The MeerKAT Fornax Survey - VI. The collapse of the galaxy H I Mass Function in Fornax

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Table A.2.

Detected H I clouds with their position and nearest cluster galaxy.

Nearest galaxy	RA (J2000)	Dec (J2000)	log(M_HI/M_⊙)	v_sys	w₂₀	\|Δv_sys\|
	(hms)	(dms)		(km s⁻¹)	(km s⁻¹)	(km s⁻¹)
(1)	(2)	(3)	(4)	(5)	(6)	(7)
ESO 358-015	03:32:32.2	-34:42:16	6.6 $\begin{matrix} + 0.06 \\ - 0.07 \end{matrix}$ $\substack{+0.06 \\ -0.07}$	1176	64	212 ^(a)
ESO 358-016	03:33:54.9	-35:39:01	6.1 $\begin{matrix} + 0.09 \\ - 0.11 \end{matrix}$ $\substack{+0.09 \\ -0.11}$	1245	38	455 ^(a)
ESO 358-063	03:45:10.6	-34:40:09	6.0 $\begin{matrix} + 0.08 \\ - 0.10 \end{matrix}$ $\substack{+0.08 \\ -0.10}$	1251	27	678 ^(a)
FCC 306	03:45:17.2	-36:32:45	6.4 $\begin{matrix} + 0.07 \\ - 0.08 \end{matrix}$ $\substack{+0.07 \\ -0.08}$	925	49	39 ^(a)
NGC 1351A	03:27:51.8	-35:30:01	6.3 $\begin{matrix} + 0.08 \\ - 0.09 \end{matrix}$ $\substack{+0.08 \\ -0.09}$	1549	40	202 ^(a)
NGC 1399	03:37:52.5	-35:14:15	5.9 $\begin{matrix} + 0.1 \\ - 0.13 \end{matrix}$ $\substack{+0.1 \\ -0.13}$	1701	26	276 ^(b)
NGC 1399	03:38:10.3	-35:16:33	6.2 $\begin{matrix} + 0.09 \\ - 0.11 \end{matrix}$ $\substack{+0.09 \\ -0.11}$	1210	42	215 ^(b)
NGC 1399	03:38:25.3	-35:19:32	6.6 $\begin{matrix} + 0.07 \\ - 0.08 \end{matrix}$ $\substack{+0.07 \\ -0.08}$	1548	50	123 ^(b)
NGC 1427	03:43:48.5	-35:20:38	6.1 $\begin{matrix} + 0.08 \\ - 0.11 \end{matrix}$ $\substack{+0.08 \\ -0.11}$	1575	25	187 ^(a)
NGC 1427A	03:39:42.6	-35:47:45	6.4 $\begin{matrix} + 0.07 \\ - 0.09 \end{matrix}$ $\substack{+0.07 \\ -0.09}$	1769	52	267 ^(a)
NGC 1427A	03:40:04.0	-36:05:52	6.2 $\begin{matrix} + 0.07 \\ - 0.09 \end{matrix}$ $\substack{+0.07 \\ -0.09}$	1943	38	93 ^(a)
NGC 1427A	03:40:56.8	-36:27:10	6.1 $\begin{matrix} + 0.08 \\ - 0.1 \end{matrix}$ $\substack{+0.08 \\ -0.1}$	1811	17	225 ^(a)
NGC 1427A	03:41:02.6	-36:01:50	6.3 $\begin{matrix} + 0.07 \\ - 0.09 \end{matrix}$ $\substack{+0.07 \\ -0.09}$	1776	27	260 ^(a)
NGC 1427A	03:41:35.9	-36:22:59	6.3 $\begin{matrix} + 0.07 \\ - 0.08 \end{matrix}$ $\substack{+0.07 \\ -0.08}$	1791	30	245 ^(a)
NGC 1427A	03:41:37.2	-36:27:01	6.3 $\begin{matrix} + 0.07 \\ - 0.09 \end{matrix}$ $\substack{+0.07 \\ -0.09}$	1773	44	263 ^(a)
NGC 1427A	03:41:52.2	-36:13:56	6.3 $\begin{matrix} + 0.07 \\ - 0.09 \end{matrix}$ $\substack{+0.07 \\ -0.09}$	1801	29	235 ^(a)
NGC 1427A	03:42:05.5	-36:25:32	6.1 $\begin{matrix} + 0.09 \\ - 0.11 \end{matrix}$ $\substack{+0.09 \\ -0.11}$	1772	33	264 ^(a)
NGC 1427A	03:42:13.4	-36:10:56	6.5 $\begin{matrix} + 0.07 \\ - 0.08 \end{matrix}$ $\substack{+0.07 \\ -0.08}$	1772	–	264 ^(a)
NGC 1427A	03:42:15.7	-36:09:39	6.2 $\begin{matrix} + 0.08 \\ - 0.1 \end{matrix}$ $\substack{+0.08 \\ -0.1}$	1772	–	264 ^(a)
NGC 1427A	03:42:19.1	-36:15:35	6.3 $\begin{matrix} + 0.07 \\ - 0.09 \end{matrix}$ $\substack{+0.07 \\ -0.09}$	1804	39	232 ^(a)
NGC 1365	03:34:20.1	-36:11:07	6.4 $\begin{matrix} + 0.06 \\ - 0.08 \end{matrix}$ $\substack{+0.06 \\ -0.08}$	1691	48	55 ^(a)
NGC 1365	03:34:24.9	-36:07:04	7.0 $\begin{matrix} + 0.04 \\ - 0.05 \end{matrix}$ $\substack{+0.04 \\ -0.05}$	1608	34	28 ^(a)
NGC 1365	03:34:25.8	-36:03:46	6.8 $\begin{matrix} + 0.05 \\ - 0.06 \end{matrix}$ $\substack{+0.05 \\ -0.06}$	1597	48	39 ^(a)
NGC 1365	03:34:32.3	-36:15:22	6.4 $\begin{matrix} + 0.07 \\ - 0.08 \end{matrix}$ $\substack{+0.07 \\ -0.08}$	1694	59	58 ^(a)
NGC 1365	03:34:34.3	-36:01:11	6.9 $\begin{matrix} + 0.05 \\ - 0.06 \end{matrix}$ $\substack{+0.05 \\ -0.06}$	1694	–	58 ^(a)
NGC 1365	03:34:37.1	-36:25:40	6.5 $\begin{matrix} + 0.06 \\ - 0.07 \end{matrix}$ $\substack{+0.06 \\ -0.07}$	1516	36	120 ^a)
NGC 1365	03:34:37.3	-36:10:09	6.2 $\begin{matrix} + 0.07 \\ - 0.08 \end{matrix}$ $\substack{+0.07 \\ -0.08}$	1591	32	45 ^(a)
NGC 1365	03:34:43.5	-36:47:30	6.3 $\begin{matrix} + 0.08 \\ - 0.1 \end{matrix}$ $\substack{+0.08 \\ -0.1}$	1591	–	45 ^(a)
NGC 1365	03:34:46.5	-36:00:39	5.7 $\begin{matrix} + 0.11 \\ - 0.14 \end{matrix}$ $\substack{+0.11 \\ -0.14}$	1591	–	45 ^(a)
NGC 1365	03:34:49.9	-36:13:50	5.8 $\begin{matrix} + 0.09 \\ - 0.12 \end{matrix}$ $\substack{+0.09 \\ -0.12}$	1636	21	0 ^(a)
NGC 1365	03:34:54.6	-36:49:50	6.1 $\begin{matrix} + 0.1 \\ - 0.14 \end{matrix}$ $\substack{+0.1 \\ -0.14}$	1777	28	141 ^(a)
NGC 1365	03:34:55.0	-36:01:50	6.3 $\begin{matrix} + 0.07 \\ - 0.09 \end{matrix}$ $\substack{+0.07 \\ -0.09}$	1745	32	109 ^(a)
NGC 1365	03:35:02.3	-36:22:40	6.2 $\begin{matrix} + 0.08 \\ - 0.10 \end{matrix}$ $\substack{+0.08 \\ -0.10}$	1613	62	23 ^(a)
NGC 1365	03:35:03.4	-36:07:44	6.4 $\begin{matrix} + 0.07 \\ - 0.08 \end{matrix}$ $\substack{+0.07 \\ -0.08}$	1599	32	37 ^(a)
NGC 1365	03:35:08.2	-36:25:27	6.2 $\begin{matrix} + 0.07 \\ - 0.08 \end{matrix}$ $\substack{+0.07 \\ -0.08}$	1633	20	3 ^(a)
NGC 1365	03:35:11.3	-36:12:12	6.3 $\begin{matrix} + 0.07 \\ - 0.08 \end{matrix}$ $\substack{+0.07 \\ -0.08}$	1569	39	67 ^(a)
NGC 1365	03:35:12.2	-36:31:28	6.3 $\begin{matrix} + 0.08 \\ - 0.09 \end{matrix}$ $\substack{+0.08 \\ -0.09}$	1629	30	7 ^(a)
NGC 1365	03:35:16.3	-36:34:14	6.8 $\begin{matrix} + 0.05 \\ - 0.06 \end{matrix}$ $\substack{+0.05 \\ -0.06}$	1623	52	13 ^(a)
NGC 1365	03:35:21.0	-36:32:32	6.3 $\begin{matrix} + 0.07 \\ - 0.09 \end{matrix}$ $\substack{+0.07 \\ -0.09}$	1503	43	133 ^(a)
NGC 1365	03:35:23.0	-36:26:55	6.4 $\begin{matrix} + 0.07 \\ - 0.08 \end{matrix}$ $\substack{+0.07 \\ -0.08}$	1596	48	40 ^(a)
NGC 1365	03:35:22.6	-36:34:45	6.2 $\begin{matrix} + 0.08 \\ - 0.11 \end{matrix}$ $\substack{+0.08 \\ -0.11}$	1444	34	192 ^(a)
NGC 1365	03:35:32.7	-36:18:31	6.3 $\begin{matrix} + 0.07 \\ - 0.08 \end{matrix}$ $\substack{+0.07 \\ -0.08}$	1580	27	56 ^(a)
NGC 1365	03:35:37.0	-36:41:37	6.9 $\begin{matrix} + 0.05 \\ - 0.06 \end{matrix}$ $\substack{+0.05 \\ -0.06}$	1503	34	133 ^(a)
NGC 1365	03:36:46.3	-36:33:49	6.3 $\begin{matrix} + 0.08 \\ - 0.10 \end{matrix}$ $\substack{+0.08 \\ -0.10}$	1563	34	73 ^(a)

Notes. (1) Name of nearest galaxy with a measured redshift. (2) Right ascension. (3) Dec. (4) M_HI and its uncertainty, as measured from the 41″ resolution image. (5) Systemic velocity measured in the optical definition. (6) Width of the H I profile at 20% of the peak flux. Those without a w₂₀ were not able to be determined by the SoFiA fitting procedure. (7) Velocity difference between the systemic velocities of the clouds and the nearest galaxy with a spectroscopic redshift. The superscript ^(a) denotes a velocity difference calculated from two (cloud and galaxy) MFS detections, and the superscript ^(b) is from a MFS (cloud) and optical (galaxy) cz difference.

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