (Acker et al., 1992).
UCM1257+2826  Probable Sb in Coma with a possible field star that contaminates
UCM1257+2826  the profile.
UCM1257+2808  Mrk 60, SBa in Coma (Mazzarella & Balzano, 1986) and KUG1257+281, 
UCM1257+2808  although we do not see the bar structure. There are other two 
UCM1257+2808  galaxies 18" SE and 20" S from the UCM Sa object.
UCM1258+2754  ZWG 160.086 and KUG1258+279A, Coma Sa galaxy apparently
UCM1258+2754  asymmetrical maybe due to the presence of dust.
UCM1259+2934  NGC 4922B, northeastern interacting Sy 2 member in a triple
UCM1259+2934  system. Gavazzi et al. (1991) give c31 = 2.83 in the V band, 
UCM1259+2934  similar to our value of 2.93 in the r band. Sb according to
UCM1259+2934  our morphological criteria.
UCM1259+3011  Only known as the object 735 in a Coma catalogue of van Haarlem
UCM1259+3011  et al. (1993), more probably Sa type.
UCM1259+2755  NGC 4926A, S0 pec in RC3 and KUG1259+279; although Gavazzi
UCM1259+2755  et al. (1994) obtain c31 = 3.72 in the V band, a typical value
UCM1259+2755  for Sa type, they classify it as Irr; however, our criteria
UCM1259+2755  and also the direct image point rather to Sa type, according 
UCM1259+2755  to Dressler & Shectman (1988).
UCM1300+2907  Only known as CG 963 in the Case blue survey (Sanduleak
UCM1300+2907  & Pesch, 1990). In our r image it looks like a partially 
UCM1300+2907  distorted spiral Sb in Coma, neighbored by other faint objects.
UCM1300+3136  Almost face-on Sb galaxy in Coma region.
UCM1300+2959  Coma galaxy, only known as PB 3260 blue object in Berger
UCM1300+2959  & Fringant (1977) catalogue; the B+D decomposition profile 
UCM1300+2959  is rather anomalous. Although there is some trend to Sa type,
UCM1300+2959  the morphological criteria are very discrepants between them.
UCM1301+2904  ZWG 160.128 in Coma cluster and KUG1301+290. Gavazzi &
UCM1301+2904  Randone (1994) give mB = 15.56 and mV = 15.21. Sb galaxy
UCM1301+2904  (mr = 15.18) with various HII regions.
UCM1302+2853  KUG1302+288A, Sa Coma galaxy placed 45" W from KUG1302+288B,
UCM1302+2853  but without obvious signs of interaction between them.
UCM1303+2908  Coma galaxy, only known as the blue object PB 3295 (Berger
UCM1303+2908  & Fringant, 1977) and CG 972 (Sanduleak & Pesch, 1990).
UCM1303+2908  Our image shows it like an Irr galaxy, probably merger, with 
UCM1303+2908  various emitting knots.
UCM1304+2808  MCG+05-31-132 and KUG1304+281. Sa galaxy with a bright bulge
UCM1304+2808  component and a knot at SE of the nucleus; the irregular aspect
UCM1304+2808  of some of its isophotes could indicate the presence of dust.
UCM1304+2830  Coma galaxy, very faint (Mr = -17.9) and compact (D24 = 5.2 kpc).
UCM1304+2830  We propose it like a new BCD candidate.
UCM1304+2907  MCG+05-31-133, the interactive fragmented system VV 841 and
UCM1304+2907  KUG1304+291. Irr Coma system with an embeded disk aligned 
UCM1304+2907  near NS direction.
UCM1304+2818  ZWG 160.141 and KUG1304+283. Disk dominated almost face-on Sc
UCM1304+2818  galaxy in Coma cluster.
UCM1306+2938  MCG+05-31-143 and KUG1306+296. In their Coma survey, Gavazzi
UCM1306+2938  et al. (1991) give mV = 14.96 whereas we obtain mr = 14.80.
UCM1306+2938  It presents a knot near the nucleus and photometric parameters
UCM1306+2938  of Sb type.
UCM1307+3111  Sc galaxy in Coma with an off center knot that deviates the
UCM1307+3111  light profile from the disk trend.
UCM1307+2910  NGC 5000, SB(rs)bc in RC3 and Sb (i=35 degrees) in near IR
UCM1307+2910  Coma survey of Gavazzi & Trinchieri (1989) and analyzed in
UCM1307+2910  the van Haarlem et al. (1993) dynamic study. According to
UCM1307+2910  our data it is a very luminous (Mr = -22.3) SBb galaxy
UCM1307+2910  (i = 39+/-4 degrees) with the bar oriented EW.
UCM1308+2958  NGC 5004B, Sb in Gavazzi & Trinchieri (1989) and analyzed in
UCM1308+2958  the van Haarlem et al. (1993) dynamic study of Coma cluster.
UCM1308+2958  Acording to our data, it shows an excess of light between 9"
UCM1308+2958  and 18", maybe denoting the presence of a ring, and there is 
UCM1308+2958  a knot in the NW arm. Its parameters are more typical of a 
UCM1308+2958  Sc type.
UCM1308+2950  NGC 5004 A, SBab in RC3 and in the Gavazzi & Trinchieri (1989)
UCM1308+2950  work. Gavazzi et al. (1990) obtain c31 = 3.13, mV = 14.13 in
UCM1308+2950  the V band and we have c31 = 3.66, mr = 13.92 in the r band.
UCM1308+2950  We obtain SBb type for this luminous galaxy (Mr = -22.0) with 
UCM1308+2950  the bar oriented at PA = 172 degrees. 
UCM1309+2937  Without B+D decomposition, profile with FWHM equal to the
UCM1309+2937  PSF seeing, with anomalous photometric parameters for a galaxy.
UCM1309+2937  Posible star.
UCM1310+3027  Sa galaxy in Coma cluster, very bright nucleus.
UCM1312+3040  ZWG 160.170, Sa type with a knot at NE, barred and probably
UCM1312+3040  ringed.
UCM1312+2954  Disk dominated Sc galaxy. The emission would arise from the 
UCM1312+2954  brigth nucleus.
UCM1313+2938  Was 66 in the Bothun et al. (1989) sample. Sa galaxy with an
UCM1313+2938  appendix at NE, 0.6 mag brigther than obtained by these authors.
UCM1314+2827  Only known as the blue object CG 1001 (Sanduleak & Pesch, 1990). 
UCM1314+2827  It looks very compact, with an anomalous B+D decomposition,
UCM1314+2827  maybe Sa type, although its photometric parameters result
UCM1314+2827  very ambiguous.
UCM1320+2727  Only known as the blue object CG 1019 (Sanduleak & Pesch, 1990).
UCM1320+2727  Faint Sb type galaxy.
UCM1321+2648  MCG+05-32-012, S ring in PGC (Paturel et al., 1989) and
UCM1321+2648  KUG1321+268. SBc galaxy whose deviations in the brightness 
UCM1321+2648  profile probably denote the presence of the bar and a ring
UCM1321+2648  structure.
UCM1324+2926  Was 70, very compact galaxy, 0.6 mag fainter than reported by
UCM1324+2926  Bothun et al. (1989). We obtain D24 = 5.4 kpc and Mr = -18.3,
UCM1324+2926  and we propose it like a BCD candidate.
UCM1324+2651  Pair Mrk 454 (Mazzarella & Balzano, 1986) and KUG1324+268.
UCM1324+2651  Merger system with photometric parameters globally typical
UCM1324+2651  for S0. There is a prominent tail to the south.
UCM1325+2955  Without B+D decomposition, profile with FWHM equal to the
UCM1325+2955  PSF seeing, with anomalous photometric parameters for a galaxy.
UCM1325+2955  Posible star.
UCM1330+3011  Ambiguous photometric classification, probable star.
UCM1331+2900  Was 74, but without photometric information in Bothun et
UCM1331+2900  al. (1989). We propose it like a BCD candidate, very small
UCM1331+2900  (D24 = 6.5 kpc) and faint ( Mr = -18.2).
UCM1428+2727  Mrk 685, Sc in Mazzarella & Balzano (1986) and KUG1428+274.
UCM1428+2727  According to our data it is a Sc galaxy with two bright 
UCM1428+2727  emitting knots at the SW side of the nucleus.
UCM1429+2645  Almost face-on Sc with a fainter companion to the east.
UCM1430+2947  Only known as the blue object CG 1239 in the XIII list of
UCM1430+2947  the Case survey (Stephenson et al., 1992). Bulge dominated
UCM1430+2947  system, more probably S0 type galaxy.
UCM1431+2854  ZWG 136.078, probably Sb galaxy with a bright value for the 
UCM1431+2854  central surface brightness of the disk component.
UCM1431+2702  Probably Sb galaxy neighbored by various objects, althoug we 
UCM1431+2702  do not appreciate obvious signs of interaction between them.
UCM1431+2947  Only known as the blue object CG 1240 in the XIII list of
UCM1431+2947  the Case survey (Stephenson et al., 1992). This authors
UCM1431+2947  remark about the H-alpha emission suspected on III-F plate,
UCM1431+2947  confirmed now by our survey. We propose it like a BCD 
UCM1431+2947  candidate (D24 = 9 kpc and Mr = - 18.3).
UCM1431+2814  Sa galaxy with its major apparent axis oriented at PA = 115 deg.
UCM1432+2645  UGC 9384, IC 4461, VV 303, spiral of the multiple system
UCM1432+2645  Arp 95 in PGC. The UCM object is a SBb with the bar at PA = 132
UCM1432+2645  degrees and presents a knot at 8" NW. The bar is oriented to
UCM1432+2645  the eastern lenticular IC 4462, although there is no obvious
UCM1432+2645  interaction signs with it.
UCM1439+2439  Almost face-on Sc galaxy, with a faint object (mr = 18.43) 
UCM1439+2439  12" SW from the UCM, but without conexion signs.
UCM1440+2521S Southern member of the pair UGC 9489. Sb type with an appendix
UCM1440+2521  to the SW.
UCM1440+2511  Although its B+D decomposition indicates early type,
UCM1440+2511  the remaining criteria points to Sb morphology.
UCM1440+2521N Northern member of the pair UGC 9489. This Sa galaxy is 0.4 mag
UCM1440+2521  brigther than the south companion, and both present the same
UCM1440+2521  apparent inclination (i = 60 degrees).
UCM1442+2845  MCG+05-35-009 and IC 4497. Although it is previously catalogued
UCM1442+2845  as S0 uncertain in RC3, our data point to later Hubble type, Sb.
UCM1442+2845  Its central isophotes shape denote the presence of dust.
UCM1443+2714  ZWG 164.019. Sa galaxy with a prominent bulge component, Sy 2
UCM1443+2714  in de Grijp et al. (1987) and also according our spectroscopic
UCM1443+2714  analysis (Gallego et al., 1995).
UCM1443+2844  MCG+05-35-014. SBc with the bar oriented at PA = 121 degrees.
UCM1443+2844  The northern arm appears more prominent denoting the presence
UCM1443+2844  of dust and there are two knots at NE and SE directions.
UCM1443+2548  ZWG 134.030. Disk dominated system, Sc+.
UCM1444+2923  Almost face-on galaxy, S0 type with faint value of central
UCM1444+2923  surface brightness of the disk component.
UCM1445+2855  Probably Sb galaxy, although the faint neighbor object
UCM1445+2855  (mr = 20.2) contaminates the light profile, difficulting
UCM1445+2855  its classification.
UCM1447+2535  UGC 9544 and MCG+04-35-010, uncertain spiral in RC3. Very
UCM1447+2535  luminous galaxy (Mr= -23.04, D24 = 67 kpc) with photometric
UCM1447+2535  parameters pointing to S0-Sa type.
UCM1449+2844  ZWG 164.035, Sc+ with the major axis at PA = 116 degrees.
UCM1451+2954  Almost face-on Sb without extranuclear emitting regions.
UCM1452+2754  Sb type galaxy. The drop in the profile between 2.5" and 4.5"
UCM1452+2754  and the image denote the presence of dust.
UCM1506+1922  MCG+03-39-008 and ZWG 106.010. The B+D decomposition reveals
UCM1506+1922  an important bulge component, but the rest of the criteria
UCM1506+1922  points to Sb.
UCM1513+2012  ZWG 106.023. Distorted galaxy, especially at the north region
UCM1513+2012  and with an emitting knot near the nucleus, difficulting the B+D
UCM1513+2012  decomposition. The majority of the criteria points to S0 type.
UCM1537+2506S Southern and fainter member of the Mrk 860 interacting pair.
UCM1537+2506  SBa galaxy with the northern arm in contact with its companion.
UCM1537+2506N Northern member of the Mrk 860 system, 15" N and 20" E from 
UCM1537+2506  UCM1537+2506S. Parameters proper for SBb type.
UCM1557+1423  Sb galaxy with two field stars at the N and S directions.
UCM1604+1642  Sc galaxy with the major axis at PA = 40 degrees.
UCM1608+1335  Without B+D decomposition, profile with FWHM equal to the PSF
UCM1608+1335  seeing, with anomalous photometric parameters for a galaxy. 
UCM1608+1335  Field star.
UCM1612+1308  Very faint galaxy (D24 = 3 kpc, Mr = -16.7), candidate to BCD.
UCM1646+2725  Disk dominated Sc+, with the emitting region off centered.
UCM1647+2950  ZWG 169.004 and KUG1647+298, compact in Kiso survey (Takase
UCM1647+2950  & Miyauchi-Isobe, 1993). Our image reveals it as a luminous SBc
UCM1647+2950  with a dusty region at the north distorting the shape of the
UCM1647+2950  central isophotes.
UCM1647+2729  ZWG 169.005 and KUG1647+274. B+D decomposition dominated by
UCM1647+2729  the disk component, developed arms, Sb galaxy.
UCM1647+2727  Almost face-on galaxy close to another galaxy (8" W) that 
UCM1647+2727  contaminates the outermost isophotes of the main object,
UCM1647+2727  difficulting its classification, although probably it is a
UCM1647+2727  Sa galaxy.
UCM1648+2855  Mrk 1108, without morphology in Mazzarella & Balzano (1986)
UCM1648+2855  and spherical compact in Kiso survey (KUG1648+289). According 
UCM1648+2855  our r data, it is a Sa galaxy with various emitting 
UCM1648+2855  circumnuclear regions.
UCM1651+2721  Without B+D decomposition, profile with FWHM equal to the PSF 
UCM1651+2721  seeing, with anomalous photometric parameters for a galaxy.
UCM1651+2721  Field star.
UCM1651+3017  The southeastern star contaminates the profile of the galaxy,
UCM1651+3017  probably Sb type. Overlapping efect of the two spectra at the
UCM1651+3017  objective-prism plate can not be discarded, causing a false
UCM1651+3017  emission feature.
UCM1654+2812  Disk dominated Sc+, with an off centered emitting region.
UCM1655+2755  NGC 6264, very luminous Sb (D24 = 43.5 kpc and Mr = -22.2),
UCM1655+2755  probably barred and ringed. Sy 2 according to our data
UCM1655+2755  (Gallego et al., 1995).
UCM1656+2845  Sb galaxy, previously unknown, in spite of its apparent size 
UCM1656+2845  and magnitude (39" x 15" and mr = 15.13).
UCM1656+2744  Although its B+D decomposition appears clearly bulge dominated,
UCM1656+2744  the remaining criteria point to Sa type.
UCM1657+2901  KUG1657+290. Disk dominated Sc, according to our r data.
UCM1659+2928  Mrk 504, barred and Sy 1 spiral in Mazzarella & Balzano (1986)
UCM1659+2928  and KUG1659+294. Really, according our data it is a SB0
UCM1659+2928  very bright (D24 = 35 kpc and Mr = -22.0) galaxy and Sy1
UCM1659+2928  (Gallego et al., 1995).
UCM1701+3131  Mrk 700, LINER in Mazzarella & Balzano (1986), but Sy 1 in 
UCM1701+3131  Gallego et al. (1995) as in Weedman (1978) and it is 
UCM1701+3131  KUG1701+315 in Takase & Miyauchi-Isobe (1993) survey.
UCM1701+3131  Asymmetric spiral, with photometric parameters proper for 
UCM1701+3131  a S0 type and presents a prominent tail pointing to the SW
UCM1701+3131  and a faint residual interacting feature at the opposite
UCM1701+3131  direction.
UCM2238+2308  UGC 12148 and KUG2238+231. In our r image it presents a bright
UCM2238+2308  nucleus (Sa type) with various HII regions. UGC 12153, that 
UCM2238+2308  presents a merger aspect, it is 2.'9 far from the UCM and
UCM2238+2308  although both of them present the same z, the latter was not 
UCM2238+2308  selected in our survey due to the uncertainty in its emission
UCM2238+2308  feature appearance.
UCM2239+2402  Without B+D decomposition, profile with FWHM equal to the PSF
UCM2239+2402  seeing, with anomalous photometric parameters for a galaxy.
UCM2239+2402  It would be a field star. 15" SW from our object it is a galaxy
UCM2239+2402  with an emitting region at the SE of the nucleus, but it was 
UCM2239+2402  not selected in our exploration due to it is at z = 0.08, out
UCM2239+2402  of the region of detectability in our prism-objective technique.
UCM2239+1959  Mrk 308, Irr in RC3 and compact with halo, KUG2239+199, in 
UCM2239+1959  Takase & Miyauchi-Isobe (1993). In our r image it appears like
UCM2239+1959  a S0 distorted at the NE region, pointing to another emitting 
UCM2239+1959  galaxy, at the same z, placed at 54" from UCM. This points to
UCM2239+1959  an emitting system caused by interaction.
UCM2244+2049  NGC 7375, S(r) in PGC. This ringed structure would cause the
UCM2244+2049  observed raise in the profile between 12" and 20". We classify
UCM2244+2049  it as S(r)0.
UCM2249+2149  In spite of its size and luminosity (D24 = 54 kpc and Mr = -22.5)
UCM2249+2149  this Sa galaxy was previously unknown.
UCM2250+2427  Mrk 309, Wolf-Rayet dominated nucleus galaxy in Osterbrock
UCM2250+2427  & Cohen (1982), and KUG2250+244. Luminous Sa (D24 = 42.6, and
UCM2250+2427  Mr = -22.4) with various HII regions outside the nucleus.
UCM2250+2427  Southern arm more prominent.
UCM2251+2352  Disk dominated system, probably Sc type. The object placed
UCM2251+2352  19" SW from the UCM it is a bright field star.
UCM2253+2219  KUG2253+223. Sa galaxy with its apparent major axis at PA = 33
UCM2253+2219  degrees. No extranuclear knots are observed in the r image.
UCM2255+1930S ZWG 453.031, probably Sb type, 30" SW from UCM2255+1930N, both
UCM2255+1930  with the same z, but without apparent signs of interaction 
UCM2255+1930  between them.
UCM2255+1930N UGC 12265, main component in the ZWG 453.031 multiple system.
UCM2255+1930  Sb galaxy, 0.6 mag brigther than the south member.
UCM2255+1926  Disk dominated Sc with a bright knot at SE.
UCM2255+1654  High inclination (i = 69+/-2 degrees) Sc near another compact
UCM2255+1654  galaxy placed at NE direction.
UCM2256+2002  UGC 12278, Sc-Sd in RC3. In our r profile there is an excess
UCM2256+2002  of light betwwen 9" and 18", maybe denoting a ring, although
UCM2256+2002  there is no evident in the image. Its morphological parameters
UCM2256+2002  point to Sc+ type.
UCM2257+2438  Only previously known as KAZ 320 (Kazaryan & Kazaryan, 1980).
UCM2257+2438  Our spectroscopic, near IR and IRAS data (Zamorano et al., 1992)
UCM2257+2438  indicate that it is a Sy 1 nucleus, and our r data, especially
UCM2257+2438  the bulge dominated profile, point to early type, more 
UCM2257+2438  probably S0.
UCM2258+1920  ZWG 453.046 and KUG2258+193. Disk dominated, Sc system with 
UCM2258+1920  its eastern arm more prominent.
UCM2300+2014  Almost face-on galaxy with photometric parameters more typical
UCM2300+2014  for a Sb.
UCM2302+2053W Faintest Sb component of a pair of spirals, both at the same z
UCM2302+2053  and possibly in interaction.
UCM2302+2053E ZWG 453.065, brightest Sb component of a pair of spirals,
UCM2302+2053  both at the same z, and with its southern arm pointing to the
UCM2302+2053  companion, possibly denoting an interaction.
UCM2303+1856  ZWG 453.067, high inclination (i = 61+/-1 degrees) galaxy. 
UCM2303+1856  There is a star 7" E contaminating the profile and dificulting
UCM2303+1856  its classification, but it could be a Sa type.
UCM2303+1702  Our spectroscopic, near IR and IRAS data (Rego et al., 1994)
UCM2303+1702  indicate that it is a Sy 2 nucleus, and our r data, especially
UCM2303+1702  the disk dominated profile, point to Sc type.
UCM2304+1640  Very compact galaxy (D24 = 7 kpc and Mr = -18.1) in a populated 
UCM2304+1640  environment, although there is no signs of interactions.
UCM2304+1640  Candidate to BCD galaxy.
UCM2305+1621  Anomalous B+D decomposition, and inconclusive classification, 
UCM2305+1621  although it could be an almost face-on Sa galaxy.
UCM2306+1703  Disk dominated, Sc  with a bright region at the SW arm.
UCM2306+1947  ZWG 454.001 and KARA 1007. Sb type with i = 50+/-5 degrees.
UCM2307+2118  Without B+D decomposition, profile with FWHM equal to the PSF
UCM2307+2118  seeing, with anomalous photometric parameters for a galaxy.
UCM2307+2118  Field star. Its spectrum (Gallego et al., 1995) indicates that
UCM2307+2118  it is a symbiotic star.
UCM2310+1800  Disk dominated almost face-on Sc galaxy.
UCM2312+2500  NGC 7548, lenticular and double ringed galaxy in RC3. Our
UCM2312+2500  brightness profile reveals oscilations that would indicate
UCM2312+2500  the presence of these rings. We obtain D24 = 48 kpc, Mr = -22.8
UCM2312+2500  and S(r)a classification.
UCM2313+1842  Probably Sb, with a field star at NW contaminating the profile.
UCM2315+1625  ZWG 454.027 and MCG+3-59-29. A very bright star contaminates 
UCM2315+1625  the brightness profile and force us to truncate it, so its
UCM2315+1625  classification is very difficult, although it could be a
UCM2315+1625  S0 galaxy.
UCM2315+1923  Bulge component relatively important, Sa type.
UCM2315+1658  The faintest object in the sample (mr = 20.5). Without B+D
UCM2315+1658  decomposition, profile with FWHM equal to the PSF seeing,
UCM2315+1658  with anomalous photometric parameters for a galaxy. Field star.
UCM2315+1658  There is another object 2.8" NW far from the UCM and fainter
UCM2315+1658  (mr = 21.6) than ours. 
UCM2316+2457  Mrk 319, SBa in RC3 and KUG2316+249. According to our data it is
UCM2316+2457  a luminous SBa galaxy (Mr = -22.8) with various HII regions.
UCM2316+2459  ZWG 475.061 and KARA 72581B. Disk dominated galaxy, Sc, with 
UCM2316+2459  its southern arm more prominent and a bright knot in the north.
UCM2316+2028  Small Sc galaxy without emitting knots outside the nucleus.
UCM2317+1607  Sa with a prominent bulge component.
UCM2317+2356  NGC 7620, Mrk 321 and KUG2317+239. The brightest spiral galaxy 
UCM2317+2356  of our sample (D24 = 50 kpc, Mr = -23.5) with various HII
UCM2317+2356  regions. Our data in the red band delay the Hubble type to Sa,
UCM2317+2356  indicating nuclear emission stronger than in the B band that 
UCM2317+2356  assigns it Scd type in RC3.
UCM2319+2234  KUG2319+225. Although it is described as spheroidal compact 
UCM2319+2234  in Kiso survey, it is a Sc galaxy with i = 49o, placed 30" NE
UCM2319+2234  from another brighter and spheroidal object but without
UCM2319+2234  emission lines.
UCM2319+2243  Bulge dominated profile, S0 galaxy, previously unknown in spite
UCM2319+2243  of its bright apparent magnitude (mr = 14.75).
UCM2320+2428  ZWG 476.027 and KAZ 332. Almost edge-on Sa galaxy.
UCM2321+1631  NGC 7647, elliptical galaxy in RC3. It is the brightest galaxy 
UCM2321+1631  in the sample (Mr = -23.6). This object is a cD galaxy with 
UCM2321+1631  a red envelope that would explain the apparent disk component
UCM2321+1631  obtained with our B+D decomposition and the consequent S0 
UCM2321+1631  missclassification.
UCM2321+2149  Disk dominated Sc galaxy, with asymmetric arms maybe denoting
UCM2321+2149  the presence of dust.
UCM2321+2506  ZWG 476.030 and KUG2321+251. Sc galaxy with i = 57 degrees
UCM2321+2506  and whose emission would arise from the nucleus.
UCM2322+2218  Sc+, without specific emitting regions outside the nucleus.
UCM2323+2047  Previously unknown in spite of its bright apparent magnitude
UCM2323+2047  (mr = 14.84). The image and the excess of light between 6"
UCM2323+2047  and 12" observed in the profile denote the presence of a bar
UCM2323+2047  at PA = 65 degrees. We classify it as SBb.
UCM2323+2252  Without B+D decomposition, profile with FWHM equal to the PSF
UCM2323+2252  seeing, with anomalous photometric parameters for a galaxy.
UCM2323+2252  Field star.
UCM2324+2448  NGC 7664, Sc in RC3. Nearby spiral (z = 0.01230). The apparent
UCM2324+2448  off centered nucleus would denote the presence of dust.
UCM2325+1628  Anomalous B+D decomposition. One of the two faintest objects 
UCM2325+1628  of the UCM sample (D24 = 3 kpc, Mr = -16.7). BCD candidate.
UCM2325+1815  MCG+03-59-58. Very luminous Sb galaxy (D24 = 55 kpc, Mr = -22.4),
UCM2325+1815  almost face-on, and with various HII regions.
UCM2325+1945  ZWG 454.070. Sb with its western arm more prominent. The galaxy
UCM2325+1945  at SE direction does not present conexion with our object.
UCM2325+2208  NGC 7678, SAB(rs)c in RC3, UGC 12614 and KUG2325+221. It is
UCM2325+2208  a SBc with prominent arms, specially the southern one, and 
UCM2325+2208  with various HII regions. Kent (1985b) obtains dL = 6.34 kpc,
UCM2325+2208  but without considering a bulge component, whereas our B+D 
UCM2325+2208  method gives dL = 8.2 kpc.
UCM2326+2435  High inclination galaxy (i = 72+/-2 degrees) with a knot placed
UCM2326+2435  at 3" NW from the nucleus that could delay the Hubble type to Sa.
UCM2327+2515N Northern component of the system ZWG 476.055. Although its
UCM2327+2515  profile results contaminated by a star at the north and by
UCM2327+2515  its southern companion, it would be a Sb.
UCM2327+2515S Southern member, probably S0, of the pair ZWG 476.055, both
UCM2327+2515  galaxies with the same z. The SW tail indicates a sign of
UCM2327+2515  interaction.
UCM2329+2427  ZWG 476.060. The asymmetric aspect of the arms could denote
UCM2329+2427  the presence of dust, mainly at the NW direction, in this
UCM2329+2427  Sb galaxy.
UCM2329+2500  Only known as KAZ 341. The brightness profile and the direct
UCM2329+2500  image reveal an excess of light from 8" due to the presence 
UCM2329+2500  of a ring, as confirmed by the sustraction of a r1/4
UCM2329+2500  bidimensional model (Gallego et al., 1994). These authors also
UCM2329+2500  claim the presence of a Sy 1 nucleus in this galaxy.
UCM2329+2511  Small Sa galaxy with an important bulge contribution.
UCM2331+2214  Sb with a bright off centered region distorting the isophotes.
UCM2332+1723  Sa galaxy with an emitting knot 2" W from the nucleus.
UCM2333+2248  A bright knot 4.7" SE from the nucleus distorts the isophotes 
UCM2333+2248  of this galaxy, with typical parameters of a Sc type.
UCM2333+2359  S0 dominated by the Sy 1 activity of its nucleus. It draws
UCM2333+2359  an equilateral triangle with two fainter galaxies (20" S and
UCM2333+2359  20" SW from the UCM).
UCM2344+2157  Without B+D decomposition, profile with FWHM equal to the PSF
UCM2344+2157  seeing, with anomalous photometric parameters for a galaxy.
UCM2344+2157  Field star.
UCM2346+2011  Without B+D decomposition, profile with FWHM equal to the PSF
UCM2346+2011  seeing. Anomalous photometric parameters for a galaxy. Probable
UCM2346+2011  field star.
UCM2348+2407  Brightness profile contaminated by a field star which dificults
UCM2348+2407  its classification, although it would more probably be a Sa.
UCM2351+2321  Small Sb withouth specific features outside its nucleus.
UCM2357+2440  Without B+D decomposition, profile with FWHM equal to the PSF
UCM2357+2440  seeing, with anomalous photometric parameters for a galaxy, 
UCM2357+2440  especially the bright mean surface brightnesses. Field star.
UCM2357+2241  Without B+D decomposition, profile with FWHM equal to the PSF
UCM2357+2241  seeing, with anomalous photometric parameters for a galaxy, 
UCM2357+2241  especially the mean surface brightnesses. Field star.