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Table 2: Coordinates, Velocities and Magnitudes of Emission-Line Galaxies

#	Name	$\alpha\,(1950)$	$\delta\,(1950)$	$v_{0}^{\,a}$	m$_{\rm B}$	M $_{\rm B}^{\;\;b}$	Type	Other Names from NED
	(1)	(2)	(3)	(4)	(5)	(6)	(7)	(8)
1	HS 0940+3737*	09h40m10.7s	37$^{\circ}$37'14''	15655 $\pm$107	16.1	-20.5	Sy	IRAS F09401+3737
2	HS 0948+3723	09 48 19.0	37 23 05	4806 $\pm$ 30	+17.8	-16.2	NON
3	HS 0954+3612	09 54 01.1	36 12 12	13602 $\pm$ 24	17.3	-19.0	BCG?
4	HS 0956+3847	09 56 51.0	38 47 54	15785 $\pm$ 21	16.7	-19.9	BCG
5	HS 1012+3655	10 12 49.0	36 55 31	10097 $\pm$ 12	18.3	-17.4	BCG
6	HS 1015+3737*	10 15 23.3	37 37 44	14533 $\pm$ 66	16.4	-20.0	Sy	IRAS F10154+3737 ?
7	HS 1018+3619*	10 18 11.8	36 19 16	22244 $\pm$ 65	17.3	-20.0	BCG
8	HS 1024+3648*	10 24 56.4	36 48 54	11184 $\pm$ 68	16.6	-19.3	Sy	FIRST J102749.9+363334
9	HS 1053+3722*	10 53 43.0	37 22 55	13011 $\pm$ 61	16.7	-19.5	SBN?
10	HS 1058+3553	10 58 12.5	35 53 15	9366 $\pm$ 12	17.0	-18.5	BCG
11	HS 1103+3627*	11 03 15.9	36 27 30	13832 $\pm$ 67	15.5	-20.8	BCG	CG 810, IRAS
12	HS 1103+3758*	11 03 03.4	37 58 24	13664 $\pm$ 60	18.1	-18.2	SBN
13	HS 1106+3621	11 06 35.6	36 21 52	6526 $\pm$ 60	18.4	-16.3	BCG
14	HS 1107+3524	11 07 53.1	35 24 36	8362 $\pm$ 48	17.4	-17.8	BCG
15	HS 1107+3637	11 07 04.0	36 37 16	8206 $\pm$ 18	19.5	-15.7	NON
16	HS 1107+3710*	11 07 31.5	37 10 49	8750 $\pm$ 84	17.0	-18.3	SBN
17	HS 1107+3712	11 07 17.7	37 12 21	9639 $\pm$ 13	17.6	-17.9	BCG?
18	HS 1133+3852	11 33 50.2	38 52 37	6631 $\pm$ 27	+19.8	-14.9	BCG?
19	HS 1134+3805*	11 34 28.0	38 05 10	9578 $\pm$ 70	+18.6	-16.9	BCG
20	HS 1139+3712*	11 39 01.3	37 12 19	6523 $\pm$ 60	17.0	-17.7	BCG
21	HS 1148+3827*	11 48 00.3	38 27 00	10334 $\pm$ 65	18.7	-17.0	BCG
22	HS 1158+3837	11 58 21.5	38 37 41	6898 $\pm$ 15	17.9	-16.9	BCG	CG 1493
23	HS 1159+3940	11 59 52.5	39 40 59	6350 $\pm$ 41	+17.4	-17.2	NON
24	HS 1207+3957	12 07 14.2	39 57 57	11700 $\pm$ 30	18.5	-17.5	BCG
25	HS 1209+3726	12 09 20.2	37 26 57	7273 $\pm$ 54	16.9	-18.0	BCG?
26	HS 1210+3759*	12 10 13.4	37 59 40	6875 $\pm$ 84	+17.2	-17.6	DANS?
27	HS 1214+3922	12 14 30.6	39 22 22	4438 $\pm$ 12	18.2	-15.5	BCG
28	HS 1214+3801*	12 14 39.6	38 01 32	276 $\pm$ 67	+16.5	-11.3	SA in SpG	part of NGC 4244
29	HS 1237+3900	12 37 04.0	39 00 00	11199 $\pm$ 21	+18.6	-17.3	BCG
30	HS 1248+3523	12 48 53.0	35 23 06	10025 $\pm$ 15	17.4	-18.2	BCG
31	HS 1249+4021*	12 49 25.1	40 21 04	9882 $\pm$ 67	17.0	-18.6	SBN?
32	HS 1254+3740	12 54 55.2	37 40 46	7635 $\pm$ 15	18.0	-17.0	BCG
33	HS 1257+3658*	12 57 45.0	36 58 05	8658 $\pm$ 84	17.1	-18.2	BCG	NGP9 F269-0458422
34	HS 1302+3607	13 02 49.9	36 07 49	9561 $\pm$ 27	17.1	-18.4	BCG	CG 1080
35	HS 1309+3701	13 09 50.6	37 01 54	7211 $\pm$ 30	18.1	-16.8	BCG	NGP9 F269-0480622
36	HS 1311+3641*	13 11 54.7	36 41 48	28685 $\pm$ 116	17.5	-20.4	SBN	NGP9 F269-0606354
37	HS 1323+3851*	13 23 43.1	38 51 25	6580 $\pm$ 61	17.5	-17.2	BCG
38	HS 1327+3731*	13 27 26.8	37 31 28	4187 $\pm$ 64	16.5	-17.2	BCG	NGP9 F270-0319016
39	HS 1331+3545*	13 31 59.8	35 45 05	17661 $\pm$ 93	18.1	-18.8	BCG
40	HS 1331+3657	13 31 46.5	36 57 21	18351 $\pm$ 15	18.0	-18.9	BCG
41	HS 1333+3717*	13 33 34.6	37 17 04	17008 $\pm$ 33	18.0	-18.8	BCG	HS 1333+3717
42	HS 1341+3700*	13 41 00.9	37 00 01	5882 $\pm$ 81	15.8	-18.7	SBN	CG 1181=IRAS
43	HS 1347+3811	13 47 02.3	38 11 35	2828 $\pm$ 32	18.8	-14.1	NON	HS 1347+3811

Table 2. (Continued)

#	Name	$\alpha\,(1950)$	$\delta\,(1950)$	$v_{0}^{\,a}$	m$_{\rm B}$	M $_{\rm B}^{\;\;b}$	Type	Other Names from NED
	(1)	(2)	(3)	(4)	(5)	(6)	(7)	(8)
44	HS 1402+3945	14h02m55.0s	39$^{\circ}$45'11''	19654 $\pm$ 18	16.6	-20.5	SBN
45	HS 1414+3605*	14 14 50.8	36 05 01	43503 $\pm$ 132	18.3	-20.5	Sy?
46	HS 1424+3836	14 24 25.9	38 36 26	6708 $\pm$ 15	+18.4	-16.4	BCG	CG 428=HS 1424+3836
47	HS 1425+3847*	14 25 33.8	38 47 17	6578 $\pm$ 63	16.0	-18.7	SBN?	CG 436
48	HS 1428+3545	14 28 23.3	35 45 24	11858 $\pm$ 27	+18.5	-17.5	BCG
49	HS 1434+3644*	14 34 20.1	36 44 26	9385 $\pm$ 88	+18.1	-17.4	BCG
50	HS 1437+4002	14 37 58.5	40 02 29	11068 $\pm$ 31	+19.2	-16.7	BCG?
51	HS 1447+3636*	14 47 48.0	36 36 03	1861 $\pm$ 67	17.7	-14.3	BCG
52	HS 1449+3647	14 49 02.3	36 47 24	10086 $\pm$ 15	+18.6	-17.1	BCG
53	HS 1457+3652	14 57 59.6	36 52 39	11768 $\pm$ 18	+19.8	-16.2	BCG
54	HS 1458+3726*	14 58 32.4	37 26 02	32205 $\pm$ 306	+20.7	-17.5	NON
55	HS 1513+3612*	15 13 04.1	36 12 05	18466 $\pm$ 67	+17.8	-19.2	BCG
56	HS 1519+4007*	15 19 30.0	40 07 39	2625 $\pm$ 60	+16.5	-16.2	BCG	CG 691
57	HS 1520+3717	15 20 30.6	37 17 56	11144 $\pm$ 78	+18.1	-17.8	NON
58	HS 1524+3536*	15 24 48.8	35 36 39	8770 $\pm$ 12	18.0	-17.3	BCG	CG 720
59	HS 1526+3729*	15 26 18.7	37 29 36	9792 $\pm$ 64	+16.5	-19.1	Sy?	IRAS F15263+3729
60	HS 1526+3634	15 26 27.2	36 34 29	18825 $\pm$ 20	+19.1	-17.9	BCG
61	HS 1527+3912	15 27 46.2	39 12 30	23004 $\pm$ 38	+15.7	-21.7	SBN	CG 734
62	HS 1529+4003*	15 29 45.1	40 03 21	8379 $\pm$ 60	+16.7	-18.5	BCG?	CG 749
63	HS 1530+3617	15 30 57.5	36 17 40	4666 $\pm$ 24	+17.0	-17.0	DANS?
64	HS 1535+3747*	15 35 40.6	37 47 47	7660 $\pm$ 63	+19.1	-16.0	BCG
65	HS 1536+3958	15 36 52.3	39 58 10	4367 $\pm$ 18	18.0	-15.8	BCG
66	HS 1543+3830	15 43 44.8	38 30 30	7862 $\pm$ 18	19.2	-15.9	BCG
67	HS 1557+3549*	15 57 35.8	35 49 45	12852 $\pm$ 97	16.8	-19.4	BCG?
68	HS 1558+3543	15 58 27.3	35 43 15	20377 $\pm$ 84	18.3	18.9	NON
69	HS 1558+3636*	15 58 34.1	36 36 34	12495 $\pm$ 62	17.8	-18.3	BCG
70	HS 1608+3654	16 08 31.5	36 54 42	9587 $\pm$ 18	17.3	-18.2	NON
71	HS 1613+3701	16 13 50.6	37 01 13	8844 $\pm$ 21	17.1	-18.3	BCG
72	HS 1615+3521*	16 15 48.4	35 21 07	8507 $\pm$ 70	17.5	-17.8	BCG
73	HS 1619+3557*	16 19 11.3	35 57 35	15092 $\pm$ 42	17.4	-19.1	BCG
74	HS 1624+3618	16 24 22.3	36 18 25	9484 $\pm$ 12	19.0	-16.5	BCG
75	HS 1638+3938	16 38 01.8	39 38 17	8969 $\pm$ 15	18.2	-17.2	BCG
76	HS 1643+4015	16 43 39.0	40 15 07	11617 $\pm$ 18	17.4	-18.6	BCG
77	HS 1645+3551*	16 45 51.9	35 51 57	6720 $\pm$ 61	17.7	-17.1	BCG
78	HS 1653+3634	16 53 07.2	36 34 55	845 $\pm$ 24	+16.0	-14.3	BCG
79	HS 1656+3927	16 56 34.7	39 27 58	10290 $\pm$ 42	17.7	-18.0	Sy?	FIRST J165815.4+392329
80	HS 1711+3756*	17 11 41.5	37 56 12	8273 $\pm$ 59	17.6	-17.6	BCG
81	HS 1721+3615	17 21 47.5	36 15 43	15596 $\pm$ 15	18.1	-18.5	BCG
a Heliocentric velocities.
b Absolute magnitudes are not corrected for the Galaxy extinction.
* Objects observed with the 2.2m Calar Alto telescope.
+ APM magnitude.

 

Table 3: Coordinates, Redshifts and Magnitudes of QSO

Name	$\alpha\,(1950)$	$\delta\,(1950)$	$z^{\,a}$	$m_{\rm B}$	Detected Emission Lines
(1)	(2)	(3)	(4)	(5)	(6)
HS 1003+3719	10h03m12.5s	37$^{\circ}$19 '51''	3.204	17.7	Ly$\alpha$ 1216 Å, Si IV/O IV] 1400 Å, C IV 1549 Å
HS 1024+3558	10 2421.7	35 5836	3.106	16.9	Ly$\alpha$ 1216 Å, Si IV/O IV] 1400 Å, C IV 1549 Å
HS 1152+3700	11 5250.0	37 0020	3.069	20.0	Ly$\alpha$ 1216 Å
HS 1649+3905	16 4902.6	39 0546	3.166	18.3	Ly$\alpha$ 1216 Å, C IV 1549 Å
a Observed redshift.
+ APM magnitude.

 

Table 4: Parameters of Emission Lines of Galaxies

#	Name	F(H$\beta$)a	$\frac{F(\lambda 3727)}{F(\rm H\beta)}$	$\frac{F(\lambda 5007)}{F(\rm H\beta)}$	$\frac{F(\rm H\alpha)}{F(\rm H\beta)}$	$\frac{F(\lambda 6583)}{F(\rm H\alpha)}$	$\frac{F([\rm SII])}{F(\rm H\alpha)}$	W $_{\lambda 3727}$(Å)	W $_{\rm H\beta}$(Å)	W $_{\lambda 5007}$(Å)
	(1)	(2)	(3)	(4)	(5)	(6)	(7)	(8)	(9)	(10)
1	HS 0940+3737*	48:	-	14.00	22.17	0.64	0.21	-	5	73
2	HS 0948+3723	+20	-	-	-	-	-	-	+76	58
3	HS 0954+3612	84	1.71	3.21	3.16	0.11	0.30	55	21	72
4	HS 0956+3847	68	3.02	4.06	2.93	0.09	0.06:	295	59	225
5	HS 1012+3655	49	1.50	4.53	3.42	0.11	0.16:	67	55	302
6	HS 1015+3737*	+133:	-	-	-	0.58	0.73	-	+27	94
7	HS 1018+3619*	68:	3.78	4.15	3.38	0.06:	0.17	98	47	212
8	HS 1024+3648*	40:	-	4.20	8.61	0.59	0.33	-	8	37
9	HS 1053+3722*	39:	-	3.35	5.76	0.23	0.31	-	15	53
10	HS 1058+3553	36	4.14	5.72	5.47	0.12	0.29	43	11	68
11	HS 1103+3627*	109:	-	2.92	5.47	0.25	0.13	-	12	35
12	HS 1103+3758*	25:	-	1.51	1.96	0.10:	0.39	-	20	33
13	HS 1106+3621	14	1.04	10.51	4.92	-	-	58	17	197
14	HS 1107+3524	13	5.69	4.04	4.37	-	0.39:	33	7	28
15	HS 1107+3637	+45	-	-	-	-	-	-	+316	144
16	HS 1107+3710*	+117:	-	-	-	0.65	0.23	-	+44	-
17	HS 1107+3712	27	3.28	4.64	4.00	-	-	23	12	60
18	HS 1133+3852	15	4.04	13.92	5.04	0.07	-	146	22	332
19	HS 1134+3805*	77:	2.81	4.20	2.65	-	0.18	440	65	253
20	HS 1139+3712*	32:	-	3.45	3.75	0.12	0.18	-	71	259
21	HS 1148+3827*	49:	0.72	5.70	4.05	0.05:	0.09	147	79	469
22	HS 1158+3837	93	2.37	3.67	3.37	0.05	0.08	75	27	105
23	HS 1159+3940	+31	-	-	-	-	-	-	+74	22
24	HS 1207+3957	79	1.47	3.86	2.29	-	0.07:	69	42	165
25	HS 1209+3726	9	-	11.65	9.18	-	-	-	4	45
26	HS 1210+3759*	+32:	-	-	-	0.15	-	-	+20	9
27	HS 1214+3922	621	0.85	4.73	2.79	-	0.03:	136	105	522
28	HS 1214+3801*	683:	0.49	5.44	2.74	0.05:	0.07	101	313	1557
29	HS 1237+3900	28	0.68	3.79	2.52	0.20:	-	39	36	138
30	HS 1248+3523	82	1.67	3.29	3.39	-	0.06	56	38	136
31	HS 1249+4021*	28:	-	3.25	5.66	0.29	0.51	-	7	24
32	HS 1254+3740	75	1.06	6.33	3.57	-	-	46	53	336
33	HS 1257+3658*	15:	-	6.21	2.94	0.10	0.17	-	36	255
34	HS 1302+3607	88	1.70	4.05	3.25	0.14	0.17:	19	21	88
35	HS 1309+3701	26	2.15	4.77	5.04	-	0.09:	43	25	128
36	HS 1311+3641*	+49:	-	-	-	0.32	0.43	-	+36	-
37	HS 1323+3851*	15:	-	4.28	4.27	0.03	0.11	-	13	56
38	HS 1327+3731*	36:	-	5.90	7.26	-	0.17	-	9	53
39	HS 1331+3545*	74:	3.27	4.64	2.89	0.02:	0.16	114	62	295
40	HS 1331+3657	21	2.13	6.43	3.39	-	0.13:	328	140	962
41	HS 1333+3717*	193:	2.30	4.72	3.27	0.09	0.13	161	149	648
42	HS 1341+3700*	54:	-	1.93	4.51	0.30	0.39	-	15	31
43	HS 1347+3811	+28	-	-	-	-	-	249	+51	85

Table 4. (Continued)

#	Name	F(H$\beta$)a	$\frac{F(\lambda 3727)}{F(\rm H\beta)}$	$\frac{F(\lambda 5007)}{F(\rm H\beta)}$	$\frac{F(\rm H\alpha)}{F(\rm H\beta)}$	$\frac{F(\lambda 6583)}{F(\rm H\alpha)}$	$\frac{F([\rm SII])}{F(\rm H\alpha)}$	W $_{\lambda 3727}$(Å)	W $_{\rm H\beta}$(Å)	W $_{\lambda 5007}$(Å)
	(1)	(2)	(3)	(4)	(5)	(6)	(7)	(8)	(9)	(10)
44	HS 1402+3945	19	2.05	1.53	9.37	0.48	0.30	13	6	11
45	HS 1414+3605*	+8:	-	-	-	1.76	-	-	+40	61
46	HS 1424+3836	51	0.92	7.01	3.37	-	0.05:	184	73	556
47	HS 1425+3847*	59:	-	3.17	4.36	0.13	0.23	-	16	50
48	HS 1428+3545	47	2.26	6.20	3.87	-	-	94	41	271
49	HS 1434+3644*	27:	-	5.93	3.02	0.02:	0.13	-	48	290
50	HS 1437+4002	12	-	4.60	3.00	-	-	-	30	128
51	HS 1447+3636*	61:	-	4.59	1.95	0.06	0.10	-	79	408
52	HS 1449+3647	83	1.10	5.51	3.24	-	0.11	33	84	414
53	HS 1457+3652	100	-	3.82	1.66	-	-	-	67	279
54	HS 1458+3726*	+12:	-	-	-	-	-	-	+11	-
55	HS 1513+3612*	45:	2.20	5.47	5.55	-	0.16	89	53	273
56	HS 1519+4007*	72:	0.66	5.77	2.90	-	0.10	19	34	200
57	HS 1520+3717	11	-	6.79	4.64	-	-	-	6	47
58	HS 1524+3536*	86:	1.54	5.41	2.70	0.08	0.09	84	74	320
59	HS 1526+3634	110	1.14	4.65	2.36	-	0.23	136	77	385
60	HS 1526+3729*	+29:	-	-	-	1.52	0.94	-	+6	10
61	HS 1527+3912	36	3.39	1.17	3.77	0.17	0.22	28	10	13
62	HS 1529+4003*	30:	-	3.03	5.19	0.24	0.20	-	9	29
63	HS 1530+3617	12	-	4.29	3.38	-	-	-	4	19
64	HS 1535+3747*	14:	-	5.20	2.95	-	-	-	33	178
65	HS 1536+3958	90	-	4.52	4.01	-	0.27	-	24	114
66	HS 1558+3543	+42	-	-	-	-	-	49	+73	17
67	HS 1543+3830	115	2.33	4.21	3.01	0.09	0.08:	78	27	123
68	HS 1557+3549*	13:	-	3.72	3.98	-	0.24	-	14	54
69	HS 1558+3636*	49:	-	2.64	3.63	0.04:	0.25	-	24	68
70	HS 1608+3654	+105	-	-	-	-	0.22	-	+60	80
71	HS 1613+3701	49	3.13	4.10	5.61	0.10	0.18	48	14	62
72	HS 1615+3521*	7:	-	5.30	5.72	0.06	0.16	-	5	26
73	HS 1619+3557*	22:	-	4.22	4.27	0.06	0.22	-	21	89
74	HS 1624+3618	31	1.07	5.96	-	-	-	67	70	390
75	HS 1638+3938	87	1.58	6.13	3.74	0.04:	0.19	77	62	367
76	HS 1643+4015	87	2.45	3.32	3.46	0.08	0.17	49	23	81
77	HS 1645+3551*	16:	-	5.34	3.41	0.05:	0.09	-	23	133
78	HS 1653+3634	346	1.08	5.16	2.37	0.03	0.11	124	102	561
79	HS 1656+3927	31:	-	21.41	3.33	1.59	0.58	-	4:	81
80	HS 1711+3756*	89:	3.46	4.38	3.98	-	0.20	108	33	146
81	HS 1721+3615	57	1.72	7.25	4.28	0.10	0.16	54	45	363
* Objects observed under poor photometric conditions.
a Flux in 10-16 ergs s-1 sm-2 Å-1 .
+ Parameters for H$\alpha$ emission line.
: Parameters with less confident values.

 

Table 5: Galaxies with Nondetected Emission Lines

Name	$\alpha\,(1950)$	$\delta\,(1950)$	$v^{\,a}_{0}$	m$_{\rm B}$	M $_{\rm B}^{\,b}$	Absorption lines
(1)	(2)	(3)	(4)	(5)	(6)	(7)
HS 1639+3535	16h 39m 25.7s	+35$^{\circ}$ 35' 49''	21285:	18.0	-19.3	Gband, NaD, H$\alpha$
HS 1711+3619	17 11   05.4	+36 19  50	5696	+19.2	-15.2	H$\beta$, Mgb, NaD, H$\alpha$
a Heliocentric velocities.
b Absolute magnitudes are not corrected for the Galaxy extinction.
+ APM magnitude.
: less confident values.

 

Table 6: Stars

#	Name	$\alpha\,(1950)$	$\delta\,(1950)$	mB	Type	Spectral features
	(1)	(2)	(3)	(4)	(5)	(6)
1	HS 1002+3900	10 02 47.5	39 00 24	16.9	A-F	CaK, CaH, Gband, H$\beta$, NaD?, H$\alpha$
2	HS 1202+4023	12 02 04.0	40 23 23	+19.0	M
3	HS 1207+3818	12 07 51.5	38 18 18	+19.5	A	H$\delta$, H$\gamma$, H$\beta$, Mgb, H$\alpha$
4	HS 1207+4007	12 07 44.9	40 07 52	+20.0	M
5	HS 1218+3857	12 18 15.0	38 57 12	+19.9	K	TiI,II4533, Mgb, NaD, TiO 6156-6180, H$\alpha$
6	HS 1334+3521	13 34 37.6	35 21 39	+19.3	M
7	HS 1513+3616	15 13 14.5	36 16 58	17.9	F-G	CaK, CaH, Gband, H$\beta$, NaD, H$\alpha$
8	HS 1514+3908	15 14 23.3	39 08 43	+18.5	F-G	CaK, CaH, Gband, Mgb
9	HS 1518+3600	15 18 55.1	36 00 44	+18.7	F-G	H$\beta$, Mgb, NaD, H$\alpha$
10	HS 1609+3909	16 09 57.3	39 09 13	18.5	F-G	CaK, H$\beta$, Mgb, NaD, H$\alpha$
11	HS 1652+3851	16 52 15.1	38 51 39	19.1		MgFe 4703, Mgb, NaD
12	HS 1726+3514	17 26 47.6	35 14 42	17.4	A-F	CaK, CaH, Gband, H$\beta$, Mgb, NaD, H$\alpha$
13	HS 1730+3607	17 30 36.1	36 07 22	18.3	F-G	CaK, CaH, H$\beta$, H$\alpha$
+ APM magnitude.