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Table 1.

Journal of observations.

ID RA Dec zSDSS Telescope Transition Beamsize νcont σ40 km s−1 σcont
(arcsec2) (GHz) (mJy beam−1) (mJy beam−1)
(1) (2) (3) (4) (5) (6) (7) (8) (9) (10)
J0209−0005 02:09:50.71 −00:05:06.22 2.849 NOEMA CO(5−4) 4.9 × 2.7 148.7 0.90 0.040
JVLA CO(1−0) 3.1 × 2.3 31.6 0.08 0.005
J0801+5210 08:01:17.82 +52:10:34.94 3.217 NOEMA CO(5−4) 3.8 × 1.9 136.6 1.05 0.100
JVLA CO(1−0) 3.4 × 2.3 30.2 0.16 0.010
J1433+0227 14:33:52.21 +02:27:14.01 4.622 ALMA [CII] 0.44 × 0.34 338.1 0.43 0.051
J1538+0855 15:38:30.49 +08:55:17.42 3.542 ALMA CO(4−3) 1.1 × 0.7 94.3 0.49 0.028
J1549+1245 15:49:38.71 +12:45:09.25 2.386 ALMA CO(4−3) 1.0 × 0.9 141.8 0.10 0.007
J1555+1003 15:55:14.86 +10:03:51.23 3.512 ALMA CO(4−3) 1.0 × 0.7 94.30 0.57 0.028
J1639+2824 16:39:09.11 +28:24:47.16 3.786 ALMA CO(4−3) 0.20 × 0.13 100.4 0.43 0.026
J1701+6412 17:01:00.60 +64:12:09.32 2.724 NOEMA CO(5−4) 4.0 × 2.1 154.7 1.03 0.100
J1015+0020 (*) 10:15:49.00 +00:20:20.03 4.400 ALMA [CII] 0.22 × 0.18 357.3 0.19 0.040

Notes. Columns give the following information: (1) SDSS ID, (2) and (3) Celestial coordinates, (4) Redshift based on SDSS DR12 (Alam et al. 2015), (5) Observation telescope, (6) Observed transition, (7) Angular resolution, (8) Observed continuum frequency, (9) rms sensitivity for a channel width of 40 km s−1, and (10) Continuum rms sensitivity. (*)Presented in Bischetti et al. (2018).

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