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Table 2.

Properties of continuum and line (CO or [CII]) emission for the WISSH QSOs analysed here.

ID Transition zcold FWHM SΔv L[CII] Scont
(km s−1) (Jy km s−1) (1010 K km s−1 pc2) (109L) (mJy)
(1) (2) (3) (4) (5) (6) (7) (8)
J0209–0005 CO(5−4) 2.870 435 ± 95 1.4 ± 0.3 2.15 ± 0.46 0.38 ± 0.04
CO(1−0) 2.870 440 ± 85 0.062 ± 0.012 2.39 ± 0.46 0.039 ± 0.005
J0801+5210 CO(5−4) 3.256 685 ± 70 3.68 ± 0.40 6.99 ± 0.76 <0.30 (b)
CO(1−0) <0.095 (a) <4.48 0.091 ± 0.010
J1433+0227 [CII] 4.728 400 ± 40 5.40 ± 0.24 3.72 ± 0.16 7.7 ± 0.3
J1538+0855 CO(4−3) 3.572 320 ± 90 0.36 ± 0.11 1.23 ± 0.38 <0.087 (b)
J1549+1245 CO(4−3) 2.374 245 ± 40 0.27 ± 0.03 0.47 ± 0.05 0.12 ± 0.01
J1555+1003 CO(4−3) 3.529 605 ± 90 0.87 ± 0.14 2.94 ± 0.68 0.10 ± 0.02
J1639+2824 CO(4−3) 3.846 615 ± 90 0.92 ± 0.15 3.55 ± 0.66 <0.090 (b)
J1701+6412 CO(5−4) 2.753 595 ± 120 1.50 ± 0.34 2.15 ± 0.49 0.60 ± 0.06
J1015+0020 (*) [CII] 4.407 340 ± 40 0.47 ± 0.05 0.29 ± 0.03 0.60 ± 0.06

CompJ0209 CO(5−4) 2.881 600 ± 95 1.1 ± 0.3 1.74 ± 0.46 0.14 ± 0.03
CO(1−0) <0.044 (a) <1.71 <0.014 (b)
CompJ0801 CO(5−4) 3.271 385 ± 65 0.71 ± 0.26 1.36 ± 0.49 <0.30 (b)
CO(1−0) <0.058 (a) <2.78 <0.30 (b)
CompJ1433 [CII] 4.728 100 ± 43 0.11 ± 0.02 0.08 ± 0.02 <0.015 (b)
Comp1J1549 CO(4−3) 2.363 540 ± 95 0.29 ± 0.05 0.49 ± 0.08 0.12±0.01
Comp2J1549 CO(4−3) 2.374 540 ± 110 0.046 ± 0.013 0.08 ± 0.02 <0.021 (b)
CompJ1555 CO(4−3) 3.531 370 ± 70 0.29 ± 0.06 0.98 ± 0.20 <0.084 (b)
CompJ1701 CO(5−4) 2.753 130 ± 60 0.50 ± 0.19 0.84 ± 0.27 <0.30 (b)

Notes. Columns give the following information: (1) SDSS ID, (2) Observed transition, (3) Redshift estimated from (sub-)mm emission lines with typical uncertainty Δzcold ∼ 0.001, (4) and (5) FWHM and integrated flux of CO or [CII], (6) CO luminosity, (7) [CII] luminosity and (8) Continuum flux. Uncertainties do not include errors on abso. (*)Presented in Bischetti et al. (2018).

(a)

Upper limit computed for a point source as 3 × σcold, where σcold is the rms of the velocity integrated JVLA map produced by assuming the same FWHM of CO(5−4).

(b)

Upper limit computed for a point source as 3 × σcont (Table 1).

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