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Table A.1

Properties of serendipitous sources.

LBQS0109-A LBQS0109-B LBQS0109-C HB8903-A HB8903-B 2QZJ0028-A

RA 01:12:17.08 01:12:17.49 01:12:17:23 3:31:06.77 3:31:06.09 00:28:31.812
Dec 2:29:32.99 2:29:52.26 2:29:63.64 –38:24:02.79 –38:24:20.95 –28.16.51.616
S3 mm [μJy] 115 ± 12 52 ± 12 48 ± 12 36 ± 18 54 ± 18 61 ± 12
Mdust [108M]a 4–6 1–3 1–3 1–2 2–3 2–3
SFR [M yr-1]a 2800 1200 1100 900 1400 1500
λCO(3 − 2) [mm] 2.90642 ± 0.00008 2.9112 ± 0.0003 2.9045 ± 0.0003 2.9779 ± 0.0006 2.9843 ± 0.0005
FWHMCO(3−2) [km s-1] 190 ± 20 590 ± 70 300 ± 20 400 ± 100 400 ± 100
SCO(3 − 2)Δv [Jy km s-1] 1.72 ± 0.06 7.16 ± 0.05 0.19 ± 0.05 0.27 ± 0.03 0.32 ± 0.04
[1010 K km s-1 pc2] 5.2 ± 0.2 22.9 ± 0.2 0.58 ± 0.15 0.88 ± 0.09 1.04 ± 0.13
LCO(3 − 2) [107L] 6.9 ± 0.2 29.1 ± 0.2 0.8 ± 0.2 1.26 ± 0.13 1.38 ± 0.17
MCO(αCO = 0.8) [1010M]b 4 ± 2 18 ± 9 0.5 ± 0.3 0.7 ± 0.4 0.8 ± 0.5
MCO(αCO = 4) [1010M]b 21 ± 11 90 ± 50 2.3 ± 1.7 3 ± 2 4 ± 2

Notes.

(a)

Under the assumption that the continuum emission at 3 mm is completely associated to thermal dust continuum emission. We assume a Td = 40 − 60 K and a β = 2.0.

(b)

Under the assumption that the line detection is associated to the CO(32) transition and assuming a r31 = 1.0 ± 0.5. The statistical errors associated to the molecular gas include r31 uncertainties.

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