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Bibliography

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Popescu, C. C., Hopp, U., Hagen, H.-J., & Elsässer, H. 1996, A&AS, 116, 43

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Pustilnik, S. A., Engels, D., Ugryumov, A. V., et al. 1999, A&AS, 135, 299 (Paper II)

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Pustilnik, S. A., Kniazev, A. Y., Lipovetsky, V. A., & Ugryumov, A. V. 2001, A&A, in press = astro-ph/0104334

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Vennik, J., Hopp, U., & Popescu, C. C. 2000, A&AS, 142, 399


 
Table 3: Coordinates, Velocities and Magnitudes of Emission-Line Galaxies
# Name $\alpha\,(1950)$ $\delta\,(1950)$ $V_{hel}^{\,a}\pm\sigma_V$ mB M $_{B}^{\;\;b}$ Type Other names from NED
                and number of reference
  (1) (2) (3) (4) (5) (6) (7) (8)
1 HS 0809+4334 08 09 01.5 +43 34 17 14146 $\pm$ 57 18.4 -18.0 BCG  
2 HS 0818+4234 08 18 40.5 +42 34 23 17424 $\pm$ 68 19.7 -17.1 NON  
3 HS 0822+4049 08 22 25.1 +40 49 57 12087 $\pm$ 100 17.3 -18.7 BCG  
4 HS 0822+4238 08 22 50.9 +42 38 24 11637 $\pm$ 60 18.2 -17.8 BCG  
5 HS 0824+4139 08 24 11.6 +41 39 00 10784 $\pm$ 53 18.4 -17.4 BCG? IRAS F08241+4139
6 HS 0828+4305 08 28 04.6 +43 05 24 10700 $\pm$ 86 16.7 -19.0 SBN  
7 HS 0828+4346 08 28 32.0 +43 46 24 7649 $\pm$ 62 18.4 -16.6 BCG  
8 HS 0831+4208 08 31 14.5 +42 08 17 44859 $\pm$ 56 +17.3 -21.5 SBN MBWU023
9 HS 0849+3802$^\ddagger$ 08 49 09.9 +38 02 27 13368 $\pm$ 71 16.9 -19.4 SBN IRAS F08491+3802
10 HS 0849+3639$^\ddagger$ 08 49 34.0 +36 39 14 7503 $\pm$ 47 20.0 -15.0 BCG  
11 HS 0850+3722$^\ddagger$ 08 50 17.5 +37 22 40 14925 $\pm$ 68 +18.7 -17.8 NON  
12 HS 0855+4118 08 55 02.3 +41 18 44 8113 $\pm$ 80 17.0 -18.2 BCG?  
13 HS 0855+3729$^\ddagger$ 08 55 27.6 +37 29 06 14921 $\pm$ 59 17.5 -19.0 SBN  
14 HS 0900+4318 09 00 26.4 +43 18 52 2421 $\pm$ 95 18.5 -14.0 BCG MBWU369
15 HS 0901+3517$^\ddagger$ 09 01 17.6 +35 17 29 12397 $\pm$ 95 18.2 -17.9 BCG?  
16 HS 0904+3752$^\ddagger$ 09 04 29.2 +37 52 27 6803 $\pm$ 86 18.4 -16.4 DANS? FGC0841
17 HS 0907+4201 09 07 43.6 +42 01 48 12004 $\pm$ 104 17.1 -18.9 SBN  
18 HS 0912+4427 09 12 08.2 +44 27 26 11637 $\pm$ 101 17.4 -18.6 DANS?  
19 HS 0912+4259 09 12 23.6 +42 59 50 14268 $\pm$ 53 16.4 -20.0 SBN IRAS F09123+4259
20 HS 0912+4433 09 12 28.7 +44 33 55 11345 $\pm$ 92 17.3 -18.6 BCG  
21 HS 0912+3900$^\ddagger$ 09 12 38.2 +39 00 21 20628 $\pm$ 92 17.2 -20.0 SBN NPM1G+39.0196
22 HS 0923+4021 09 23 13.8 +40 21 32 5190 $\pm$ 110 17.2 -17.0 BCG  
23 HS 0927+4159 09 27 00.6 +41 59 35 13533 $\pm$ 95 17.4 -18.9 BCG  
24 HS 0934+4150 09 34 21.3 +41 50 29 12011 $\pm$ 74 17.0 -19.0 BCG KUG0934+418
25 HS 0934+4256 09 34 53.9 +42 56 20 3600 $\pm$ 44 17.2 -16.2 DANS KUG0934+429
26 HS 0935+4135 09 35 30.7 +41 35 07 79288 $\pm$ 300 18.0 -22.1 LINER  
27 HS 0938+4215 09 38 49.6 +42 15 40 4680 $\pm$ 98 17.6 -16.4 BCG  
28 HS 0939+4124 09 39 37.2 +41 24 03 13646 $\pm$ 62 18.5 -17.8 BCG  
29 HS 0940+4052 09 40 08.1 +40 52 28 18255 $\pm$ 44 16.1 -20.8 BCG?  
30 HS 0941+4024A 09 41 54.7 +40 24 52 21709 $\pm$ 20 +17.2 -20.1 SBN FIRSTJ094501.7+40110
31 HS 0941+4024B 09 41 56.2 +40 24 53 21724 $\pm$ 14 16.6 -20.7 BCG?  
32 HS 0947+3526$^\ddagger$ 09 47 59.6 +35 26 39 4678 $\pm$ 44 16.4 -17.6 BCG KUG0947+354
33 HS 0948+3723 09 48 19.0 +37 23 05 5140 $\pm$ 37 +17.8 -16.4 BCG 6
34 HS 0951+3712$^\ddagger$ 09 51 40.6 +37 12 07 12275 $\pm$ 65 16.9 -19.2 SBN FIRSTJ095440.9+36575
35 HS 0952+4024$^\ddagger$ 09 52 30.8 +40 24 28 8648 $\pm$ 50 17.3 -18.0 DANS  
36 HS 0953+3628 09 53 16.5 +36 28 41 14435 $\pm$ 101 17.3 -19.1 BCG CG 308, 5
37 HS 0954+3615$^\ddagger$ 09 54 35.4 +36 15 47 5193 $\pm$ 68 18.4 -15.8 BCG  
38 HS 0956+3702$^\ddagger$ 09 56 08.4 +37 02 05 15679 $\pm$ 74 16.7 -19.9 SBN  
39 HS 0958+3654$^\ddagger$ 09 58 27.9 +36 54 43 12265 $\pm$ 300 17.4 -18.7 SBN? CGCG182-058, 8
40 HS 0958+3637 09 58 29.2 +36 37 30 13134 $\pm$ 75 17.6 -18.6 DANS?  



Table 3. (Continued)

# Name $\alpha\,(1950)$ $\delta\,(1950)$ $V_{hel}^{\,a}\pm\sigma_V$ mB M $_{B}^{\;\;b}$ Type Other names from NED
                and number of reference
  (1) (2) (3) (4) (5) (6) (7) (8)
41 HS 0958+3718 09 58 15.5 +37 18 38 1606 $\pm$ 77 15.7 -16.0 BCG CG 315,KUG0958+373, 5
42 HS 1004+3730$^\ddagger$ 10 04 22.3 +37 30 22 10133 $\pm$ 94 16.5 -19.2 SBN KUG1004+375
43 HS 1008+3620$^\ddagger$ 10 08 01.5 +36 20 51 11424 $\pm$ 53 17.2 -18.7 BCG  
44 HS 1011+3604 10 11 29.6 +36 04 55 10227 $\pm$ 65 17.5 -18.2 DANS?  
45 HS 1014+3535$^\ddagger$ 10 14 50.0 +35 35 50 26718 $\pm$ 72 17.6 -20.2 SBN KUG1014+355
46 HS 1016+3733 10 16 02.7 +37 33 04 14451 $\pm$ 78 16.1 -20.3 LINER KUG1016+375
47 HS 1021+4839 10 21 39.0 +48 39 53 7495 $\pm$ 69 16.7 -18.3 SBN?  
48 HS 1025+3707A 10 25 12.7 +37 07 08 7503 $\pm$ 102 17.9 -17.1 BCG  
49 HS 1025+3707B 10 25 13.7 +37 07 10 39650 $\pm$ 300 +16.9 -21.7 SBN  
50 HS 1025+3658$^\ddagger$ 10 25 32.3 +36 58 28 10988 $\pm$ 59 16.9 -18.9 BCG  
51 HS 1025+4057 10 25 51.0 +40 57 52 16482 $\pm$ 59 16.7 -20.0 SBN  
52 HS 1027+4728 10 27 45.9 +47 28 57 18225 $\pm$ 100 17.6 -19.3 SBN  
53 HS 1028+3716 10 28 24.8 +37 16 15 11137 $\pm$ 109 16.9 -19.0 DANS KUG1028+372
54 HS 1032+4600 10 32 21.2 +46 00 11 9299 $\pm$ 61 17.1 -18.4 BCG? KUG1032+460
55 HS 1043+3852$^\ddagger$ 10 43 09.0 +38 52 15 10071 $\pm$ 60 +18.9 -16.7 BCG  
56 HS 1122+3800$^\ddagger$ 11 22 53.7 +38 00 33 11438 $\pm$ 98 +18.7 -17.2 BCG  
57 HS 1148+3732 11 48 05.4 +37 32 22 10835 $\pm$ 51 17.5 -18.3 DANS KUV11481+3732, 14
58 HS 1159+3940 11 59 52.5 +39 40 59 6299 $\pm$ 29 +17.4 -17.2 DANS 6
59 HS 1200+3824 12 00 41.7 +38 24 01 23983 $\pm$ 146 +18.0 -19.4 SBN? MAPS-NGPO 266 006267
60 HS 1201+3535 12 01 17.6 +35 35 08 10216 $\pm$ 11 19.0 -16.7 BCG MAPS-NGPO 267 026327
61 HS 1202+3732 12 02 36.8 +37 32 55 6787 $\pm$ 7 +18.7 -16.1 BCG MAPS-NGPO 267 0065953
62 HS 1204+3945 12 04 45.2 +39 45 47 11178 $\pm$ 195 18.0 -17.9 BCG?  
63 HS 1205+3940 12 05 29.2 +39 40 19 6362 $\pm$ 14 18.1 -16.5 BCG CG 1517
64 HS 1206+4012 12 06 19.8 +40 12 24 26721 $\pm$ 300 18.1 -19.7 NON  
65 HS 1210+3831 12 10 46.7 +38 31 42 15800 $\pm$ 66 16.9 -19.7 BCG? CG 1538
66 HS 1211+3807 12 11 20.1 +38 07 27 7433 $\pm$ 133 16.3 -18.7 BCG MAPS-NGPO 267 004482
67 HS 1211+4012 12 11 51.5 +40 12 23 7091 $\pm$ 23 18.3 -16.6 BCG  
68 HS 1212+3640 12 12 09.5 +36 40 57 12704 $\pm$ 56 16.5 -19.6 BCG KUG1212+366
69 HS 1213+3636A 12 13 03.8 +36 36 56 522 $\pm$ 35 17.5: -11.7: BCG  
70 HS 1213+3636B 12 13 04.1 +36 36 31 229 $\pm$ 38 17.3  -9.6 SA in SBm in NGC 4214
71 HS 1215+3850 12 15 46.7 +38 50 07 15702 $\pm$ 65 16.1 -20.5 BCG? CG 1553
72 HS 1216+3743 12 16 38.5 +37 43 24 5978 $\pm$ 124 17.9 -16.6 DANS MAPS-NGPO 267 007023
73 HS 1218+3945 12 18 52.5 +39 45 44 11475 $\pm$ 57 17.7 -18.2 BCG  
74 HS 1220+3845 12 20 11.8 +38 45 38 57118 $\pm$ 57 +17.8 -21.6 Sy2  
75 HS 1223+3938 12 23 29.6 +39 38 31 10873 $\pm$ 69 16.8 -19.0 BCG NPM1G+39.0289,CG 1566, 2, 7
76 HS 1224+4027 12 24 42.2 +40 27 56 17724 $\pm$ 5 18.6 -18.3 BCG  
77 HS 1225+4129 12 25 45.5 +41 29 16 11411 $\pm$ 17 18.7 -17.2 BCG  
78 HS 1226+4113 12 26 55.8 +41 13 52 3845 $\pm$ 17 18.7 -14.9 BCG  
79 HS 1232+3834 12 32 25.0 +38 34 31 4049 $\pm$ 57 +16.8 -16.9 BCG MAPS-NGPO 218 110114
80 HS 1232+3947 12 32 54.6 +39 47 39 6506 $\pm$ 143 17.2 -17.5 BCG 2, 7
81 HS 1235+4232 12 35 13.7 +42 32 02 7449 $\pm$ 90 18.4 -16.6 DANS?  
82 HS 1236+3821 12 36 31.9 +38 21 52 2069 $\pm$ 103 15.4 -16.8 BCG UGC 7816,CGCG1236.5+3822,
                NPM1G+38.0259, 2, 7



Table 3. (Continued)

# Name $\alpha\,(1950)$ $\delta\,(1950)$ $V_{hel}^{\,a}\pm\sigma_V$ mB M $_{B}^{\;\;b}$ Type Other names from NED
                and number of reference
  (1) (2) (3) (4) (5) (6) (7) (8)
83 HS 1236+4532 12 36 39.8 +45 32 54 16334:$\pm$ 300 17.6 -19.1 NON MAPS-NGPO 172 027192
84 HS 1237+3900 12 37 04.0 +39 00 00 11198 $\pm$ 11 +18.6 -17.3 BCG 6
85 HS 1238+4229 12 38 24.1 +42 29 08 11370 $\pm$ 53 18.9 -17.0 BCG  
86 HS 1242+4058A 12 42 00.3 +40 58 12 5512 $\pm$ 197 16.6 -17.7 BCG MAPS-NGPO 218 061180
87 HS 1244+3647 12 44 36.9 +36 47 45 14171 $\pm$ 89 16.4 -20.0 BCG 2, 7
88 HS 1245+4413 12 45 52.8 +44 13 25 9293 $\pm$ 62 17.7 -17.8 DANS  
89 HS 1300+4225 13 00 36.5 +42 25 39 11374 $\pm$ 23 +17.3 -18.6 BCG?  
90 HS 1302+4058 13 02 13.6 +40 58 51 9200 $\pm$ 34 +16.8 -18.6 BCG MAPS-NGPO 219 053488
91 HS 1302+4101 13 02 49.8 +41 01 22 10567 $\pm$ 20 +18.5 -17.2 BCG  
92 HS 1305+4049 13 05 49.2 +40 49 09 10456 $\pm$ 57 +17.8 -17.9 BCG  
93 HS 1306+4146 13 06 13.5 +41 46 23 17237 $\pm$ 5 +19.1 -17.7 BCG  
94 HS 1306+4151 13 06 46.9 +41 51 04 82269 $\pm$ 23 +18.0 -22.2 NON  
95 HS 1306+4232 13 06 57.7 +42 32 19 14701 $\pm$ 90 +16.9 -19.6 DANS MAPS-NGPO 219 019849
96 HS 1307+4225 13 07 38.8 +42 25 04 2677 $\pm$ 20 +17.4 -15.3 BCG MAPS-NGPO 219 022840
97 HS 1309+4446 13 09 20.6 +44 46 42 8944 $\pm$ 158 +16.4 -19.0 DANS  
98 HS 1310+4224 13 10 20.8 +42 24 08 12565 $\pm$ 117 +17.7 -18.4 DANS  
99 HS 1311+3628 13 11 00.0 +36 28 02 1094 $\pm$ 12 18.0 -12.9 BCG Near UGC 8303, 2, 7
                NGP9 F269-0669419 is 14 to E
100 HS 1311+4507 13 11 30.2 +45 07 33 18285 $\pm$ 11 +18.6 -18.4 BCG  
101 HS 1311+4204 13 11 50.0 +42 04 50 10495 $\pm$ 14 +18.1 -17.6 DANS  
102 HS 1311+3924 13 11 54.2 +39 24 47 1401 $\pm$ 54 15.6 -15.8 BCG UGC 8315, 4
103 HS 1313+4440 13 13 04.4 +44 40 15 10982 $\pm$ 144 16.5 -19.3 SBN UGC 8327,MRK 248, 9
104 HS 1313+4246 13 13 25.5 +42 46 04 12055 $\pm$ 11 +19.2 -16.9 BCG MAPS-NGPO 219 017637
105 HS 1313+4041 13 13 34.2 +40 41 07 6373 $\pm$ 23 +17.6 -17.1 BCG  
106 HS 1313+4521 13 13 40.2 +45 21 59 3449 $\pm$ 18 +18.9 -14.4 BCG  
107 HS 1314+4145 13 14 00.0 +41 45 28 6445 $\pm$ 127 15.4 -19.3 SBN MRK 1477, 10
108 HS 1315+4129 13 15 42.5 +41 29 14 35297 $\pm$ 116 +18.0 -20.3 NON FIRSTJ131755.8+41132,
                7C1315+4129
109 HS 1316+3839 13 16 01.7 +38 39 22 18065 $\pm$ 86 16.4 -20.5 BCG?  
110 HS 1317+4521B 13 17 50.9 +45 21 60 32888 $\pm$ 133 +16.3 -21.9 Sy1  
111 HS 1322+3708 13 22 17.0 +37 08 39 14127 $\pm$ 67 16.4 -20.0 BCG KUG1322+371
112 HS 1323+3946 13 23 29.9 +39 46 13 7064 $\pm$ 162 16.0 -18.9 DANS IRAS F13235+3945
113 HS 1330+3651 13 30 54.0 +36 51 55 5044 $\pm$ 117 16.7 -17.4 BCG 2, 7
114 HS 1334+3957 13 34 11.4 +39 57 31 2513 $\pm$ 61 16.9 -15.7 BCG 2, 7
115 HS 1336+3650 13 36 43.9 +36 50 57 5791 $\pm$ 94 17.8 -16.6 BCG 2, 7
116 HS 1354+3635 13 54 29.9 +36 35 39 5056 $\pm$ 56 16.1 -18.0 BCG CG 1201, 3, 2, 7
117 HS 1402+3650 14 02 39.2 +36 50 47 10456 $\pm$ 83 16.3 -19.4 BCG 2, 7
118 HS 1408+4227 14 08 07.5 +42 27 26 20355 $\pm$ 17 20.6 -16.6 BCG  
119 HS 1408+4522 14 08 09.3 +45 22 23 20443 $\pm$ 113 17.8 -19.4 BCG CG 367
120 HS 1410+3627 14 10 02.2 +36 27 15 9890 $\pm$ 90 16.9 -18.7 BCG 2, 7
121 HS 1412+4203 14 12 12.3 +42 03 50 24842 $\pm$ 160 19.1 -18.5 SBN  
122 HS 1414+4034 14 14 43.1 +40 34 58 6097 $\pm$ 32 20.1 -14.5 BCG  
123 HS 1417+4433 14 17 27.9 +44 33 14 18797 $\pm$ 5 19.8 -17.2 BCG  



Table 3. (Continued)

# Name $\alpha\,(1950)$ $\delta\,(1950)$ $V_{hel}^{\,a}\pm\sigma_V$ mB M $_{B}^{\;\;b}$ Type Other names from NED
                and number of reference
  (1) (2) (3) (4) (5) (6) (7) (8)
124 HS 1419+3639 14 19 16.2 +36 39 18 3579 $\pm$ 42 17.1 -16.3 BCG UGC 9198, 2
125 HS 1420+3726 14 20 50.1 +37 26 58 10847 $\pm$ 45 17.5 -18.3 BCG  
126 HS 1423+3945 14 23 13.6 +39 45 27 1480 $\pm$ 35 18.5 -13.0 SA in Sp in UGC 9242
127 HS 1423+4054 14 23 50.0 +40 54 48 8059 $\pm$ 93 18.5 -16.7 BCG  
128 HS 1427+4309 14 27 53.4 +43 09 40 2679 $\pm$ 151 17.8 -15.0 BCG CG 449,PGC051797,
                [KOS87]142752+430936, 12
129 HS 1428+4056 14 28 15.9 +40 56 16 10276 $\pm$ 49 19.9 -15.8 DANS  
130 HS 1430+4040 14 30 17.9 +40 40 54 6999 $\pm$ 60 17.2 -17.7 DANS CG 467,IRAS F14302+4041,
                PGC051943, 13
131 HS 1433+4411 14 33 27.2 +44 11 21 2945 $\pm$ 90 16.8 -16.2 BCG CG 480,NPM1G+44.0284
132 HS 1433+4245 14 33 53.6 +42 45 23 21481 $\pm$ 300 14.0 -23.3 LINER NPM1G+42.0387
133 HS 1437+4002 14 37 58.5 +40 02 29 11084 $\pm$ 29 +19.2 -16.7 BCG 6
134 HS 1441+4122 14 41 24.4 +41 22 44 11007 $\pm$ 122 17.3 -18.5 DANS NPM1G+41.0365
135 HS 1443+4027 14 43 11.0 +40 27 39 8425 $\pm$ 30 17.1 -18.2 BCG CG 527
136 HS 1447+4402 14 47 20.1 +44 02 50 24642 $\pm$ 56 19.2 -18.4 DANS  
137 HS 1448+4518 14 48 56.3 +45 18 01 10661 $\pm$ 149 17.8 -18.0 DANS?  
138 HS 1450+3844 14 50 20.8 +38 44 37 4179 $\pm$ 54 17.8 -15.9 BCG CG 565,[SP82]25, 2
139 HS 1450+4234 14 50 55.3 +42 34 20 10393 $\pm$ 194 17.4 -18.3 DANS CG 568,NPM1G+42.0398
140 HS 1458+4129 14 58 03.9 +41 29 17 8687 $\pm$ 116 18.4 -16.9 DANS  
141 HS 1514+4602 15 14 27.6 +46 02 48 22810 $\pm$ 300 16.8 -20.7 SBN NPM1G+46.0322, 1
142 HS 1537+4411 15 37 19.2 +44 11 23 9312 $\pm$ 43 17.2 -18.3 BCG  
143 HS 1545+4055 15 45 26.2 +40 55 36 9521 $\pm$ 14 18.8 -16.7 BCG [SP82]54
144 HS 1545+4459 15 45 34.0 +44 59 19 10480 $\pm$ 114 18.4 -17.3 BCG?  
145 HS 1546+4319 15 46 31.9 +43 19 50 12400 $\pm$ 45 16.5 -19.6 SBN IRAS F15465+4320
146 HS 1603+3759$^\ddagger$ 16 03 13.2 +37 59 08 12071 $\pm$ 82 18.6 -17.4 BCG  
147 HS 1613+3902 16 13 51.4 +39 02 28 10046 $\pm$ 77 18.7 -16.9 BCG FIRSTJ161538.5+38544
148 HS 1616+3627 16 16 19.9 +36 27 11 10210 $\pm$ 38 16.5 -19.2 Sy1 RXJ1618.1+3619, 11
149 HS 1625+3847 16 25 49.1 +38 47 28 9355 $\pm$ 131 18.4 -17.1 BCG?  
150 HS 1633+4703 16 33 12.8 +47 03 44 2681 $\pm$ 62 16.7 -16.1 BCG 2, 7
151 HS 1645+4339 16 45 57.7 +43 39 27 9577 $\pm$ 118 18.3 -17.2 BCG  
152 HS 1646+4003B 16 46 35.6 +40 03 59 9877 $\pm$ 83 19.7 -15.9 BCG?  
153 HS 1649+3621 16 49 35.6 +36 21 13 9189 $\pm$ 162 18.1 -17.3 BCG  
154 HS 1650+3706 16 50 22.4 +37 06 22 6898 $\pm$ 30 19.1 -15.7 BCG  
155 HS 1653+4340 16 53 19.4 +43 40 29 59773 $\pm$ 116 +18.7 -20.9 SBN?  
156 HS 1655+3845 16 55 47.9 +38 45 56 2221 $\pm$ 112 17.1 -15.3 BCG  
157 HS 1704+3542$^\ddagger$ 17 04 51.5 +35 42 15 7602 $\pm$ 162 18.0 -17.0 BCG  
158 HS 1710+3746 17 10 19.8 +37 46 26 11196 $\pm$ 104 17.8 -18.1 BCG  
159 HS 1713+4417 17 13 12.3 +44 17 03 8425 $\pm$ 80 18.4 -16.9 BCG?  
160 HS 1713+4856 17 13 25.3 +48 56 53 8051 $\pm$ 44 19.3 -15.9 BCG  
161 HS 1716+3817 17 16 34.1 +38 17 31 13062 $\pm$ 178 16.9 -19.3 SBN? 6
                 
a Heliocentric velocities.; b absolute magnitudes are not corrected for galactic extinction;
+ APM magnitudes; objects from the second priority random sample; $^\ddagger$ galaxies from the APM selected sample.



Table 3. (Continued)
References:
1 - Klemola, A. R., Jones, B. F., & Hanson, R. B. 1987, AJ, 94, 501
2 - Popescu, C. C., Hopp, U., Hagen, H.-J., & Elsässer, H. 1996, A&AS, 116, 43
3 - Ugryumov, A. V., Pustilnik, S. A., Lipovetsky, V. A., Izotov, Yu. I., & Richter, G. M. 1998, A&AS, 131, 295
4 - RC3
5 - Weistrop, D., & Downes, R. A. 1991, AJ, 102, 1680
6 - Hopp, U., Engels, D., Green, R., et al. 2000, A&AS, 142, 417 ( Paper III)
7 - Popescu, C. C., & Hopp, U. 2000, A&AS, 142, 247
8 - Falco, E. E., Kurtz, M. J., Geller, M. J., et al. 1999, PASP, 111, 438
9 - Markarian, B. E., Lipovetsky, V. A., Stepanian, et al. 1989, Soob. SAO. No.62, 5
10 - Fisher, K. B., Huchra, J. P., Strauss, M. A., et al. 1995, ApJS, 100, 69
11 - Grupe, D., Beuermann, K., Mannheim, K., & Thomas H.-C. 1999, A&A, 350, 895
12 - Kirshner, R. P., Oemler, A., Schechter, P. L., & Shectman, S. A. 1987, ApJ, 314, 493
13 - Tifft, W. C., Kirshner, R. P., Gregory, S. A., & Moody, J. W. 1986, ApJ, 310, 75
14 - Wegner, G., & Boley, F. I. 1993, AJ, 105, 660


 
Table 4: Emission line parameters
# Name F(H$\beta$)a W (Å) W(Å) W (Å)
  (1) (2) (3) (4) (5) (6) (7) (8) (9) (10)
1 HS 0809+4334 51 1.16 3.96 3.71 0.16 0.20 41 24 92
2 HS 0818+4234 +5:         0.75:   +12: 5:
3 HS 0822+4049 85 1.45 2.25 4.62 0.14 0.20 72 38 86
4 HS 0822+4238 16 2.81 3.94 4.63 0.08 0.16 39 14 55
5 HS 0824+4139 11   3.55 4.64 0.08 0.41   8 31
6 HS 0828+4305 43 1.63 1.60 5.77 0.26 0.32 16 9 15
7 HS 0828+4346 23   6.22 4.39 0.02 0.10   16 103
8 HS 0831+4208 8:   2.50 13.12 0.38 0.30   4: 11
9 HS 0849+3802$^\ddagger$ 36   2.50 7.25 0.34 0.35   7 17
10 HS 0849+3639$^\ddagger$ 20   2.10 4.45 0.08 0.26   11 22
11 HS 0850+3722$^\ddagger$ +5:             +10: 10:
12 HS 0855+4118 64   2.59 3.88 0.12 0.25   17 45
13 HS 0855+3729$^\ddagger$ 28 1.93 0.75 4.00 0.29 0.30 24 14 11
14 HS 0900+4318 18   6.06 4.50   0.06:   19 120
15 HS 0901+3517$^\ddagger$ 2:   11: 16:   0.25:   2: 19
16 HS 0904+3752$^\ddagger$ +13         0.08:   +26 8:
17 HS 0907+4201 4:   1.75: 9.50: 0.29 0.32   4: 7:
18 HS 0912+4427 +10       0.20 0.20:   +35 18:
19 HS 0912+4259 37 5.46 1.70 6.03 0.21 0.30 68 15 26
20 HS 0912+4433* 16   4.91 7.50 0.17 0.02:   11 53
21 HS 0912+3900$^\ddagger$ +40       0.35 0.28   +31 2:
22 HS 0923+4021* 16   5.94 4.44 0.04 0.20   15 78
23 HS 0927+4159 30   3.13 4.23 0.09 0.29   22 75
24 HS 0934+4150 32   4.75 4.78 0.06 0.17   24 113
25 HS 0934+4256 16:   5.31: 9.25: 0.24 0.71   2: 11
26 HS 0935+4135 7: 1: 0.71: 2.86: 0.60 0.15 10: 10: 8:
27 HS 0938+4215 27   3.39 3.54 0.05 0.28   20 69
28 HS 0939+4124 61 1.43 7.89 4.39 0.01 0.04 175 171 1367
29 HS 0940+4052 133 3.65 4.48 3.73 0.05 0.17 91 41 196
30 HS 0941+4024A 12   3.11 8.09 0.40 0.40   4 13
31 HS 0941+4024B 51   2.37 4.96 0.18 0.24   17 41
32 HS 0947+3526$^\ddagger$ 24   4.29 2.92   0.20   28 118
33 HS 0948+3723* 20 1.50 5.30 2.78: 0.05:   375 32 187
34 HS 0951+3712$^\ddagger$ 6: 4.83: 2.17: 12.50: 0.32 0.36 10: 2: 5:
35 HS 0952+4024$^\ddagger$ 18   1.28 4.22 0.17 0.32   9 11
36 HS 0953+3628 77 2.53 3.83 2.64 0.10 0.19 92 42 177
37 HS 0954+3615$^\ddagger$ 6:   6.17: 6.33: 0.08 0.50:   2: 18
38 HS 0956+3702$^\ddagger$ 14 9.14 2.14 7.36 0.28 0.32 39 5 11
39 HS 0958+3654$^\ddagger$ +95       0.53 0.44   +16  
40 HS 0958+3637* 4:   5.05: 9.77:   0.40   3: 14
                     



Table 4. (Continued)
# Name F(H$\beta$)a W (Å) W(Å) W (Å)
  (1) (2) (3) (4) (5) (6) (7) (8) (9) (10)
41 HS 0958+3718* 190 0.24 6.46 2.25 0.03   21 64 430
42 HS 1004+3730$^\ddagger$ +81       0.42 0.40   +38 3
43 HS 1008+3620$^\ddagger$ 13   6.15 6.31 0.07 0.22   10 64
44 HS 1011+3604 26 1.81 2.08 3.85 0.16 0.29 97 15 33
45 HS 1014+3535$^\ddagger$ 5:     16: 0.37 0.25   2:  
46 HS 1016+3733* 27 3.39 4.61 5.35 0.68 0.56 23 5 22
47 HS 1021+4839 +53       0.33 0.12:   +33 6:
48 HS 1025+3707A 37   3.78 2.92 0.07 0.12   25 99
49 HS 1025+3707B +42       0.43:     +62  
50 HS 1025+3658$^\ddagger$ 24   6.08 4.75 0.11 0.18   17 106
51 HS 1025+4057* 16:     2.19: 0.29 0.49:   19:  
52 HS 1027+4728 +24       0.42: 0.21:   +11  
53 HS 1028+3716* 32 1.00 2.88 5.63 0.20 0.30 60 13 35
54 HS 1032+4600* 45   2.88 5.81 0.15 0.32   11 34
55 HS 1043+3852$^\ddagger$ 5:   7.60: 5.60:   0.11:   6: 54
56 HS 1122+3800$^\ddagger$ 2:   9.50: 11.00: 0.05: 0.09:   6: 57
57 HS 1148+3732* 37 2.54 2.16 2.59 0.21 0.35 50 21 47
58 HS 1159+3940 14 4.07 1.79 2.71 0.21 0.18: 61 21 40
59 HS 1200+3824 +12       0.25:     +16  
60 HS 1201+3535 14 2.86 5.79 3.14 0.02: 0.20: 50 28 180
61 HS 1202+3732 27 4.66 4.60 3.50 0.04:   43 12 54
62 HS 1204+3945* 6:   4.45: 9.06: 0.10 0.24   5: 23
63 HS 1205+3940 33 1.67 5.55 3.36 0.05 0.09 81 36 237
64 HS 1206+4012 +9:             +10:  
65 HS 1210+3831* 39 4.64 2.51 3.51 0.14 0.36 59 12 32
66 HS 1211+3807* 40   2.75 5.63 0.12 0.18   8 22
67 HS 1211+4012 12 5.33 6.67 3.75 0.04: 0.13: 60 11 79
68 HS 1212+3640* 70 3.43 2.54 6.27 0.08 0.25 79 14 36
69 HS 1213+3636A 237 0.41 3.48 2.55 0.05 0.08 66 281 1094
70 HS 1213+3636B 31   3.43 3.96 0.04: 0.18   35 145
71 HS 1215+3850* 97 3.05 3.34 4.54 0.07 0.22 52 16 53
72 HS 1216+3743* +39         0.23   +65 31
73 HS 1218+3945* 28 3.46 3.79 2.29 0.14 0.19 173 28 106
74 HS 1220+3845 19 1.27 1.43 2.85 0.62 0.21 13 13 19
75 HS 1223+3938* 48   6.25 4.46 0.07 0.15   17 109
76 HS 1224+4027 22 3.82 3.50 3.50 0.09 0.19 50 17 60
77 HS 1225+4129 17 2.47 3.06 3.82 0.14 0.38 32 14 44
78 HS 1226+4113 21 2.19 5.10 5.19 0.05: 0.12: 65 12 60
79 HS 1232+3834* 16 3.19 8.06 4.63 0.09: 0.34: 130 7 62
80 HS 1232+3947* 87   3.54 2.90   0.15   36 136
81 HS 1235+4232* 7:   2.14: 1.86: 0.15: 0.38:   24: 55:
82 HS 1236+3821* 55 5.82 5.25 5.47 0.02 0.19 124 7 41
                     


Table 4. (Continued)
# Name F(H$\beta$)a W (Å) W(Å) W (Å)
  (1) (2) (3) (4) (5) (6) (7) (8) (9) (10)
83 HS 1236+4532 +3:             +3:  
84 HS 1237+3900 40 2.33 5.35 2.90 0.07: 0.11: 79 39 227
85 HS 1238+4229 15 5.07 4.93 4.53 0.09 0.25: 86 18 91
86 HS 1242+4058A* 47   2.94 4.09 0.08 0.27   18 53
87 HS 1244+3647* 110 0.89 4.01 2.55 0.03 0.32 22 37 150
88 HS 1245+4413 32   2.16 2.06 0.18 0.26   24 57
89 HS 1300+4225 15: 2.20: 2.20: 2.33:     57 28: 64
90 HS 1302+4058 32 6.44 3.75 1.88   0.22 137 29 117
91 HS 1302+4101 22 2.09 3.59 3.45 0.09 0.20 55 25 98
92 HS 1305+4049 32 2.11 3.35 2.20 0.10 0.16 36 21 77
93 HS 1306+4146 64 1.55 5.98 2.56 0.02: 0.09: 237 146 889
94 HS 1306+4151 7: 2.71: 1.00:       17: 6: 6:
95 HS 1306+4232* 18   2.39 2.78   0.50   13 31
96 HS 1307+4225 26 0.83 5.52 3.86   0.10: 18 31 164
97 HS 1309+4446 19   2.00 3.11   0.32   9 19
98 HS 1310+4224 14 5.79 2.07 3.07   0.30 219 9 21
99 HS 1311+3628 448 1.29 5.18 2.92 0.05 0.09 299 393 2100
100 HS 1311+4507 52 2.58 4.33 2.75 0.08 0.15 116 76 335
101 HS 1311+4204 18 4.22 2.44 3.00 0.19 0.26 66 16 40
102 HS 1311+3924 179 1.89 4.38 2.30 0.04 0.13 97 61 290
103 HS 1313+4440 140   2.05 4.97 0.49 0.63   12 25
104 HS 1313+4246 30 1.93 4.80 3.57 0.05: 0.13: 57 36 180
105 HS 1313+4041* 28 2.82 5.07 3.50 0.05: 0.13: 44 19 102
106 HS 1313+4521 117 1.19 3.84 3.11 0.03: 0.12 92 77 306
107 HS 1314+4145 214   0.82 4.07 0.34 0.16   44 38
108 HS 1315+4129 +25       0.32: 0.40: 15: +16  
109 HS 1316+3839* 48 3.13 3.17 3.29 0.13 0.29 83 25 78
110 HS 1317+4521B* 48   0.48 1.89 0.14: 0.05:   24 12
111 HS 1322+3708 20 2.60 4.35 2.85 0.16 0.19 86 35 155
112 HS 1323+3946* 103 1.80 2.32 3.79 0.31 0.15 53 15 35
113 HS 1330+3651* 188 1.92 5.02 2.71 0.01 0.13 504 84 456
114 HS 1334+3957* 60 1.28 5.22 3.12 0.02 0.10 99 96 548
115 HS 1336+3650 36   3.80 4.76 0.07 0.34   14 54
116 HS 1354+3635* 154 3.01 3.36 4.22 0.06 0.22 159 23 77
117 HS 1402+3650 107 1.38 3.03 3.27 0.12 0.21 61 27 86
118 HS 1408+4227 120 0.82 7.58 2.78 0.02: 0.04: 99 219 1615
119 HS 1408+4522* 125   2.97 2.96 0.12 0.24   35 110
120 HS 1410+3627* 13:   3.46: 4.46: 0.05: 0.26   13: 41
121 HS 1412+4203* +16       0.44 0.25 13: +19  
122 HS 1414+4034 8: 4: 5.13: 3.25: 0.08: 0.15: 41 12: 69
123 HS 1417+4433 44 2.18 5.73 3.07 0.02: 0.12: 167 61 364
                     


Table 4. (Continued)
# Name F(H$\beta$)a W (Å) W(Å) W (Å)
  (1) (2) (3) (4) (5) (6) (7) (8) (9) (10)
124 HS 1419+3639 69 3.74 2.43 1.96 0.13 0.31 186 41 102
125 HS 1420+3726 34 2.53 3.21 2.56   0.34 69 35 120
126 HS 1423+3945 70   4.56 2.24 0.03 0.11   136 638
127 HS 1423+4054 25 4.12 2.72 1.96 0.08 0.20 64 18 54
128 HS 1427+4309* 34 2.24 4.09 2.91 0.08 0.26 54 23 99
129 HS 1428+4056 +13       0.08: 0.15:   +21 7:
130 HS 1430+4040 121 2.94 0.79 2.78: 0.13: 0.05: 281 51 45
131 HS 1433+4411 45   3.27 3.58 0.06 0.24   10 34
132 HS 1433+4245* +97       1.20   17: +41  
133 HS 1437+4002 30 1.47 6.13 3.53 0.03: 0.11: 114 60 340
134 HS 1441+4122* 22 5.16 2.85 5.09 0.15 0.26 47 11 32
135 HS 1443+4027 61 1.87 2.97 3.26 0.15 0.19 163 19 56
136 HS 1447+4402 8: 3.75: 1.50: 5.50: 0.25: 0.30: 22: 5: 8:
137 HS 1448+4518* +53       0.15 0.31 19 +44 8:
138 HS 1450+3844* 72 2.31 3.46 3.53 0.07 0.21 132 23 82
139 HS 1450+4234 29   0.72 2.93 0.27 0.40   13 10
140 HS 1458+4129 +28       0.17 0.40   +29  
141 HS 1514+4602* +62       0.46 0.19:   +61  
142 HS 1537+4411* 19   3.91 3.30 0.03 0.23   12 50
143 HS 1545+4055 161 1.27 5.66 2.70 0.02: 0.05: 181 163 983
144 HS 1545+4459 12 7.92 3.75 5.33 0.13 0.28 76 7 29
145 HS 1546+4319* 41 3.80 1.81 4.23 0.33 0.24 25 7 14
146 HS 1603+3759$^\ddagger$ 19 2.16 4.89 2.42     104 43 228
147 HS 1613+3902 19   4.37 2.84   0.13   12 52
148 HS 1616+3627 120   0.63 3.57 0.16     11 8
149 HS 1625+3847 7:   3.00: 4.57:   0.25   8: 25
150 HS 1633+4703* 170 3.96 3.29 3.38 0.07 0.23 76 16 55
151 HS 1645+4339 23   4.43 4.83 0.06 0.22   11 51
152 HS 1646+4003B 21:   1.62: 3.33: 0.14     13: 19:
153 HS 1649+3621 21: 1.86: 3.57: 3.43:     37: 13: 48
154 HS 1650+3706 66 2.36 5.55 2.39 0.08 0.09 275 124 647
155 HS 1653+4340 6: 3.83: 3.17: 6.00: 0.44: 0.44: 21: 4: 13:
156 HS 1655+3845* 49 2.31 4.14 2.76   0.19 60 30 125
157 HS 1704+3542$^\ddagger$ 4: 12.54: 8.16: 6.16:   0.22: 60 5: 46
158 HS 1710+3746* 19 2.84 3.11 3.74 0.07 0.23 110 24 68
159 HS 1713+4417 15 4.27 3.07 5.93 0.22 0.25 24 5 16
160 HS 1713+4856 140 1.04 5.91 3.08 0.04 0.05 147 101 632
161 HS 1716+3817 9:   1.67: 10.11: 0.13 0.32   3: 5:
                     
a Flux in 10-16 ergs s-1 cm-2; * objects observed during non-photometric conditions;  
objects from the second priority random sample; $^\ddagger$ galaxies from the APM selected sample;  
+ parameters for H$\alpha$ emission line; : parameters with less confident values.  


 
Table 5: Coordinates, Redshifts and Magnitudes of QSOs
# Name $\alpha\,(1950)$ $\delta\,(1950)$ mB Detected emission lines
  (1) (2) (3) (4) (5) (6)
1 HS 0936+4204 09 36 59.6 +42 04 24 3.3211 18.3 Ly$\alpha$ 1216 Å, Si IV/O IV] 1400 Å, C IV 1549 Å
2 HS 1009+3706 10 09 02.4 +37 06 31 3.0393 17.6 Ly$\alpha$ 1216 Å, Si IV/O IV] 1400 Å, C IV 1549 Å
3 HS 1224+4410 12 24 55.1 +44 10 03 3.0718 19.5 Ly$\alpha$ 1216 Å, C IV 1549 Å
4 HS 1301+4233 13 01 47.0 +42 33 30 0.8460: +18.7 Mg II 2798 Å
5 HS 1541+4452 15 41 23.0 +44 52 27 2.3588 18.8 Ly$\alpha$ 1216 Å, Si IV/O IV] 1400 Å, C IV 1549 Å
             
a Observed redshift; + APM magnitudes; : less confident values.



 
Table 6: Galaxies without detected emission lines
# Name $\alpha\,(1950)$ $\delta\,(1950)$ mB M Absorption lines
  (1) (2) (3) (4) (5) (6) (7)
1 HS 1008+3538 10 08 00.1 +35 38 02 13968: 17.4 -19.0 H$\beta$, MgIb, H$\alpha$
2 HS 1207+3745 12 07 38.0 +37 45 53 13381: 18.8 -17.5 H$\beta$, H$\alpha$
3 HS 1408+3524 14 08 32.6 +35 24 23 19933 16.8 -20.3 CaK, CaH, Gband, H$\beta$, MgIb, CaFe5269, NaD
4 HS 1419+4026 14 19 50.0 +40 26 28 14235: 18.1 -18.3 Gband, H$\alpha$
               
a Heliocentric velocities; b absolute magnitudes are not corrected for galactic extinction;
objects from the second priority random sample; : less confident values.

             



 
Table 7: Stars
# Name $\alpha\,(1950)$ $\delta\,(1950)$ mB Type Spectral features
  (1) (2) (3) (4) (5) (6)
1 HS 0852+4257 08 52 23.3 +42 57 22 +20.2 A H, H, H
2 HS 0945+4851 09 45 00.5 +48 51 00 +18.0 F-G H, MgIb, CaFe5269, H
3 HS 1012+3815 10 12 45.4 +38 15 01 17.2 A H, H, H
4 HS 1013+3804 10 13 05.6 +38 04 27 17.7 F H, NaD, H
5 HS 1029+4020 10 29 10.6 +40 20 35 16.7 G MgIb, CaFe5269, NaD, H
6 HS 1158+3920 11 58 04.6 +39 20 32 +18.2 A-F H, H, MgIb, NaD, H
7 HS 1411+4312 14 11 12.8 +43 12 53 19.6 G Gband, MgIb, NaD, H
8 HS 1424+4029 14 24 57.9 +40 29 28 19.8 F Gband, H, MgIb, NaD, H
9 HS 1609+4941 16 09 46.6 +49 41 45 19.1 G Gband, MgIb, CaFe5269, H
10 HS 1630+3620 16 30 33.0 +36 20 17 19.1 G Gband, MgIb, CaFe5269, NaD, H
11 HS 1640+4158 16 40 18.0 +41 58 42 18.3 G Gband, MgIb, NaD
12 HS 1652+3820 16 52 47.9 +38 20 16 17.7 G Gband, MgIb, CaFe5269, NaD, H
13 HS 1653+4430 16 53 49.9 +44 30 10 19.7 F CaK, CaH, Gband, H, MgIb, NaD, H
14 HS 1656+4309 16 56 02.7 +43 09 01 19.2 A H, H, H
15 HS 1657+4419 16 57 28.6 +44 19 26 20.0 F CaK, CaH, H, H, H
16 HS 1710+4343 17 10 04.2 +43 43 47 +18.2 F H, MgIb, H
17 HS 1711+3804 17 11 31.4 +38 04 32 +19.1 F H, MgIb, NaD, H
18 HS 1716+3544 17 16 14.0 +35 44 07 18.9 F Gband, H, H, MgIb, CaFe5269, H
19 HS 1720+3927 17 20 13.6 +39 27 11 18.1 F-G Gband, H, MgIb, NaD, H
20 HS 1733+3749 17 33 41.9 +37 49 13 18.4 G Gband, H, MgIb, NaD, H
21 HS 1733+3915$^\ddagger$ 17 33 45.8 +39 15 08 18.1 F-G H, MgIb, NaD, H
             
objects from the second priority random sample; $^\ddagger$ galaxies from the APM selected sample;
+ APM magnitudes.


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2001-06-08