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Table C.1.

SMG sample.

Target RA & Dec (J2000) z Jup rJup, 1 LCO (1010 K km s−1 pc2) Mgas (1010 M) log(Mstar) (M) log(LIR) (L) ref
(1) (2) (3) (4) (5) (6) (7) (8) (9) (10)
SGP-196076 00:03:07 −33:02:50 4.425 4 0.41 38.83 ± 3.8 31.1 ± 3.0∘ 13.44 F17
SMMJ021725 02:17:25 −04:59:34 2.292 4 0.41 4.7±0.5 4.7 ± 0.5 12.67 Bo13
SMMJ021738-050339 02:17:38 −05:03:39 2.037 4 0.41 11.0±3.1 11.0±3.1 12.67 Bo13
SMMJ021738-050528 02:17:38 −05:05:28 2.541 4 0.41 9.4±2.9 9.4±2.9 12.66 Bo13
ADFS-27 04:36:57 −54:38:10 5.655 5 0.32 35.9 ± 2.1 28.7 ± 1.7∘ 13.46 F17
SMMJ044315 04:43:07 +02:10:23 2.509 3 0.52 12.1±3.5 12.1±3.5 12.50 Bo13
J044307+0210 04:43:05+02:09:06 2.509 1 1.00 1.48 ± 0.40 1.18 ± 0.32∘ 12.17 ± 0.10 S16
J04135+10277 04:13:27 +10:27:43 2.846 1 1.00 8.4 ± 1.7 6.7 ± 1.4∘ 13.24 ± 0.05 S16
G09-81106 08:49:36 +00:14:54 4.531 4 0.41 15.3 ± 2.5 12.2 ± 2∘ 13.39 F17
SMMJ094303 09:43:03 +47:00:15 3.346 4 0.41 7.1±1.6 7.1±1.6 13.25 Bo13
PACS867 09:59:38 +02:28:56 1.566 2 0.85 2.03 ± 0.16 2.23 ± 0.18 10.67 12.62 ± 0.04 S15
PACS299 09:59:41 +02:14:42 1.645 2 0.85 3.21 ± 0.35 3.53 ± 0.38 10.44 12.81 ± 0.03 S15
PACS819 09:59:55 +02:15:11 1.445 2 0.85 4.15 ± 0.23 2.49 ± 1.2 10.61 12.96 ± 0.01 S15
PACS282 10:00:01 +02:11:24 2.187 3 0.70 3.20 ± 0.46 3.52 ± 0.51 10.88 12.83 ± 0.03 S15
PACS325 10:00:05 +02:19:42 1.656 2 0.85 1.67 ± 0.26 1.84 ± 0.28 10.29 12.21 ± 0.03 S15
PACS830 10:00:08 +02:19:01 1.463 2 0.85 4.55 ± 0.35 7.3 ± 2.2 10.86 12.78 ± 0.01 S15
AzTEC-3 10:00:20 +02:35:22 5.299 2 sled 7.6 6.1∘ 13.1 F17
PACS164 10:01:30 +01:54:12 1.648 2 0.85 2.93 ± 0.47 3.22 ± 0.50 > 10.28 12.62 ± 0.01 S15
SMMJ105141 10:51:41 57:19:52 1.214 2 0.84 6.55 ± 0.52 6.55 ± 0.52 12.69 Bo13
SMMJ105151 10:51:51 +57:26:35 1.597 2 0.84 2.64 ± 1.45 2.64 ± 1.45 11.16 12.54 Bo13
SMMJ105227 10:52:27 +57:25:16 2.443 3 0.52 2.87 ± 0.61 2.87 ± 0.61 11.24 12.82 Bo13
SMMJ105307 10:53:07 +57:24:31 1.524 2 0.84 2.21 ± 0.31 2.21 ± 0.31 12.21 Bo13
SMMJ123549 12:35:49 +62:15:37 2.202 3 0.52 8.99 ± 0.72 8.99 ± 0.71 11.20 12.71 Bo13
SMMJ123555 12:35:55 +62:09:02 1.864 2 0.84 4.67 ± 1.54 4.67 ± 1.54 11.11 13.0 Bo13
SMMJ123634 12:36:34 +62:12:41 1.225 2 0.84 3.95 ± 0.42 3.95 ± 0.42 10.82 12.61 Bo13
GN 20 12:37:11 +62:22:11 4.055 2 1.0 18.7 ± 5.2 15.0 ± 4.2∘ 11.36 13.52 F17
SMMJ123712 12:37:12 +62:13:26 1.996 3 0.52 5.4 ± 1.4 5.4±1.4 11.19 12.46 Bo13
SMMJ131201 13:12:01 +42:42:08 3.408 4 0.41 14.95 ± 3.8 14.95 ± 3.8 10.96 12.96 Bo13
NGP-284357 13:32:51 +33:23:42 4.894 6 0.21 30.2 ± 6.1 24.2 ± 4.9∘ 13.14 F17
NGP-246114 13:41:14 +33:59:38 3.847 4 0.41 14.3 ± 1.8 11.4 ± 1.4∘ 13.21 F17
SMMJ163658+405728 16:36:50 +40:57:34 1.193 2 0.84 2.2 ± 0.4 2.2 ± 0.4 10.89 12.09 Bo13
SMMJ163658+410523 16:36:58 +41:05:24 2.454 3 0.52 9.5±1.0 9.5±1.0 11.01 12.90 Bo13
MIPS506 17:11:38 +58:38:36 2.470 3 1.0 1.61 ± 0.34 1.29 ± 0.28∘ 12.92 Y10
MIPS16144 17:24:21 +59:31:51 2.131 3 1.0 4.05 ± 0.95 3.24 ± 0.74∘ 12.75 Y10
SMMJ221804 22:18:04 +00:21:54 2.517 3 0.52 9.96±1.12 9.96±1.12 10.79 12.53 Bo13
J22174+0015 22:17:34 +00:15:33 3.099 1 1.00 4.3 ± 1.0 4.3 ± 1.0 10.51 12.66 ± 0.11 S16
Lensed galaxies

J083051.0+013224 08:30:51 +01:32:24 3.634 3 0.17 10.0 ± 4.4 8.0 ± 3.5∘ 13.11 ± 0.12 Y17
J085358.9+015537 08:53:58 +01:55:37 2.092 2 0.84 2.3 ± 0.9 1.8 ± 0.7∘ 12.39 ± 0.19 Y17
J090302.9-014127 09:03:03 −01:41:27 2.304 3 0.17 7.8 ± 2.1 6.2 ± 1.67∘ 12.92 ± 0.17 Y17
J090311.6+003906 09:03:11 +00:39:06 3.042 3 0.17 5.7 ± 1.5 46 ± 1.2∘ 12.48 ± 0.12 Y17
J114637.9−001132 11:46:37 −00:11:31 3.259 4 0.41 8.3 ± 2.4 6.6 ± 1.9∘ 12.97 ± 0.12 Y17
HDF 850.1 12:36:51 +62:12:25 5.183 2 sled 4.6 3.7∘ 12.83 F17
J125632.7+233625 12:56:32 +23:36:27 3.565 3 0.17 5.7 ± 1.5 4.6 ± 1.2∘ 12.82 ± 0.15 Y17
J133008.4+245900 13:30:08 +24:58:59 3.111 5 0.32 2.4 ± 0.6 1.9 ± 0.5∘ 12.68 ± 0.16 Y17
J133649.9+291801 13:36:49 +29:18:01 2.202 3 0.17 5.8 ± 1.6 4.6 ± 1.3∘ 12.89 ± 0.26 Y17
J134429.4+303036 13:44:29 +30:30:34 2.301 5 0.32 5.5 ± 1.1 4.4 ± 0.9∘ 12.75 ± 0.12 Y17
J141351.9−000026 14:13:51 −00:00:26 2.478 3 0.17 28.8 ± 7.6 23.0 ± 6.8∘ 12.95 ± 0.13 Y17
G15v2.779 14:24:13 +02:23:04 4.243 4 0.41 18.0 ± 4.3 14.4 ± 3.4∘ 13.10 ± 0.14 Y17
HFLS3 17:06:47 +58:46:23 6.337 1 1.0 9.49 ± 3.13 9.49 ± 3.13 10.57 13.45 ± 0.05 F17

Notes. Column (1): target name; Column (2): coordinates; Column (3): redshift; Column (4): Jup refers to the upper level of the (JupJup − 1) CO transition; Column (5): the excitation correction defined as rJup, 1 = CO(JupJup − 1)/CO(1 → 0); Column (6): CO(1-0) luminosity; Column (7): gas mass; Column (8): stellar mass; Column (9): 8–1000 μm IR luminosity; Column (10): reference for the paper from which we derived CO and far-IR measurements, as well as assumed excitation correction and αCO conversion factors. All lensed galaxy properties are corrected for magnification. The three lensed galaxies from Fudamoto et al. (2017), SGP-261206, NGP- 190387, and G09-83808, are not included in our sample as their magnification factors are unknown. The S15 and Y17 infrared luminosities are derived from SFR, using the following prescription: LIR= SFR ×1010L (Kennicutt 1998, correcting for a Chabrier IMF). The luminosity-to-gas-mass conversion factors used to derive the gas mass in the different papers are indicated in the table as follows: : αCO = 1.0; ∘: αCO = 0.8; : αCO = 1.1; : the gas masses are derived from a CO-based dynamical mass estimate by subtracting stellar and dark matter components (Silverman et al. 2015). The inferred Mgas yielded the estimate of αCO = 0.6 ± 0.3 (PACS819) and αCO = 1.6 ± 0.6 (PACS830).

References. Bothwell et al. (2013, Bo13); Fudamoto et al. (2017, F17); Sharon et al. (2016, S16); Silverman et al. (2015, S15); Yan et al. (2010, Y10); Yang et al. (2017, Y17).

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