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Table 1:

List of sources observed at 21 cm.

Object
  RA(2000) Dec(2000) Seyferta Morphologicalb $v_{\rm0}$ (LSR) z $D_{\rm L}$ $t_{\rm obs, on}$c Cali-d Resolutione rms noise
    [h] [m] [s] [$^\circ$] [$^\prime $] [ $^{\prime\prime}$] type type [km s-1]   [Mpc] [min] brators [km s-1] [Jy]
HE 0021-1819   00:23:55.3 -18:02:50   E, C 15 954 0.053 215.4 60 1, 1 1.3 0.008
HE 0040-1105   00:42:36.8 -10:49:21 Sy 1.5 E, C 12 578 0.042 169.6 60 1, 1 0.3 0.013
HE 0045-2145   00:47:41.3 -21:29:27   S 6403 0.021 86.0 60 2, 1 5.2 0.004
HE 0114-0015   01:17:03.6 +00:00:27   E, C, poss. M 13 682 0.046 184.3 90 2, 1, 1 1.3 0.006
HE 0119-0118   01:21:59.8 -01:02:25 Sy 1.5 E 16 412 0.055 221.5 60 1, 1 2.1 0.007
HE 0150-0344   01:53:01.4 -03:29:24   M 14 329 0.048 193.3 90 1, 3, 1 16.5 0.004
HE 0212-0059   02:14:33.6 -00:46:00 Sy 1.2 E, C 7921 0.026 106.2 60 2, 3 8.2 0.004
HE 0224-2834   02:26:25.7 -28:20:59   M, C 18 150 0.060 245.4 60 1, 1 8.0 0.003
HE 0227-0913   02:30:05.4 -08:59:53 Sy 1 S 4914 0.016 65.8 30 2 2.6 0.007
HE 0232-0900   02:34:37.7 -08:47:16 Sy 1 R, M, C 12 886 0.043 173.7 60 2, 1 32.0 0.002
HE 0253-1641   02:56:02.6 -16:29:16 Sy 2 S 9580 0.032 128.9 30 1 0.3 0.019
HE 0433-1028   04:36:22.2 -10:22:33 Sy 1 S 10 651 0.036 143.1 60 1, 1 2.1 0.007
HE 0853-0126   08:56:17.8 -01:38:07 Sy 1 E, C 17 899 0.060 242.1 60 1, 1 0.3 0.017
HE 0949-0122   09:52:18.9 -01:36:44 Sy 1.5 E 5905 0.020 79.1 60 4, 3 4.1 0.016
HE 1011-0403   10:14:20.6 -04:18:41 Sy 1 S, C 17 572 0.059 237.6 30 1 0.3 0.021
HE 1017-0305   10:19:32.9 -03:20:15 Sy 1 S, C, poss. M 14 737 0.049 199.0 30 1 0.3 0.018
HE 1029-1831   10:31:57.3 -18:46:34 Sy 1 S, C 12 112 0.040 163.1 60 3, 1 16.0 0.001
HE 1107-0813   11:09:48.5 -08:30:15   E 17 481 0.058 236.3 30 1 0.3 0.021
HE 1108-2813   11:10:48.0 -28:30:03 Sy 1.5 S 7198 0.024 96.5 90 4, 1, 1 0.3 0.017
HE 1126-0407   11:29:16.6 -04:24:08 Sy 1 S, C 18 006 0.060 243.7 30 1 0.3 0.020
HE 1237-0504   12:39:39.4 -05:20:40 Sy 1 S 2531 0.008 33.6 30 4 4.1 0.008
HE 1248-1356   12:51:32.4 -14:13:17 Sy 1 S, C 4338 0.015 58.2 60 4, 3 2.1 0.002
HE 1330-1013   13:32:39.1 -10:28:53 Sy 1 S, C 6744 0.023 90.4 90 1, 3, 3 16.5 0.006
HE 1353-1917   13:56:36.7 -19:31:44 Sy 1 S 10 472 0.035 140.7 60 1, 1 0.3 0.017
HE 2222-0026   22:24:35.3 -00:11:04   E 17 414 0.058 235.5 30 1 0.3 0.019
HE 2233+0124   22:35:41.9 +01:39:33 Sy 1 S, C 16 913 0.056 228.5 30 1 0.3 0.018
HE 2302-0857   23:04:43.4 -08:41:09 Sy 1.5 S, C 14 120 0.047 190.4 90 1, 1, 1 8.0 0.002

a
Taken from the NED; b E denotes elliptical morphology; S represents a spiral morphology; M stands for possible mergers or merger remnants; R denotes ringed objects; C marks galaxies with other extragalactic sources within a projected distance of up to 340 kpc; c total integration time spent on the source; d 1 - Holmberg I; 2 - UGC 2345; 3 - Sextans B; 4 - NGC 4303; e spectral resolution of the spectra shown in Fig. 1.


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