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Table 1. Continued

IAU Name Other Name alpha (1950) delta (1950) z B Ext (B) Morph. Type Ref(Ident.) Ref(z) Ref(B,Ext (B))

2302+1916 CGCG453-062 23 02 28.5 +19 16 57 0.025097 15.1 0.13 ... NED NED NED
2311-4259 ESO291-G009 23 11 12.2 -42 59 59 0.056396 14.64 ... SA0- 957 957 895
2312-5919N ESO148-IG002N 23 12 51.0 -59 19 40 0.044601 15.17 0.00 Merger DM97 NED NED
2313+2516 b IC5298 23 13 33.1 +25 17 01 0.027342 14.94 0.27 Spiral Wu98 NED NED
2315+0618 NGC7591 23 15 43.9 +06 18 45 0.016531 13.86 0.18 SBbc K95 NED NED
2315-0441B NGC7592B 23 15 47.3 -04 41 22 0.024617 11.4 0.10 Sab?;p MB93 NED NED
2316+0537 IC1481 23 16 52.6 +05 37 57 0.020407 14.39 0.21 S? VCV7 VCV7 HUC
2318+0756 NGC7626 23 18 10.3 +07 56 35 0.011418 12.16 0.16 E;pec Ho97 NED NED
2322-1223 NPM1G-12.0625 23 22 43.8 -12 23 56 0.082200 15.4 0.08 E 559 559 108
2322+2813 UGC12591 23 22 53.5 +28 13 14 0.023179 13.90 0.29 S0/a K84 NED NED
2323-6926 IRAS2323-6926 23 23 02.7 -69 26 47 0.106307 16.6 0.06 Merger DM97 NED NED
2336+3604 IRAS2336+3604 23 36 32.2 +36 04 32 0.064480 16.3 0.52 ... NED NED NED
2339-0356A ARP195A 23 39 13.2 -03 56 42 0.022856 14.5 0.09 Sc KK85 NED NED
2341+1029 a NGC7742 23 41 43.1 +10 29 25 0.005514 12.35 0.10 SA(r)b Ho97 NED NED
2341+0939 NGC7743 23 41 48.6 +09 39 25 0.005704 12.38 0.17 (R)SB(s)0+ HUC VCV HUC
2344+2912 NGC7753 23 44 33.3 +29 12 21 0.017239 12.83 0.19 SAB(rs)bc KK85 NED NED
2348+1949C b NGC7769 23 48 31.2 +19 52 19 0.014036 12.77 0.11 (R)SA(rs)b Wu98 NED NED
2350+0326 UM011 23 50 45.1 +03 26 23 0.038000 14.9 0.17 ... VCV VCV ...
2354-3502 ESO349-G010 23 54 25.9 -35 02 12 0.049051 13.86 ... E+4;cD 957 NED ESO
2354-3457 ESO349-G009 23 54 26.0 -34 57 32 0.042069 14.6 ... (R'1)SB(rs)b 957 NED 895
2358+3109 NGC7805 23 58 53.1 +31 09 20 0.016178 14.2 0.16 SAB0;pec KK85 NED NED

Particular classification preferences expressed by the respective authors of the cited data:
a Transition objects that are Liner/HII-nucleus systems; Ho et al. 1993; Ho et al. 1997.
b Mixture type with properties of both Liner and HII galaxy; Wu et al. 1998.
c L/H emission class; Keel et al. 1985.
d Ambiguous objects between HII galaxies and Liners; Veilleux, Sanders & Kim 1997.
e Two criteria favor Liner and one to Starburst; Duc, Mirabel & Maza 1997.

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