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Table 3.

Line and continuum detections.

Target zCO(2 − 1) SCO(2 − 1)Δv FWHMCO (×109) S1.3 mm
[Jy km s−1] [km s−1] [K km s−1 pc−2] [K km s−1 pc−2] [mJy]
J1524+4409 1.2113 ± 0.0001 0.28 ± 0.01 64 ± 4 5.77 ± 0.22 6.71 ± 0.26 0.011 ± 0.006
B1608+656 ( * ) < 0.01 < 0.3 < 0.4 1.7 ± 0.06
J1330+1810 1.3943 ± 0.0002 0.08 ± 0.01 214 ± 12 2.26 ± 0.15 2.63 ± 0.17 0.002 ± 0.001
J1455+1447 1.4265 ± 0.0005 0.05 ± 0.01 224 ± 31 4.54 ± 0.31 1.74 ±0.37 < 0.04
J1633+3134 ( * ) 1.5229 ± 0.0003 0.06 ± 0.01 408 ± 37 1.93 ± 0.90 2.24 ± 1.16 0.006 ± 0.002
J0924+0219 1.5249 ± 0.0003 0.14 ± 0.01 216 ± 12 4.53 ± 0.31 5.27 ± 0.36 < 0.04
J1650+4251 1.5431 ± 0.0003 0.10 ± 0.01 341 ± 19 3.21 ± 1.60 3.73 ± 1.90 0.011 ± 0.002
B1152+200 ( * ) < 0.03 - < 0.4 < 0.5 1.35 ± 0.01
B1600+434 ( * ) < 0.01 - < 0.4 < 0.5 3.43 ± 0.01
J0806+2006 1.5422 ± 0.0006 0.03 ± 0.01 548 ± 36 0.87 ± 0.49 1.01 ± 0.57 < 0.004

Notes. The table lists: CO(2–1) line flux, line FWHM (measured from the spectra), CO(2–1) line luminosity, CO(1–0) line luminosity given r21 = 0.86, and the rest-frame 1.3-mm continuum. Luminosities and fluxes were corrected for magnification as given in Table 1. Upper limits are quoted at the 3σ level. ( * )Radio–loud, “jetted” QSOs (Stacey et al. 2018).

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