Table C.5
HI gas masses.
ID | Galaxy name | log MHI |
![]() |
Telescope | Reference |
[M⊙] | [M⊙] | ||||
(1) | (2) | (3) | (4) | (5) | (6) |
|
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APEX targets | |||||
|
|||||
1 | UGC 11631 | 9.70 ± 0.02 | 9.78 ± 0.02 | GBT | Masters et al. (2014) |
2 | UGC 00272 | 9.83 ± 0.05 | 9.95 ± 0.05 | Arecibo | Springob et al. (2005) |
3 | IC 0159 | 9.53 ± 0.07 | 9.56 ± 0.07 | Nançay | Theureau et al. (2005) |
4 | KUG0200-101 | 10.07 ± 0.04 | 10.11 ± 0.04 | Parkes | Barnes et al. (2001) † |
5 | NGC 1234 | 9.74 ± 0.05 | 9.77 ± 0.05 | Nançay | Theureau et al. (2005) |
6 | UGC 06838 | 9.55 ± 0.09 | 9.59 ± 0.09 | Nançay | Theureau et al. (2005) |
7 | UGC 09359 | 9.68 ± 0.07 | 9.80 ± 0.07 | Arecibo | Springob et al. (2005) |
8 | 2MASXJ2235-0845 | 9.78 ± 0.15 | 9.79 ± 0.15 | Nançay | Theureau et al. (2005) |
9 | NGC 5414 | 9.832 ± 0.005 | 9.843 ± 0.005 | Arecibo | Haynes et al. (2011) |
10 | NGC 5405 | 10.096 ± 0.007 | 10.096 ± 0.007 | Arecibo | Haynes et al. (2011) |
11 | UGC 10005 | 9.70 ± 0.06 | 9.70 ± 0.06 | NRAO 91m | Hewitt et al. (1983) |
12 | MCG+00-25-005 | 9.80 ± 0.13 | 9.82 ± 0.13 | Parkes | Barnes et al. (2001) † |
13 | UGC 02004 | 9.93 ± 0.05 | 9.96 ± 0.05 | Arecibo | Springob et al. (2005) |
14 | UGC 02529 | 10.01 ± 0.11 | 10.07 ± 0.11 | Parkes | Barnes et al. (2001) † |
15 | MCG+00-29-013 | ≤9.69 | ≤9.69 | Parkes | Barnes et al. (2001) † |
16 | UGC 06329 | 10.15 ± 0.05 | 10.16 ± 0.05 | Arecibo | Lewis (1987) |
17 | UGC 05648 | 10.131 ± 0.009 | 10.181 ± 0.008 | Arecibo | Haynes et al. (2011) |
18 | IC 0605 | 10.00 ± 0.07 | 10.01 ± 0.07 | Arecibo | Paturel et al. (2003) |
19 | 2MASXJ0910+0752 | ≤ 9.06 | ≤9.06 | Arecibo | Haynes et al. (2011) † |
20 | 2MASXJ0939+0624 | 9.80 ± 0.02 | 9.83 ± 0.02 | Arecibo | Haynes et al. (2011) |
21 | 2MASXJ0955+0632 | ≤8.91 | ≤8.91 | Arecibo | Haynes et al. (2011) † |
22 | 2MASXJ1014+0748 | 9.73 ± 0.02 | 9.77 ± 0.02 | Arecibo | Haynes et al. (2011) |
23 | 2MASXJ1011+0746 | 9.82 ± 0.02 | 9.88 ± 0.02 | Arecibo | Haynes et al. (2011) |
24 | PGC 031905 | 9.619 ± 0.013 | 9.631 ± 0.012 | Arecibo | Haynes et al. (2011) |
25 | PGC 031382 | 9.94 ± 0.02 | 9.98 ± 0.02 | Arecibo | Haynes et al. (2011) |
26 | 2MASXJ1110+0411 | 9.72 ± 0.03 | 9.75 ± 0.18 | Arecibo | Haynes et al. (2011) |
27 | 2MASXJ0855+0345 | ≤9.87 | ≤9.92 | Parkes | Barnes et al. (2001) † |
28 | 2MASXJ0839+0349 | ≤9.92 | ≤9.94 | Parkes | Barnes et al. (2001) † |
29 | UGC 04977 | ≤9.84 | ≤9.88 | Parkes | Barnes et al. (2001) † |
30 | 2MASXJ0846+0230 | 10.16 ± 0.15 | 10.16 ± 0.15 | Parkes | Barnes et al. (2001) † |
31 | SDSSJ1328-0202 | 9.35 ± 0.13 | 9.37 ± 0.12 | Parkes | Barnes et al. (2001) † |
32 | MCG+00-34-038 | 9.98 ± 0.12 | 10.00 ± 0.12 | Nançay | Theureau et al. (2005) |
33 | UGC 08526 | 9.86 ± 0.09 | 9.88 ± 0.09 | Parkes | Barnes et al. (2001) † |
34 | CGCG017-017 | 9.86 ± 0.05 | 9.94 ± 0.06 | Nançay | Springob et al. (2005) |
35 | NGC 2936 | ≤9.95 | ≤10.04 | Parkes | Barnes et al. (2001) † |
36 | SDSSJ0937+0927 | 9.784 ± 0.012 | 9.831 ± 0.012 | Arecibo | Haynes et al. (2011) |
37 | SDSSJ0950+1118 | 8.79 ± 0.06 | 8.79 ± 0.06 | Arecibo | Haynes et al. (2011) |
38 | IC3069 | 9.32 ± 0.03 | 9.37 ± 0.03 | Arecibo | Haynes et al. (2011) |
39 | SDSSJ1112+0931 | 9.35 ± 0.02 | 9.37 ± 0.02 | Arecibo | Haynes et al. (2011) |
40 | SDSSJ0805+0659 | 9.18 ± 0.02 | 9.20 ± 0.02 | Arecibo | Haynes et al. (2011) |
41 | SDSSJ1104+0507 | 8.93 ± 0.04 | 8.95 ± 0.04 | Arecibo | Haynes et al. (2011) |
42 | CGCG050-042 | 9.03 ± 0.02 | 9.04 ± 0.02 | Arecibo | Haynes et al. (2011) |
43 | 2MASXJ0858+0345 | ≤9.78 | ≤9.79 | Parkes | Barnes et al. (2001) † |
44 | SDSSJ1008+1428 | 9.33 ± 0.03 | 9.37 ± 0.03 | Arecibo | Haynes et al. (2011) |
45 | SDSSJ0954+0458 | 8.79 ± 0.06 | 8.81 ± 0.06 | Arecibo | Haynes et al. (2011) |
46 | SDSSJ1213+1056 | 8.91 ± 0.07 | 8.92 ± 0.07 | Arecibo | Haynes et al. (2011) |
47 | SDSSJ0945+0515 | 8.99 ± 0.05 | 9.00 ± 0.05 | Arecibo | Haynes et al. (2011) |
48 | SDSSJ1122+1316 | 9.02 ± 0.04 | 9.03 ± 0.04 | Arecibo | Haynes et al. (2011) |
49 | SDSSJ1403+1003 | 8.70 ± 0.04 | 8.74 ± 0.04 | Arecibo | Haynes et al. (2011) |
50 | CGCG063-006 | 9.517 ± 0.011 | 9.540 ± 0.010 | Arecibo | Haynes et al. (2011) |
51 | 2MASXJ0843+1303 | 8.83 ± 0.03 | 8.84 ± 0.03 | Arecibo | Haynes et al. (2011) |
52 | SDSSJ0920+0759 | 9.05 ± 0.04 | 9.09 ± 0.04 | Arecibo | Haynes et al. (2011) |
53 | CGCG080-042 | 9.49 ± 0.02 | 9.59 ± 0.02 | Arecibo | Haynes et al. (2011) |
54 | CGCG078-021 | 9.35 ± 0.03 | 9.38 ± 0.03 | Arecibo | Haynes et al. (2011) |
55 | UGC 04567 | 9.591 ± 0.009 | 9.669 ± 0.009 | Arecibo | Haynes et al. (2011) |
56 | SDSSJ1624+1251 | 9.43 ± 0.02 | 9.46 ± 0.02 | Arecibo | Haynes et al. (2011) |
57 | CGCG058-066 | 9.38 ± 0.02 | 9.40 ± 0.02 | Arecibo | Haynes et al. (2011) |
58 | CGCG061-003 | 9.35 ± 0.02 | 9.43 ± 0.02 | Arecibo | Haynes et al. (2011) |
59 | CGCG051-037 | 9.36 ± 0.02 | 9.39 ± 0.02 | Arecibo | Haynes et al. (2011) |
60 | SDSSJ0854+0418 | 9.42 ± 0.03 | 9.45 ± 0.03 | Arecibo | Haynes et al. (2011) |
61 | CGCG059-031 | 9.13 ± 0.04 | 9.19 ± 0.04 | Arecibo | Haynes et al. (2011) |
62 | 2MASXJ0806+1249 | 9.05 ± 0.03 | 9.07 ± 0.03 | Arecibo | Haynes et al. (2011) |
63 | VIIIZW039 | 8.92 ± 0.07 | 8.93 ± 0.06 | Arecibo | Haynes et al. (2011) |
64 | 2MASXJ0941+1056 | 9.39 ± 0.02 | 9.39 ± 0.02 | Arecibo | Haynes et al. (2011) |
65 | SDSSJ0943+0356 | 9.35 ± 0.03 | 9.37 ± 0.03 | Arecibo | Haynes et al. (2011) |
66 | CGCG035-063 | 9.676 ± 0.014 | 9.681 ± 0.014 | Arecibo | Haynes et al. (2011) |
67 | CGCG036-048 | 9.10 ± 0.02 | 9.10 ± 0.02 | Arecibo | Haynes et al. (2011) |
68 | SDSSJ1625+1142 | 9.01 ± 0.04 | 9.07 ± 0.04 | Arecibo | Haynes et al. (2011) |
69 | SDSSJ1028+0424 | 9.55 ± 0.02 | 9.60 ± 0.02 | Arecibo | Haynes et al. (2011) |
70 | UGC 06011 | 9.99 ± 0.11 | 10.03 ± 0.11 | Parkes | Barnes et al. (2001) † |
71 | PGC 051743 | 9.44 ± 0.03 | 9.45 ± 0.03 | Arecibo | Haynes et al. (2011) |
72 | 2MASXJ1437+0500 | 9.69 ± 0.02 | 9.74 ± 0.02 | Arecibo | Haynes et al. (2011) |
73 | SDSSJ0944+0400 | 9.55 ± 0.02 | 9.58 ± 0.02 | Arecibo | Haynes et al. (2011) |
74 | 2MASXJ1048+1201 | 9.24 ± 0.03 | 9.27 ± 0.03 | Arecibo | Haynes et al. (2011) |
75 | SDSSJ1110+1345 | ≤9.22 | ≤9.27 | Parkes | Barnes et al. (2001) † |
76 | PGC 012214 | 9.92 ± 0.08 | 9.98 ± 0.08 | Nançay | Paturel et al. (2003) |
77 | PGC 003530 | 9.78 ± 0.10 | 9.80 ± 0.09 | Parkes | Barnes et al. (2001) † |
78 | PGC 073268 | 9.24 ± 0.04 | 9.27 ± 0.04 | Arecibo | Haynes et al. (2011) |
79 | PGC 1452135 | 9.16 ± 0.03 | 9.22 ± 0.03 | Arecibo | Haynes et al. (2011) |
80 | PGC 3127469 | 9.08 ± 0.03 | 9.09 ± 0.03 | Arecibo | Haynes et al. (2011) |
81 | UGC 00317 | 9.2 ± 0.2 | 9.2 ± 0.2 | Parkes | Barnes et al. (2001) † |
82 | SDSSJ0011+1428 | 8.95 ± 0.05 | 8.97 ± 0.05 | Arecibo | Haynes et al. (2011) |
83 | PGC 1455779 | 9.50 ± 0.03 | 9.56 ± 0.03 | Arecibo | Haynes et al. (2011) |
84 | PGC 000010 | 9.7 ± 0.2 | 9.7 ± 0.2 | Parkes | Barnes et al. (2001) † |
85 | PGC 1446233 | 9.30 ± 0.09 | 9.36 ± 0.10 | Arecibo | Haynes et al. (2011) † |
86 | 2MASXJ0020+1413 | 9.05 ± 0.03 | 9.06 ± 0.03 | Arecibo | Haynes et al. (2011) |
87 | PGC 1464874 | 9.633 ± 0.010 | 9.70 ± 0.010 | Arecibo | Haynes et al. (2011) |
88 | IC 1706 | 9.30 ± 0.03 | 9.30 ± 0.03 | Arecibo | Haynes et al. (2011) |
|
|||||
IRAM Targets | |||||
|
|||||
89 | SDSSJ0944+1116 | 9.44 ± 0.04 | 9.46 ± 0.04 | Arecibo | Haynes et al. (2011) |
90 | SDSSJ1049+1108 | 9.49 ± 0.04 | 9.53 ± 0.04 | Arecibo | Haynes et al. (2011) |
91 | 2MASXJ1336+1552 | 9.41 ± 0.03 | 9.42 ± 0.03 | Arecibo | Haynes et al. (2011) |
92 | SDSSJ1032+1227 | ≤9.55 | ≤9.55 | Arecibo | Haynes et al. (2011) † |
93 | SDSSJ1100+1207 | 9.24 ± 0.14 | 9.27 ± 0.14 | Arecibo | Haynes et al. (2011) † |
94 | SDSSJ1207+1200 | 9.50 ± 0.09 | 9.53 ± 0.09 | Arecibo | Haynes et al. (2011) † |
95 | KUG1147+149 | 9.52 ± 0.02 | 9.58 ± 0.02 | Arecibo | Haynes et al. (2011) |
96 | SDSSJ1320+1524 | 8.85 ± 0.18 | 8.87 ± 0.18 | Arecibo | Haynes et al. (2011) † |
97 | VPC0873 | 9.677 ± 0.015 | 9.680 ± 0.015 | Arecibo | Haynes et al. (2011) |
Notes. †For these sources we have re-performed the Hi 21 cm spectral analysis on the original data and used the Hi flux (or upper limit on it) measured by us to calculate MHI (further details in Sect. 4.2). Column (1): ALLSMOG ID. Column (2): galaxy name. Column (3): Hi gas mass computed from the integrated Hi 21 cm emission line flux following Eq. (6). Column (4): Hi gas mass corrected for self-absorption as explained in Sect. 4.2. Column (5): radio telescope used for the Hi 21 cm observations. Column (6): reference for the Hi 21 cm observations used in this work.
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