Table 3
Molecular gas mass, star formation efficiency, dust temperature and dust mass, half-light radius and galaxy type of the sample.
| S | M(H2) | SFE | T d | M d | R 1/2 | Type |
| 109M⊙ | L⊙/M⊙ | K | 108M⊙ | kpc | ||
|
|
||||||
| S 1 | 12.3 | 1003. | 58.7 | 1.4 | 1.1a | S2, Q, wi |
| S 2 | < 4.9 | >1205. | 70.1 | 0.3 | 2.9a | wi |
| S 3 | < 4.5 | >713. | 66.5 | 0.2 | 0.5a | |
| S 4 | < 1.1 | >1978. | > 52.0 | < 0.5 | 3.9 | S2, Q, si |
| S 5 | < 5.3 | >2504. | 58.6 | 1.6 | 3.1a | si |
| S 8 | < 5.6 | >674. | 33.4 | 20.7 | 7.3 | S2, Q |
| S 9 | < 4.2 | >1238. | 68.2 | 0.3 | 4.2 | S1 |
| S10 | 5.4 | 597. | 67.7 | 0.2 | 8.5 | S2 |
| S11 | < 7.8 | >1375. | 76.0 | 0.4 | 1.1a | Q, si |
| S12 | 15.4 | 400. | 75.4 | 0.2 | 5.0 | S2 |
| S13 | < 3.4 | >2012. | 58.2 | 0.8 | 2.2a | |
| S14 | 4.9 | 1776. | 49.0 | 3.0 | 0.9a | si |
| S16 | 21.0 | 1016. | 62.4 | 1.8 | 2.9a | Q |
| S18 | < 5.5 | >1624. | 81.0 | 0.2 | 3.4a | |
| S20 | < 4.7 | >1419. | 69.0 | 0.4 | 3.3a | si |
| S21 | < 4.6 | >861. | 56.5 | 0.6 | 6.4 | S2, Q |
| S22 | 8.8 | 541. | 77.2 | 0.2 | 1.5a | S2 |
| S23 | < 4.5 | > 1381. | 72.2 | 0.3 | 3.5 | |
| S25 | < 7.1 | >3536. | 64.2 | 1.8 | 1.3a | S2, si |
| S26 | < 5.9 | >656. | 70.2 | 0.2 | 6.2 | wi |
| S27 | 6.2 | 1070. | 41.3 | 9.4 | 7.9 | |
| S28 | < 5.0 | >1254. | 42.2 | 7.7 | – | |
| S29 | 24.1 | 286. | 65.4 | 0.4 | 1.6a | si |
| S30 | 12.2 | 683. | 71.8 | 0.3 | 1.1a | wi |
| S32 | < 4.2 | >7190. | 74.8 | 0.9 | 4.0 | |
| S34 | 20.7 | 569. | 49.1 | 4.2 | 7.8a | si |
| S35 | 7.4 | 346. | 50.0 | 0.8 | 2.8a | S2, Q, wi |
| S36 | < 8.6 | > 531. | 35.1 | 18.6 | 6.4 | |
| S37 | < 5.6 | > 284. | 34.2 | 7.0 | – | |
| S38 | < 6.7 | > 161. | 30.4 | 9.1 | 2.2 | wi |
| S39 | < 7.8 | >222. | 29.9 | 23.5 | 11. | wi |
| S40 | < 4.6 | >574. | 33.1 | 20.5 | – | |
| S41 | < 5.2 | >265. | 26.3 | 55.6 | – | |
| S42 | 8.9 | 287. | 44.0 | 1.7 | 7.8 | Q,si |
| S43 | 22.0 | 109. | 34.1 | 6.9 | 5.6 | wi |
| S44 | 28.7 | 129. | 31.9 | 21.1 | 5.6 | wi |
| S45 | < 10.9 | >265. | >32.8 | < 14.8 | 4.0 | si |
| S46 | < 6.8 | >343. | >31.3 | < 15.8 | 5.5 | |
| S47 | 19.6 | 112. | >33.1 | < 10.9 | 3.1a | si |
Notes. M(H2) and SFE are defined in Sect. 4.8, Td and Md in Sect. 4.5. R1/2 is defined from red images either from SDSS, or HST for the galaxies with index [a]. The latter images were used to determine the morphological class: wi, si = weak & strong interaction. The nuclear activity type is derived from NED: S1, S2 = Seyfert 1 & 2, Q = QSO.
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