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Table 2.

H I properties of dwarfs measured from the 66″ MFS H I cube.

Name RA (J2000) Dec (J2000) Integrated flux vsys w20 Disturbed
(hms) (dms) (Jy km s−1) (km s−1) (km s−1)
NGC 1437A 03:43:02.42 −36:16:24.2 7.25 ± 0.7 886 128 Y
ESO 358−G015 03:33:07.06 −34:48:21.2 1.50 ± 0.2 1388 133 Y
ESO 358−G016 03:33:09.19 −35:43:05.2 1.26 ± 0.1 1700 131 Y
ESO 358−G060 03:45:12.29 −35:34:15.2 11.99 ± 1.2 803 129 Y
ESO 358−G064 03:46:28.51 −36:54:21.6 5.59 ± 0.7 1465 171 N
FCC 090 03:31:08.28 −36:17:24.4 0.59 ± 0.07 1825 129 N
FCC 102 03:32:10.56 −36:13:10.6 1.19 ± 0.1 1640 83 Y
FCC 120 03:33:34.18 −36:36:20.1 1.08 ± 0.1 846 60 Y
FCC 128 03:34:07.03 −36:27:57.6 0.14 ± 0.02 1543 68 N
FCC 134 03:34:21.70 −34:35:33.0 0.02 ± 0.01 1398 34 N
FCC 207 03:38:19.25 −35:07:44.8 0.0065 ± 0.006 1420 38 N
FCC 248 03:40:43.37 −35:51:38.9 0.010 ± 0.006 1859 15 N
FCC 299 03:44:58.61 −36:53:41.6 0.31 ± 0.04 2100 136 N
FCC 306 03:45:45.38 −36:20:46.0 2.03 ± 0.1 886 176 Y
FCC 323 03:47:37.46 −36:21:48.6 0.43 ± 0.05 1499 67 N
FCC B905 03:33:57.34 −34:36:43.2 0.52 ± 0.06 1248 99 Y
FDS6 100b 03:41:27.84 −35:43:13.1 0.14 ± 0.03 1983 50 N

Notes. The position, integrated flux, and w20 are from the SoFiA catalogue, while vsys is estimated from where 11″ H I iso-velocity intercepts the optical centre. The uncertainty in the integrated flux is a combination of the statistical error and 10% uncertainty in the calibration of the flux scale (Serra et al. 2023).

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