Bibliography

**Table 3:** Coordinates, Velocities and Magnitudes of Emission-Line Galaxies
#	Name	$\alpha\,(1950)$	$\delta\,(1950)$	$V_{hel}^{\,a}\pm\sigma_V$	m_B	M $_{B}^{\;\;b}$	Type	Other names from NED
								and number of reference
	(1)	(2)	(3)	(4)	(5)	(6)	(7)	(8)
1	HS 0732+3529	07 32 23.3	+35 29 07	3730 $\pm$ 42	17.80	-15.68	BCG
2	HS 0758+3901	07 58 58.2	+39 01 29	11621 $\pm$ 57	19.20	-16.75	BCG
3	HS 0759+3811	07 59 17.0	+38 11 51	6142 $\pm$ 54	17.80	-16.77	BCG
4	HS 0801+3740	08 01 51.5	+37 40 21	9823 $\pm$ 54	18.70	-16.89	BCG
5	HS 0801+3746 $^\dagger$	08 01 47.5	+37 46 06	10793 $\pm$ 100	16.20	-19.59	NON
6	HS 0803+3648	08 03 29.2	+36 48 38	9698 $\pm$ 66	18.40	-17.16	BCG
7	HS 0826+3521	08 26 52.2	+35 21 17	18910 $\pm$ 200	19.20	-17.81	NON
8	HS 0834+3741	08 34 11.6	+37 41 14	12509 $\pm$ 15	18.30	-17.81	BCG?
9	HS 0837+3816	08 37 53.4	+38 16 08	12269 $\pm$ 3	17.80	-18.27	SBN?
10	HS 0840+3938	08 40 18.5	+39 38 21	9646 $\pm$ 102	17.40	-18.15	BCG?
11	HS 0840+4013	08 40 42.4	+40 13 23	8887 $\pm$ 15	17.40	-17.97	DANS?	KUG 0840+402
12	HS 0841+3959	08 41 31.0	+39 59 15	34316 $\pm$ 90	+18.10	-20.20	SBN
13	HS 0843+3637	08 43 23.6	+36 37 23	3207 $\pm$ 51	15.40	-17.76	BCG	Mkn 627,CG 224, 1
14	HS 0847+3639	08 47 29.5	+36 39 17	7659 $\pm$ 108	18.10	-16.95	SBN?	KUG 0847+366, 7
15	HS 0852+3614	08 52 00.8	+36 14 54	8123 $\pm$ 72	19.20	-15.97	BCG?
16	HS 0852+4003	08 52 53.2	+40 03 41	1941 $\pm$ 20	16.50	-15.56	BCG	KUG 0852+400A
17	HS 0900+3651	09 00 55.0	+36 51 10	17303 $\pm$ 48	18.40	-18.42	BCG
18	HS 0902+3759	09 02 37.5	+37 59 39	14331 $\pm$ 60	19.30	-17.11	SBN	IRAS 09026+3759
19	HS 0902+4005	09 02 58.3	+40 05 38	14453 $\pm$ 27	17.80	-18.62	BCG
20	HS 0903+4349	09 03 31.9	+43 49 45	7611 $\pm$ 100	20.20	-14.83	BCG
21	HS 0904+4357	09 04 12.7	+43 57 31	14814 $\pm$ 74	18.70	-17.78	DANS?
22	HS 0904+4400	09 04 10.1	+44 00 56	17316 $\pm$ 55	17.40	-19.42	BCG?
23	HS 0905+3948	09 05 45.2	+39 48 24	12850 $\pm$ 21	18.60	-17.57	BCG
24	HS 0907+3728	09 07 02.4	+37 28 08	9045 $\pm$ 30	16.40	-19.01	SBN
25	HS 0913+3516	09 13 59.1	+35 16 48	17098 $\pm$ 63	19.50	-17.29	BCG
26	HS 0925+3529	09 25 41.4	+35 29 47	4556 $\pm$ 15	19.20	-14.72	BCG
27	HS 0928+3725 $^\dagger$	09 28 24.7	+37 25 25	14788 $\pm$ 39	18.00	-18.47	SBN?
28	HS 0928+4006	09 28 35.6	+40 06 57	4295 $\pm$ 33	18.90	-14.89	BCG
29	HS 0930+3548	09 30 08.3	+35 48 41	6871 $\pm$ 30	18.50	-16.31	BCG
30	HS 0934+3629 $^\dagger$	09 34 00.3	+36 29 07	53840 $\pm$ 66	17.50	-21.78	Sy1?	IRAS F09339+3629
31	HS 0936+3601 $^\dagger$	09 36 03.9	+36 01 40	6011 $\pm$ 37	17.30	-17.22	DANS?
32	HS 0936+3648 $^\dagger$	09 36 19.7	+36 48 04	6018 $\pm$ 39	16.00	-18.52	SBN?	CG270, 4
33	HS 0938+3544 $^\dagger$	09 38 45.7	+35 44 18	56334 $\pm$ 61	18.60	-20.78	Sy1?
34	HS 0942+3600	09 42 09.4	+36 00 30	6668 $\pm$ 51	16.20	-18.54	BCG	CG 278, 10
35	HS 0942+3644	09 42 41.2	+36 44 58	9856 $\pm$ 36	15.80	-19.79	SBN	CG 283
36	HS 0947+3559	09 47 33.7	+35 59 55	5960 $\pm$ 54	16.30	-18.20	SBN	CG295, KUG 0947+359, 1
37	HS 0951+3606	09 51 24.7	+36 06 29	12023 $\pm$ 59	17.50	-18.52	SBN?
38	HS 0951+3841	09 51 46.4	+38 41 13	5172 $\pm$ 10	16.80	-17.39	BCG
39	HS 0952+3803	09 52 39.9	+38 03 27	9535 $\pm$ 106	18.20	-17.32	DANS?

Table 3. (Continued)

# Name $\alpha\,(1950)$ $\delta\,(1950)$ $V_{hel}^{\,a}\pm\sigma_V$ m_B M $_{B}^{\;\;b}$ Type Other names from NED

and number of reference

(1) (2) (3) (4) (5) (6) (7) (8)

40 HS 0958+4043 09 58 23.4 +40 43 45 13493 $\pm$ 56 19.50 -16.78 BCG

41 HS 1014+4030 10 14 26.2 +40 30 00 19986 $\pm$ 46 17.40 -19.73 BCG

42 HS 1014+4916 10 14 01.9 +49 16 47 15904 $\pm$ 29 18.00 -18.63 SBN?

43 HS 1018+3847 10 18 49.6 +38 47 58 4204 $\pm$ 24 16.50 -17.24 BCG

44 HS 1021+3637 $^\dagger$ 10 21 57.3 +36 37 06 52551 $\pm$ 108 18.20 -21.03 SBN?

45 HS 1021+4218 10 21 12.8 +42 18 36 11000 $\pm$ 20 18.00 -17.83 BCG

46 HS 1025+4005 $^\dagger$ 10 25 51.8 +40 05 04 9040 $\pm$ 45 15.90 -19.51 BCG KUG 1025+400D

47 HS 1026+3521 10 26 25.7 +35 21 02 11129 $\pm$ 30 18.20 -17.66 BCG

48 HS 1028+3843 10 28 57.7 +38 43 34 9014 $\pm$ 21 19.40 -16.00 BCG

49 HS 1047+3714 $^\dagger$ 10 47 13.6 +37 14 23 10461 $\pm$ 45 16.30 -19.42 LINER?

50 HS 1048+4026 10 48 00.8 +40 26 08 38840 $\pm$ 51 18.90 -19.67 SBN?

51 HS 1050+4002 10 50 40.4 +40 02 35 8451 $\pm$ 45 17.90 -17.36 BCG

52 HS 1059+3934 10 59 22.0 +39 34 54 3274 $\pm$ 66 18.20 -15.00 BCG

53 HS 1102+3644 11 02 05.1 +36 44 50 22012 $\pm$ 204 17.00 -20.34 LINER?

54 HS 1107+3524 11 07 53.1 +35 24 36 9492 $\pm$ 18 17.40 -18.11 BCG 3

55 HS 1107+3637 11 07 04.0 +36 37 16 8088 $\pm$ 15 19.50 -15.66 BCG 3

56 HS 1107+3831 11 07 09.7 +38 31 14 9543 $\pm$ 33 +14.34 -21.18 BCG CG1388, KUG 1107+385

57 HS 1116+3951 11 16 33.9 +39 51 58 10090 $\pm$ 131 +16.93 -18.71 SBN

58 HS 1118+3842 11 18 46.8 +38 42 06 10433 $\pm$ 75 +18.52 -17.20 BCG

59 HS 1124+3635 11 24 49.4 +36 35 59 9160 $\pm$ 21 +17.96 -17.43 BCG

60 HS 1125+3624 11 25 43.9 +36 24 23 10488 $\pm$ 39 +18.31 -17.42 BCG

61 HS 1125+3748 11 25 22.4 +37 48 35 10689 $\pm$ 18 +16.50 -19.27 BCG CSO 343

62 HS 1126+3701 11 26 33.8 +37 01 27 12808 $\pm$ 50 +16.02 -20.16 BCG

63 HS 1129+3730 11 29 11.2 +37 30 14 12787 $\pm$ 33 +17.71 -18.45 BCG

64 HS 1134+3639 11 34 15.7 +36 39 52 1595 $\pm$ 36 17.10 -14.54 BCG NPM1G +36.0258

65 HS 1134+3640 11 34 00.5 +36 40 19 1462 $\pm$ 58 SA in Sp? SA in NGC 3755

66 HS 1135+3709 11 35 38.0 +37 09 58 3251 $\pm$ 49 18.10 -15.08 DANS

67 HS 1144+3552 11 44 37.6 +35 52 38 11001 $\pm$ 33 +17.16 -18.67 BCG

68 HS 1145+3709 11 45 53.4 +37 09 55 12129 $\pm$ 39 16.60 -19.44 SBN CSO 365, KUG 1145+371, 1

69 HS 1147+3653 11 47 53.3 +36 53 14 9207 $\pm$ 43 +17.80 -17.65 DANS?

70 HS 1150+3756 11 50 14.8 +37 56 04 11183 $\pm$ 90 +19.08 -16.79 BCG? PC 1150+3756, 8

71 HS 1159+3701 11 59 34.6 +37 01 29 6847 $\pm$ 67 17.40 -17.40 BCG

72 HS 1221+3721 12 21 21.1 +37 21 56 3907 $\pm$ 27 17.90 -15.68 BCG

73 HS 1228+3632 12 28 04.7 +36 32 12 10329 $\pm$ 54 +19.30 -16.40 BCG

74 HS 1240+3902 12 40 52.9 +39 02 34 7030 $\pm$ 30 +17.02 -17.84 BCG

75 HS 1300+3646 13 00 24.1 +36 46 31 9081 $\pm$ 48 +18.41 -17.01 BCG NGP9 F269-0522706

76 HS 1301+3835 13 01 26.8 +38 35 02 8732 $\pm$ 45 17.40 -17.93 BCG?

77 HS 1308+3545 13 08 43.3 +35 45 55 776 $\pm$ 54 18.10 -11.97 SA in Im UGC 8261

78 HS 1309+3806 13 09 17.9 +38 06 54 16011 $\pm$ 36 +19.23 -17.42 BCG NGP9 F269-0162165

79 HS 1318+3624 13 18 34.4 +36 24 48 7590 $\pm$ 45 18.00 -17.03 BCG

Table 3. (Continued)

# Name $\alpha\,(1950)$ $\delta\,(1950)$ $V_{hel}^{\,a}\pm\sigma_V$ m_B M $_{B}^{\;\;b}$ Type Other names from NED

and number of reference

(1) (2) (3) (4) (5) (6) (7) (8)

80 HS 1324+4019 13 24 05.3 +40 19 39 7671 $\pm$ 39 17.60 -17.45 BCG

81 HS 1331+3657 13 31 46.5 +36 57 21 17949 $\pm$ 22 18.00 -18.90 BCG 3

82 HS 1344+3511 13 44 53.9 +35 11 21 16101 $\pm$ 57 16.80 -19.86 SBN CG 1189, 2

83 HS 1347+3553 13 47 12.2 +35 53 48 17062 $\pm$ 111 19.50 -17.28 DANS?

84 HS 1347+3811 13 47 02.3 +38 11 35 2804 $\pm$ 36 18.80 -14.06 BCG 3, 6

85 HS 1349+3942 13 49 22.9 +39 42 04 1752 $\pm$ 50 16.70 -15.14 BCG 5, 6

86 HS 1350+3538 $^\dagger$ 13 50 13.8 +35 38 37 17791 $\pm$ 519 17.90 -18.98 SBN?

87 HS 1400+3927 14 00 29.9 +39 27 38 1396 $\pm$ 39 17.20 -14.15 BCG CG 330, 9

88 HS 1408+3857 14 08 37.6 +38 57 11 7701 $\pm$ 37 16.80 -18.26 BCG CG 369, 9

89 HS 1425+3835 $^\ddagger$ 14 25 14.6 +38 35 33 6548 $\pm$ 21 16.80 -17.91 BCG? CG 0435, 5, 6

90 HS 1435+3645 $^\ddagger$ 14 35 23.5 +36 45 12 15655 $\pm$ 48 +17.10 -19.50 BCG?

91 HS 1440+3805 14 40 08.8 +38 05 06 9599 $\pm$ 27 16.70 -18.84 DANS? NPM1G +38.0321, 5, 6

92 HS 1440+3828 $^\ddagger$ 14 40 40.0 +38 28 52 20761 $\pm$ 12 17.28 -19.93 SBN?

93 HS 1450+3903 $^\ddagger$ 14 50 04.8 +39 03 11 18096 $\pm$ 42 +16.83 -20.08 SBN

94 HS 1502+4152 15 02 31.3 +41 52 35 5004 $\pm$ 30 +16.35 -17.77 BCG 5, 6

95 HS 1504+3922 15 04 15.6 +39 22 16 8962 $\pm$ 54 18.80 -16.59 BCG CG 624, 9

96 HS 1504+3923 15 04 10.9 +39 23 21 9189 $\pm$ 36 18.30 -17.14 BCG CG 623

97 HS 1509+4409 15 09 56.8 +44 09 28 8284 $\pm$ 69 SBN?

98 HS 1519+3948 $^\ddagger$ 15 19 49.0 +39 48 19 14716 $\pm$ 21 17.60 -18.86 BCG?

99 HS 1520+3717 15 20 30.6 +37 17 56 11239 $\pm$ 63 +15.42 -20.46 BCG 3

100 HS 1521+3617 $^\ddagger$ 15 21 04.9 +36 17 24 6998 $\pm$ 24 +16.88 -17.97 BCG

101 HS 1524+4205 15 24 08.0 +42 05 01 6700 $\pm$ 30 18.40 -16.36 DANS? 5

102 HS 1526+4045 15 26 56.7 +40 45 17 8610 $\pm$ 9 17.70 -17.60 DANS? 5

103 HS 1528+3858 $^\ddagger$ 15 28 43.3 +38 58 11 10579 $\pm$ 69 17.60 -18.15 DANS?

104 HS 1543+3602 15 43 12.5 +36 02 46 1889 $\pm$ 18 16.00 -16.00 BCG ABELL 2124

105 HS 1543+4525 15 43 23.3 +45 25 45 11519 $\pm$ 27 17.40 -18.53 DANS? 5, 6

106 HS 1544+3803 $^\ddagger$ 15 44 21.6 +38 03 12 12008 $\pm$ 27 17.20 -18.82 BCG?

107 HS 1546+3526 15 46 54.3 +35 26 24 16525 $\pm$ 27 18.20 -18.52 BCG

108 HS 1546+4755 15 46 56.5 +47 55 34 11250 $\pm$ 9 18.90 -16.98 BCG 5, 6

109 HS 1558+3543 15 58 27.3 +35 43 15 20284 $\pm$ 69 18.30 -18.87 BCG 3

110 HS 1608+3654 16 08 31.5 +36 54 42 9586 $\pm$ 12 17.30 -18.23 BCG 3

111 HS 1609+4827 16 09 44.4 +48 27 44 2817 $\pm$ 24 16.40 -16.47 BCG 5, 6

112 HS 1612+3650 16 12 34.7 +36 50 06 8750 $\pm$ 24 18.60 -16.73 BCG

113 HS 1612+3720 $^\ddagger$ 16 12 30.0 +37 20 35 11296 $\pm$ 12 17.50 -18.39 BCG

114 HS 1617+3757 16 17 32.0 +37 57 55 9118 $\pm$ 15 18.20 -17.22 BCG

115 HS 1619+3523 16 19 47.3 +35 23 16 15274 $\pm$ 66 16.80 -19.74 LINER? KUG 1619+353B

116 HS 1619+3752 16 19 55.7 +37 52 35 9883 $\pm$ 9 17.30 -18.30 BCG PC 1619+3752, 8

Table 3. (Continued)

# Name $\alpha\,(1950)$ $\delta\,(1950)$ $V_{hel}^{\,a}\pm\sigma_V$ m_B M $_{B}^{\;\;b}$ Type Other names from NED

and number of reference

(1) (2) (3) (4) (5) (6) (7) (8)

117 HS 1620+4003 $^\dagger$ 16 20 49.9 +40 03 47 18903 $\pm$ 45 16.20 -20.81 LINER

118 HS 1627+3927 $^\ddagger$ 16 27 27.4 +39 27 26 7984 $\pm$ 9 17.80 -17.34 BCG ABELL 2199:[BO85]156

119 HS 1627+3945 $^\ddagger$ 16 27 04.8 +39 45 29 8122 $\pm$ 15 +15.11 -20.06 SBN? ABELL 2199:[BO85]107

^a Heliocentric velocities.; ^b Absolute magnitudes are not corrected for galactic extinction

+ APM magnitudes; $^\dagger$ objects from the second priority random sample; $^\ddagger$ galaxies from the APM selected sample

References: 1 - Augarde et al. ([1994]); 2 - de Grijp et al. ([1992]); 3 - Hopp et al. ([2000]); 4 - Huchra et al. ([1995])

5 - Popescu et al. ([1996]); 6 - Popescu et al. ([2000]); 7 - Ramella et al. ([1995]); 8 - Schneider et al. ([1994])

9 - Tift et al. ([1986]); 10 - Weistrop & Downes ([1991])

Table 4: Emission line parameters
# Name F(H $\beta$ )^a $\frac{F(\lambda 3727)}{F(H\beta)}$ $\frac{F(\lambda 5007)}{F(H\beta)}$ $\frac{F(H\alpha)}{F(H\beta)}$ $\frac{F(\lambda 6583)}{F(H\alpha)}$ $\frac{F([SII])}{F(H\alpha)}$ W $_{\lambda 3727}$ (Å) W $_{H\beta}$ (Å) W $_{\lambda 5007}$ (Å)

(1) (2) (3) (4) (5) (6) (7) (8) (9) (10)

1 HS 0732+3529 45 2.53 10.09 5.89 0.03 - 66 21 237

2 HS 0758+3901 15 4.93 6.00 4.40 0.06 0.23 108 28 199

3 HS 0759+3811 37 2.22 2.86 3.38 0.06 0.15 31 18 56

4 HS 0801+3740 42 3.17 2.55 3.38 0.11 0.35 96 38 106

5 HS 0801+3746 $^\dagger$ +47 - - - - - - +12 -

6 HS 0803+3648 33 3.21 3.52 3.64 0.09 0.23 65 29 111

7 HS 0826+3521 +56 - - - - 0.50 - +38 -

8 HS 0834+3741 36 2.78 2.33 1.14 - - 85 60 127

9 HS 0837+3816 13 6.92 4.77 4.38 0.35 - 66 10 48

10 HS 0840+3938 42 4.45 3.17 3.43 0.07 0.36 67 16 53

11 HS 0840+4013 +61 - - - 0.49 - 67 +36 -

12 HS 0841+3959 7 8.29 1.57 7.29 0.37 - 122 6 10

13 HS 0843+3637 326 2.64 4.28 4.47 0.04 0.17 112 66 343

14 HS 0847+3639 87 4.36 1.64 3.92 0.11 0.22 56 14 23

15 HS 0852+3614 5 6.00 4.40 4.00 - - 42 7 30

16 HS 0852+4003 81 2.86 4.94 3.77 - 0.16 52 23 118

17 HS 0900+3651 38 2.16 4.63 3.37 0.05 0.23 81 52 225

18 HS 0902+3759 12 5.58 2.00 12.42 0.42 0.54 41 6 11

19 HS 0902+4005 82 3.54 3.83 3.26 0.04 0.25 94 32 130

20 HS 0903+4349* 7: - 6.00 - - - - 28 196

21 HS 0904+4357* 5: 3.40 1.80 - - - 42 16 25

22 HS 0904+4400* 10: 1.50 2.40 - - - 43 32 67

23 HS 0905+3948 44 3.05 2.77 3.98 - 0.15 56 20 57

24 HS 0907+3728 111 1.53 0.52 5.26 0.38 0.25 24 14 7

25 HS 0913+3516 19 3.79 2.95 2.89 0.09 0.51 94 17 51

26 HS 0925+3529 44 2.30 4.55 3.39 0.01 0.18 59 24 115

27 HS 0928+3725 $^\dagger$ 64 3.94 1.63 3.41 0.17 0.34 68 20 33

28 HS 0928+4006 40 1.35 5.20 3.50 0.04 0.19 39 21 109

29 HS 0930+3548 25 4.32 3.40 4.04 0.09 0.10 51 10 36

30 HS 0934+3629 $^\dagger$ 88 - 0.74 4.77 0.18 - - 33 25

31 HS 0936+3601 $^\dagger$ 5 - 2.80 4.80 - - - 7 18

32 HS 0936+3648 $^\dagger$ 47 3.32 0.89 3.49 0.24 0.30 28 9 8

33 HS 0938+3544 $^\dagger$ +23 - +0.78 - - - - +108 45

34 HS 0942+3600 26 2.50 2.73 4.62 0.13 0.39 98 23 72

35 HS 0942+3644 30 3.73 2.00 4.57 0.24 0.43 39 9 17

36 HS 0947+3559 30 2.50 1.50 4.47 0.18 0.31 43 15 21

37 HS 0951+3606 24 1.50 2.33 6.67 0.21 0.34 51 16 37

38 HS 0951+3841 42 3.76 3.19 4.55 0.08 0.28 122 34 115

39 HS 0952+3803 4 - 2.75 2.75 - - - 10 27

40 HS 0958+4043* 19: 2.05 5.95 - - - 105 73 283

Table 4. (Continued)

#	Name	F(H $\beta$ )^a	$\frac{F(\lambda 3727)}{F(H\beta)}$	$\frac{F(\lambda 5007)}{F(H\beta)}$	$\frac{F(H\alpha)}{F(H\beta)}$	$\frac{F(\lambda 6583)}{F(H\alpha)}$	$\frac{F([SII])}{F(H\alpha)}$	W $_{\lambda 3727}$ (Å)	W $_{H\beta}$ (Å)	W $_{\lambda 5007}$ (Å)
	(1)	(2)	(3)	(4)	(5)	(6)	(7)	(8)	(9)	(10)
41	HS 1014+4030*	69:	2.52	3.25	-	-	-	102	39	139
42	HS 1014+4916*	10:	4.90	1.00	-	-	-	102	15	16
43	HS 1018+3847	21	4.10	4.38	6.24	0.11	0.27	24	5	21
44	HS 1021+3637 $^\dagger$	+18	-	+0.67	-	-	-	-	+34	19
45	HS 1021+4218*	13:	2.46	3.92	-	-	-	51	91	211
46	HS 1025+4005 $^\dagger$	72	3.07	3.22	4.04	0.09	0.25	54	19	61
47	HS 1026+3521	15	1.87	7.53	5.60	0.05	0.25	49	20	166
48	HS 1028+3843	135	0.44	7.03	2.99	0.00	-	70	404	2819
49	HS 1047+3714 $^\dagger$	+38	-	+2.24	-	1.97	0.87	14	+6	15
50	HS 1048+4026	+46	-	+0.78	-	-	-	14	+43	33
51	HS 1050+4002	30	3.90	3.87	3.47	0.02	-	106	31	122
52	HS 1059+3934	25	2.12	5.52	3.68	-	-	101	56	335
53	HS 1102+3644	+31	-	-	-	0.58	-	-	+11	-
54	HS 1107+3524	20	4.55	3.90	4.35	0.07	0.23	75	12	47
55	HS 1107+3637	21	2.43	5.24	3.67	0.04	0.12	-	39	210
56	HS 1107+3831	63	3.60	3.71	4.73	0.14	0.26	42	12	50
57	HS 1116+3951	34	5.21	1.62	3.00:	0.26	0.35	107	24	44
58	HS 1118+3842	13	4.54	6.15	3.00	0.23	-	118	27	170
59	HS 1124+3635	102	1.15	6.17	3.10	-	0.09	98	111	810
60	HS 1125+3624	41	3.41	3.39	3.46	0.14	0.27	127	30	112
61	HS 1125+3748	17	5.88	5.29	4.94	0.07	0.23	77	10	56
62	HS 1126+3701	32	3.38	6.09	3.53	0.06	0.25	44	12	78
63	HS 1129+3730	40	3.05	3.85	3.70	-	-	77	35	137
64	HS 1134+3639	10	7.30	5.80	4.70	0.09	0.36	48	8	55
65	HS 1134+3640	103	2.15	4.22	2.82	0.03	0.14	97	146	689
66	HS 1135+3709	+7	-	+0.71	-	-	-	-	+19	9
67	HS 1144+3552	23	2.96	4.74	3.26	-	-	201	151	686
68	HS 1145+3709	32	3.69	2.06	4.63	0.24	0.40	56	14	30
69	HS 1147+3653	+18	-	+0.33	-	0.33	0.72	-	+37	10
70	HS 1150+3756	14	3.29	3.29	2.21	-	-	141	26	90
71	HS 1159+3701	16	3.19	3.38	4.25	0.12	0.25	58	19	61
72	HS 1221+3721	27	1.30	4.78	2.70	0.03	0.21	41	41	190
73	HS 1228+3632	34	2.41	2.65	2.50	0.15	0.35	163	47	123
74	HS 1240+3902	77	1.12	5.36	3.12	-	0.08	83	101	498
75	HS 1300+3646	13	1.85	6.31	4.69	0.05	-	70	37	300
76	HS 1301+3835	6	8.00	5.67	6.50	0.21	0.72	21	3	20
77	HS 1308+3545	8	-	4.38	4.25	-	-	-	200:	333:
78	HS 1309+3806	50	0.48	8.30	3.96	-	-	73	218	1417
79	HS 1318+3624	26	2.54	4.62	4.08	0.07	0.25	81	31	138
80	HS 1324+4019	21	3.14	4.57	4.19	0.09	0.31	106	24	114

Table 4. (Continued)

#	Name	F(H $\beta$ )^a	$\frac{F(\lambda 3727)}{F(H\beta)}$	$\frac{F(\lambda 5007)}{F(H\beta)}$	$\frac{F(H\alpha)}{F(H\beta)}$	$\frac{F(\lambda 6583)}{F(H\alpha)}$	$\frac{F([SII])}{F(H\alpha)}$	W $_{\lambda 3727}$ (Å)	W $_{H\beta}$ (Å)	W $_{\lambda 5007}$ (Å)
	(1)	(2)	(3)	(4)	(5)	(6)	(7)	(8)	(9)	(10)
81	HS 1331+3657*	87:	1.16	6.55	-	-	-	49	81	525
82	HS 1344+3511	126	2.06	2.81	5.56	0.24	0.20	111	65	184
83	HS 1347+3553	13	1.69	-	2.77	-	-	27	16	-
84	HS 1347+3811	10	1.30	4.70	4.60	0.04	0.17	27	22	108
85	HS 1349+3942	23	2.43	3.26	5.30	0.11	0.29	41	15	54
86	HS 1350+3538 $^\dagger$	+19	-	+0.32	-	-	-	-	+15	6
87	HS 1400+3927	107	1.55	5.39	3.44	0.03	0.14	94	66	375
88	HS 1408+3857	53	3.15	3.91	3.64	0.05	0.15	57	19	76
89	HS 1425+3835 $^\ddagger$	45	4.20	2.11	-	-	-	94	11	25
90	HS 1435+3645 $^\ddagger$	9	-	3.11	4.33	0.13	0.41	-	11	26
91	HS 1440+3805	14	2.14	0.57	-	-	-	40	10	5
92	HS 1440+3828 $^\ddagger$	+16	-	-	-	0.31	-	44	+53	-
93	HS 1450+3903 $^\ddagger$	25	2.72	0.64	4.08	0.34	0.22	39	11	7
94	HS 1502+4152	22	2.09	3.55	-	-	-	50	34	109
95	HS 1504+3922	97	0.91	5.69	3.04	0.02	0.13	83	151	854
96	HS 1504+3923	68	1.29	5.96	3.41	-	-	65	66	402
97	HS 1509+4409	7	8.43	3.86	-	-	-	31	3	11
98	HS 1519+3948 $^\ddagger$	6	12.50	5.67	3.67	0.27	-	114	12	53
99	HS 1520+3717	11	5.36	4.73	4.36	0.10	0.46	81	7	36
100	HS 1521+3617 $^\ddagger$	18	2.39	4.67	3.39	0.07	-	61	16	81
101	HS 1524+4205	5	7.20	2.20	-	-	-	58	3	7
102	HS 1526+4045	4	8.00	3.00	-	-	-	23	2	6
103	HS 1528+3858 $^\ddagger$	+14	-	+0.93	-	-	-	-	+58	35
104	HS 1543+3602	226	1.82	5.14	3.17	-	0.10	88	46	246
105	HS 1543+4525	32	3.78	1.22	3.69	0.25	0.39	54	14	17
106	HS 1544+3803 $^\ddagger$	33	3.33	2.61	4.67	0.23	0.20	132	14	39
107	HS 1546+3526	33	2.30	4.15	3.18	0.06	0.27	110	46	194
108	HS 1546+4755	105	2.86	5.08	3.31	0.07	0.09	152	55	261
109	HS 1558+3543	40	2.92	3.80	3.00	0.06	0.12	234	58	228
110	HS 1608+3654	23	6.35	4.04	4.65	0.04	0.32	191	11	46
111	HS 1609+4827	70	2.79	3.33	4.31	0.09	0.27	34	13	44
112	HS 1612+3650	38	2.79	4.08	3.11	0.03	0.19	103	31	133
113	HS 1612+3720 $^\ddagger$	17	6.41	3.94	5.24	0.12	0.28	86	10	41
114	HS 1617+3757	149	0.98	6.68	2.93	-	0.07	171	215	1320
115	HS 1619+3523	52	1.87	3.85	4.48	0.60	0.38	25	9	35
116	HS 1619+3752	55	2.36	2.93	3.69	0.10	0.29	47	27	76
117	HS 1620+4003 $^\dagger$	70	1.94	5.90	7.06	0.56	0.46	22	10	60
118	HS 1627+3927 $^\ddagger$	33	1.55	4.55	3.24	0.05	0.14	64	50	233
119	HS 1627+3945 $^\ddagger$	15	2.73	3.00	8.07	0.21	0.37	24	5	14

^a Flux in 10^-16 ergs s^-1 sm^-2 Å^-1; * objects observed during non-photometric conditions
$^\dagger$ 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 $\alpha\,(1950)$ $\delta\,(1950)$ m_B Detected emission lines

(1) (2) (3) (4) (5) (6)

1 HS 0833+3516 08 33 50.4 +35 16 18 3.304 19.00 Ly $\alpha$ 1216 Å, Si IV/O IV] 1400 Å, C IV 1549 Å

2 HS 0844+3842 08 44 01.4 +38 42 13 3.177 19.70 Ly $\alpha$ 1216 Å, Si IV/O IV] 1400 Å, C IV 1549 Å

3 HS 0855+3724 08 55 59.7 +37 24 42 3.207 19.60 Ly $\alpha$ 1216 Å, C IV 1549 Å

4 HS 0857+3601 $^\dagger$ 08 57 55.0 +36 01 15 3.153 17.80 Ly $\alpha$ 1216 Å, Si IV/O IV] 1400 Å, C IV 1549 Å

5 HS 0954+3549 09 54 36.8 +35 49 40 3.296 +19.20 Ly $\alpha$ 1216 Å, Si IV/O IV] 1400 Å, C IV 1549 Å

6 HS 1005+3638 10 05 44.2 +36 38 01 3.162 17.50 Ly $\alpha$ 1216 Å, Si IV/O IV] 1400 Å, C IV 1549 Å

7 HS 1143+3954 11 43 10.9 +39 54 26 3.189 19.40 Ly $\alpha$ 1216 Å, Si IV/O IV] 1400 Å, C IV 1549 Å

8 HS 1215+3821 12 15 13.1 +38 21 45 3.161 +20.70 Ly $\alpha$ 1216 Å, Si IV/O IV] 1400 Å, C IV 1549 Å

^a Observed redshift; ⁺ APM magnitudes; $^\dagger$ objects from the second priority random sample

**Table 5:** Coordinates, Redshifts and Magnitudes of QSOs
#	Name	$\alpha\,(1950)$	$\delta\,(1950)$		m_B	Detected emission lines
	(1)	(2)	(3)	(4)	(5)	(6)
1	HS 0833+3516	08 33 50.4	+35 16 18	3.304	19.00	Ly $\alpha$ 1216 Å, Si IV/O IV] 1400 Å, C IV 1549 Å
2	HS 0844+3842	08 44 01.4	+38 42 13	3.177	19.70	Ly $\alpha$ 1216 Å, Si IV/O IV] 1400 Å, C IV 1549 Å
3	HS 0855+3724	08 55 59.7	+37 24 42	3.207	19.60	Ly $\alpha$ 1216 Å, C IV 1549 Å
4	HS 0857+3601 $^\dagger$	08 57 55.0	+36 01 15	3.153	17.80	Ly $\alpha$ 1216 Å, Si IV/O IV] 1400 Å, C IV 1549 Å
5	HS 0954+3549	09 54 36.8	+35 49 40	3.296	+19.20	Ly $\alpha$ 1216 Å, Si IV/O IV] 1400 Å, C IV 1549 Å
6	HS 1005+3638	10 05 44.2	+36 38 01	3.162	17.50	Ly $\alpha$ 1216 Å, Si IV/O IV] 1400 Å, C IV 1549 Å
7	HS 1143+3954	11 43 10.9	+39 54 26	3.189	19.40	Ly $\alpha$ 1216 Å, Si IV/O IV] 1400 Å, C IV 1549 Å
8	HS 1215+3821	12 15 13.1	+38 21 45	3.161	+20.70	Ly $\alpha$ 1216 Å, Si IV/O IV] 1400 Å, C IV 1549 Å

^a Observed redshift; ⁺ APM magnitudes; $^\dagger$ objects from the second priority random sample

Table 6: Galaxies without detected emission lines
# Name $\alpha\,(1950)$ $\delta\,(1950)$ m_B M Absorption lines

(1) (2) (3) (4) (5) (6) (7)

9 HS 0812+3516 $^\dagger$ 08 12 23.1 +35 16 23 33466 18.40 -19.85 CaK, CaH, H $\beta$ , NaD

10 HS 0843+3536 08 43 49.9 +35 36 24 15883 18.80 -17.83 CaK, CaH, H $\beta$ , NaD, H $\alpha$

11 HS 0929+3956 09 29 11.9 +39 56 52 6031 +19.27 -15.26 CaK, CaH, G_band, NaD, H $\alpha$

12 HS 0936+3753 09 36 14.4 +37 53 25 46285: 18.00 -20.95 CaK, CaH, G_band, H $\beta$ , MgIb, H $\alpha$

^a Heliocentric velocities; ^b Absolute magnitudes are not corrected for galactic extinction

$^\dagger$ objects from the second priority random sample; ⁺ APM magnitude; : less confident values

**Table 6:** Galaxies without detected emission lines
#	Name	$\alpha\,(1950)$	$\delta\,(1950)$		m_B	M	Absorption lines
	(1)	(2)	(3)	(4)	(5)	(6)	(7)
9	HS 0812+3516 $^\dagger$	08 12 23.1	+35 16 23	33466	18.40	-19.85	CaK, CaH, H $\beta$ , NaD
10	HS 0843+3536	08 43 49.9	+35 36 24	15883	18.80	-17.83	CaK, CaH, H $\beta$ , NaD, H $\alpha$
11	HS 0929+3956	09 29 11.9	+39 56 52	6031	+19.27	-15.26	CaK, CaH, G_band, NaD, H $\alpha$
12	HS 0936+3753	09 36 14.4	+37 53 25	46285:	18.00	-20.95	CaK, CaH, G_band, H $\beta$ , MgIb, H $\alpha$

^a Heliocentric velocities; ^b Absolute magnitudes are not corrected for galactic extinction
$^\dagger$ objects from the second priority random sample; ⁺ APM magnitude; : less confident values

**Table 7:** Stars
#	Name	$\alpha\,(1950)$	$\delta\,(1950)$	m_B	Type	Spectral features
	(1)	(2)	(3)	(4)	(5)	(6)
1	HS 0737+3902	07 37 24.4	+39 02 30	17.40	G	CaK, CaH, G_band, MgIb, CaFe5269, H
2	HS 0745+3600	07 45 35.6	+36 00 22	18.80	A-F	H, H
3	HS 0750+3637	07 50 51.5	+36 37 07	18.30	G	CaK, CaH, G_band, MgIb, NaD, H
4	HS 0753+3519 $^\dagger$	07 53 09.6	+35 19 59	16.70	F	CaK, CaH, H, H, H, CaFe5269, H
5	HS 0802+3809	08 02 01.0	+38 09 06	18.30	A-F	H, H
6	HS 0840+3615	08 40 50.4	+36 15 09	17.10	F	CaK, CaH, H, H
7	HS 0859+3519 $^\dagger$	08 59 35.5	+35 19 21	19.00	M
8	HS 0906+3846 $^\dagger$	09 06 55.1	+38 46 29	18.50	G	CaK, CaH, G_band, H, MgIb, CaFe5269
9	HS 0929+3657 $^\dagger$	09 29 38.9	+36 57 18	19.40	F-G	CaK, CaH, H, MgIb, CaFe5269, H
10	HS 0940+3753 $^\dagger$	09 40 19.1	+37 53 33	17.10	F	H, MgIb, H
11	HS 0941+3659 $^\dagger$	09 41 52.0	+36 59 20	16.50	F	CaK, CaH, G_band, H, MgIb, H
12	HS 1031+3524 $^\dagger$	10 31 37.2	+35 24 12	17.00	A	H, H, H
13	HS 1132+3904	11 32 17.3	+39 04 43	+17.84	A	H, H, H
14	HS 1245+3842 $^\dagger$	12 45 45.7	+38 42 19	16.80	F	CaK, CaH, H, MgIb, NaD, H
15	HS 1300+3748 $^\dagger$	13 00 56.6	+37 48 16	16.90	F	H, H, MgIb, H
16	HS 1408+3957	14 08 35.3	+39 57 29	18.70	F?	H, MgIb, H

$^\dagger$ objects from the second priority random sample; ⁺ APM magnitude

Table 8: Spectroscopic classification for objects from the ``random selected'' sample observed with the Calar Alto 2.2m telescope
# Name m_B Type

(1) (2) (3)

1 HS 1007+3948 17.40 NOEM

2 HS 1013+3804 17.70 Star

3 HS 1029+4020 16.70 Star

4 HS 1322+3708 16.40 BCG?

5 HS 1355+3911 19.20 Star

6 HS 1408+3524 16.80 ABS

7 HS 1417+3921 18.30 NOEM

8 HS 1420+3726 17.50 BCG?

9 HS 1423+3945 18.50 SA in Sp

10 HS 1459+3608 18.80 NOEM

11 HS 1537+3520 17.60 NOEM

12 HS 1545+3531 18.00 NOEM

13 HS 1547+4008 17.30 NOEM

14 HS 1601+3859 18.40 NOEM

15 HS 1616+3627 16.50 Sy1

16 HS 1649+3621 18.10 BCG?

17 HS 1720+3929 17.80 NOEM

**Table 8:** Spectroscopic classification for objects from the ``random selected'' sample observed with the Calar Alto 2.2m telescope
#	Name	m_B	Type
	(1)	(2)	(3)
1	HS 1007+3948	17.40	NOEM
2	HS 1013+3804	17.70	Star
3	HS 1029+4020	16.70	Star
4	HS 1322+3708	16.40	BCG?
5	HS 1355+3911	19.20	Star
6	HS 1408+3524	16.80	ABS
7	HS 1417+3921	18.30	NOEM
8	HS 1420+3726	17.50	BCG?
9	HS 1423+3945	18.50	SA in Sp
10	HS 1459+3608	18.80	NOEM
11	HS 1537+3520	17.60	NOEM
12	HS 1545+3531	18.00	NOEM
13	HS 1547+4008	17.30	NOEM
14	HS 1601+3859	18.40	NOEM
15	HS 1616+3627	16.50	Sy1
16	HS 1649+3621	18.10	BCG?
17	HS 1720+3929	17.80	NOEM

Next: Spectra of emission-line galaxies Up: The Hamburg/SAO Survey for Previous: Conclusions

Laboratory "Structure"
2000-11-25