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Table C.1

Details of the CO observations.

ID Galaxy name tON rms (50 km s-1) ν0 σ ν S peak
[min] [mJy] [km s-1] [km s-1] [mJy] [Jy km s-1]
(1) (2) (3) (4) (5) (6) (7) (8)
APEX CO(2–1) observations
1 UGC 11631 80 35 –31 ±14 71 ± 14 170 ± 30 30 ± 8
2 UGC 00272 113 26 – – – <7
3 IC 0159 46 40 –12 ±12 67 ± 12 210 ± 30 35 ± 8
4 KUG0200-101 30 41 – – – <11
5 NGC 1234 118 25 –32 ±10 49 ± 10 130 ± 20 16 ±4
6 UGC 06838 41 24 –100 ± 30 190 ± 30 75 ± 11 36 ±8
7 UGC 09359 28 37 – – – <10
8 2MASXJ2235-0845 70 28 0 ± 6 45 ± 6 250 ± 30 28±5
9 NGC 5414 19 72 11 ± 7 47 ± 7 450 ± 60 52 ± 11
10 NGC 5405 14 75 13 ± 3 14 ± 3 610 ± 130 21 ± 7
11 UGC 10005 57 32 11 ± 10 24 ± 10 110 ± 40 6 ± 4
12 MCG+00-25-005 10 70 4 ± 13 71 ± 13 330 ± 50 60 ± 15
13 UGC 02004 14 92 –28 ± 13 90 ± 13 530 ± 60 120 ± 20
14 UGC 02529 36 43 – – – <11
15 MCG+00-29-013 26 51 –8 ± 12 71 ± 12 260 ± 40 47 ± 11
16 UGC 06329 47 33 –20 ± 18 48 ± 18 100 ± 30 12 ± 6
17 UGC 05648 36 43 –10 ± 30 120 ± 30 140 ± 30 42 ± 12
18 IC 0605 28 46 3 ± 14 67 ± 14 210 ± 40 36 ± 10
19 2MASXJ0910+0752 14 58 0 ± 18 80 ± 19 210 ± 40 42 ± 13
20 2MASXJ0939+0624 31 35 0 ± 20 120 ± 20 120 ± 20 34 ± 9
21 2MASXJ0955+0632 30 35 19 ± 18 68 ± 18 130 ± 30 22 ± 7
22 2MASXJ1014+0748 25 37 – – – <10
23 2MASXJ1011+0746 46 34 20 ± 20 100 ± 20 120 ± 20 32 ± 9
24 PGC 031905 13 55 –14 ± 9 30 ± 11 240 ± 70 18 ± 8
25 PGC 031382 17 49 – – – <13
26 2MASXJ1110+0411 47 33 – – – <9
27 2MASXJ0855+0345 45 41 140 ± 30 110 ± 30 100 ± 20 27 ± 10
28 2MASXJ0839+0349 12 71 20 ± 30 90 ± 30 190 ± 50 45 ± 17
29 UGC 04977 50 29 –14 ± 16 98 ± 16 138 ± 19 34 ± 7
30 2MASXJ0846+0230 19 46 –12 ± 10 37 ± 9 230 ± 50 21 ± 7
31 SDSSJ1328-0202 23 47 –28 ± 17 51 ± 17 150 ± 40 19 ± 8
32 MCG+00-34-038 9 65 16 ± 13 81 ± 13 350 ± 50 70 ± 15
33 UGC 08526 22 42 –4 ± 10 63 ± 10 250 ± 30 40 ± 8
34 CGCG017-017 55 33 34 ± 14 84 ± 14 170 ± 20 35 ± 8
35 NGC 2936 (narrow) 11 72 216 ± 4 34 ± 4 810 ± 80 69 ± 11
NGC 2936 (broad) 102 ± 15 193 ± 12 580 ± 40 280 ± 30
36 SDSSJ0937+0927 51 30 – – – <8
37 SDSSJ0950+1118 83 31 – – – <8
38 IC3069 41 25 – – – <7
39 SDSSJ1112+0931 42 30 – – – <8
40 SDSSJ0805+0659 66 25 – – – <7
41 SDSSJ1104+0507 51 34 – – – <9
42 CGCG050-042 72 30 – – – <8
43 2MASXJ0858+0345 43 27 4 ± 14 66 ± 14 120 ± 20 20 ± 6
44 SDSSJ1008+1428 26 43 – – – <11
45 SDSSJ0954+0458 34 26 – – – <7
46 SDSSJ1213+1056 30 48 – – – <13
47 SDSSJ0945+0515 22 30 – – – <8
48 SDSSJ1122+1316 25 37 – – – <10
49 SDSSJ1403+1003 51 30 – – – <8
50 CGCG063-006 54 31 – – – <8
51 2MASXJ0843+1303 65 22 – – – <6
52 SDSSJ0920+0759 80 29 – – – <8
53 CGCG080-042 51 37 – – – <10
54 CGCG078-021 42 25 – – – <7
55 UGC 04567 29 33 10 ± 40 100 ± 40 70 ± 20 16 ± 8
56 SDSSJ1624+1251 25 30 –60 ± 50 100 ± 50 50 ± 20 12 ± 8
57 CGCG058-066 71 27 9 ± 16 60 ± 16 100 ± 20 15 ± 5
58 CGCG061-003 93 29 – – – <8
59 CGCG051-037 109 34 – – – <9
60 SDSSJ0854+0418 62 25 –1 ± 13 32 ± 9 100 ± 20 8 ± 3
61 CGCG059-031 21 59 – – – <16
62 2MASXJ0806+1249 68 30 0 ± 5 11 ± 5 150 ± 60 4 ± 3
63 VIIIZW039 66 26 –13 ± 7 43 ± 7 180 ± 30 20 ± 4
64 2MASXJ0941+1056 46 33 21 ± 13 31 ± 13 110 ± 40 9 ± 5
65 SDSSJ0943+0356 25 38 – – – <10
66 CGCG035-063 84 47 – – – <13
67 CGCG036-048 95 32 – – – <9
68 SDSSJ1625+1142 61 51 – – – <14
69 SDSSJ1028+0424 31 32 – – – <9
70 UGC 06011 54 29 – – – <8
71 PGC 051743 20 49 18 ± 7 38 ± 7 350 ± 60 33 ± 9
72 2MASXJ1437+0500 22 43 –40 ± 20 80 ± 20 80 ± 20 17 ± 6
73 SDSSJ0944+0400 37 32 24 ± 9 16 ± 6 130 ± 40 5 ± 3
74 2MASXJ1048+1201 31 32 – – – <9
75 SDSSJ1110+1345 41 29 – – – <8
76 PGC 012214 38 30 – – – <8
77 PGC 003530 45 34 – – – <9
78 PGC 073268 118 27 60 ± 30 70 ± 30 70 ± 20 12 ± 6
79 PGC 1452135 77 30 – – – <8
80 PGC 3127469 67 36 – – – <10
81 UGC 00317 81 30 3 ± 17 31 ± 12 90 ± 30 7 ± 4
82 SDSSJ0011+1428 33 35 – – – <9
83 PGC 1455779 68 23 – – – <6
84 PGC 000010 20 62 0 ± 6 25 ± 6 380 ± 80 24 ± 8
85 PGC 1446233 41 34 –16 ± 19 51 ± 19 100 ± 30 13 ± 6
86 2MASXJ0020+1413 87 29 –8 ± 7 25 ± 7 180 ± 40 11 ± 4
87 PGC 1464874 74 31 – – – <8
88 IC 1706 12 87 –38 ± 17 33 ± 15 210 ± 80 17 ± 11
IRAM CO(1–0) observations
89 SDSSJ0944+1116 72 3.3 – – – <0.6
90 SDSSJ1049+1108 90 3.2 – – – <0.6
91 2MASXJ1336+1552 39 5.5 66 ± 8 33 ± 8 32 ± 7 2.6 ± 0.8
92 SDSSJ1032+1227 72 3.9 – – – <0.7
93 SDSSJ1100+1207 75 3.6 – – – <0.7
94 SDSSJ1207+1200 73 3.9 – – – <0.7
95 KUG1147+149 84 3.9 – – – <0.7
96 SDSSJ1320+1524 83 5.2 – – – <1.0
97 VPC0873 72 3.3 – – – <0.6
IRAM CO(2–1) observations
91 2MASXJ1336+1552 39 11.4 68 ± 8 36 ± 8 62 ± 12 5.6 ± 1.7

Notes. Column (1): ALLSMOG ID. Column (2): galaxy name. Column (3): on-source time. For the IRAM 30 m CO(1–0) observations the “human” on source time is half the value listed in the table, because the EMIR receiver allows simultaneous dual-polarisation observations that were averaged together to produce the final spectrum. Column (4): 1σ spectral rms calculated in channels of δν = 50 km s-1. Column (5): central velocity of the CO emission line with respect to the optical redshift (inferred from SDSS observations) as derived through a single-Gaussian fitting. Column (6): velocity dispersion of the observed CO line derived through a single-Gaussian fitting. Column (7): amplitude of the Gaussian function fitted to the observed CO line profile. Column (8): total velocity-integrated flux of the Gaussian function fitted to the observed CO line profile. For the non-detections, we list the 3σ-upper limit on the total integrated CO flux derived using Eq. (3).

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