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Table 2.

Measurements for our sample galaxies.

ID RA Dec zCO vCO Δv LCO Fcont Line
(deg) (deg) (Jy km s−1) km s−1 (108 K km s−1 pc2) (mJy)
(1) (2) (3) (4) (5) (6) (7) (8) (9)
J1448 222.191344 10.169614 0.6463 ± 0.0001 0.55 ± 0.08 390 ± 52 32.6 ± 4.8 < 11.9 CO(2–1)
0.6460 ± 0.0001 1.57 ± 0.27 307 ± 46 23.0 ± 4.0 < 58.1 CO(4–3)
0.6465 ± 0.0002 2.62 ± 0.54 591 ± 93 24.7 ± 5.1 < 257.2 CO(5–4)
J2258 344.523653 23.221175 0.7056 ± 0.0001 1.40 ± 0.18 220 ± 24 98.1 ± 1.2 12.3 CO(2–1)
0.7043 ± 0.0005 2.38 ± 0.75 836 ± 207 26.7 ± 8.4 < 303.1 CO(5–4)
ID83492 34.546956 −5.147125 1.1394 ± 0.0005 0.23 ± 0.09 569 ± 162 18.8 ± 7.1 < 31.9 CO(3–2)
1.1398 ± 0.0001 0.16 ± 0.05 129 ± 34 4.6 ± 1.6 < 49.7 CO(5–4)
J1109 167.384124 −0.667679 0.5937 ± 0.0001 0.64 ± 0.06 328 ± 21 31.8 ± 2.8 < 1493.8 CO(2–1)
< 0.33 < 2.6 < 156.7 CO(5–4)
J1302 195.703844 10.717528 0.5922 ± 0.0002 0.53 ± 0.08 732 ± 79 26.3 ± 3.8 < 21.8 CO(2–1)
< 0.53 < 4.2 < 210.0 CO(5–4)
J0912 138.178105 15.384847 0.7472 ± 0.0001 1.01 ± 0.07 367 ± 19 79.4 ± 5.5 < 257.2 CO(2–1)
0.7474 ± 0.0001 0.53 ± 0.11 296 ± 49 10.5 ± 2.3 < 40.8 CO(4–3)
< 0.31 < 3.9 < 165.7 CO(5–4)
J2202 330.601428 −0.559743 0.6582 ± 0.0001 0.24 ± 0.08 181 ± 44 14.6 ± 4.7 < 38.1 CO(2–1)
< 2.24 < 21.9 < 84.2 CO(5–4)
ID97148 34.333142 −5.084108 1.2727 ± 0.0002 0.09 ± 0.05 160 ± 64 9.2 ± 4.9 < 28.6 CO(3–2)
< 0.03 < 1.0 < 37.1 CO(5–4)

C1-83492* 34.547551 −5.148568 1.1374 ± 0.0002 0.79 ± 0.10 590 ± 57 71.5 ± 9.1 86.8 ± 20.1 CO(3–2)
1.1377 ± 0.0002 0.43 ± 0.08 388 ± 57 12.4 ± 2.4 510.4 ± 23.7 CO(5–4)
C2-83492* 34.550126 −5.149099 1.1379 ± 0.0001 0.89 ± 0.11 432 ± 41 63.9 ± 8.3 116.8 ± 20.6 CO(3–2)
1.1380 ± 0.0004 0.30 ± 0.10 471 ± 119 8.6 ± 2.9 318.2 ± 37.2 CO(5–4)

Notes. Columns: (1) Galaxy ID; (2) Right ascension of the galaxy center; (3) Declination of the galaxy center; (4) Redshift estimated by fitting the emission line with a Gaussian in our 1D ALMA spectra. The uncertainty that we report is the formal error obtained from the fit; (5) CO integrated flux density. Upper limits are 3σ; (6) Line velocity width; (7) CO brightness temperature. Upper limits are 3σ; (8) Flux of the continuum underlying the line. Upper limits are 3σ; (9) CO transition. * Indicate star-forming companions of ID83492.

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