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Table A.2.

Properties of the CO emission lines obtained by fitting the continuum-subtracted spectra using a single or two Gaussian components with CLASS.

Source Line νobs (GHz) Redshift FWHMline (km s−1) μIline (Jy km s−1) μLline (108L) (1010 K km s−1 pc2)
PLCK_G045.1+61.1 CO(4–3) 104.16 ± 0.01 3.4261 ± 0.0003 224 ± 51 10.6 ± 2.0 10.7 ± 2.0 34.1 ± 6.4
104.01 ± 0.01 3.4326 ± 0.0005 397 ± 78 12.7 ± 2.2 12.8 ± 2.2 40.8 ± 7.1
CO(5–4) (130.20) (3.4261) 191 ± 16 10.9 ± 0.8 13.8 ± 1.0 22.5 ± 1.6
(130.01) (3.4326) 484 ± 41 15.7 ± 1.2 19.8 ± 1.5 32.4 ± 2.5
CO(6–5) (156.23) (3.4261) 369 ± 107 9.2 ± 2.6 13.9 ± 3.9 13.2 ± 3.7
(156.00) (3.4326) 554 ± 115 11.4 ± 2.9 17.2 ± 4.4 16.4 ± 4.2
CO(8–7) (208.26) (3.4261) 241 ± 62 3.5 ± 0.9 7.1 ± 1.8 2.8 ± 0.7
(207.96) (3.4326) 304 ± 107 2.7 ± 0.9 5.4 ± 1.8 2.2 ± 0.7
CO(9–8) (500) < 23.1 < 52.4 < 14.7
PLCK_G080.2+49.8 CO(3–2) 96.10 ± 0.01 2.5984 ± 0.0001 319 ± 35 7.9 ± 0.6 3.8 ± 0.3 28.6 ± 2.2
CO(5–4) 160.13 ± 0.01 2.5987 ± 0.0003 431 ± 84 10.5 ± 1.0 8.4 ± 0.8 13.7 ± 1.3
CO(7–6) 224.17 ± 0.02 2.5984 ± 0.0003 245 ± 52 4.1 ± 0.8 4.6 ± 0.9 2.7 ± 0.5
PLCK_G092.5+42.9 CO(4–3) 108.39 ± 0.01 3.2535 ± 0.0001 267 ± 21 15.6 ± 1.6 14.5 ± 1.5 46.2 ± 4.7
108.29 ± 0.01 3.2575 ± 0.0001 270 ± 18 21.3 ± 1.6 19.8 ± 1.5 63.1 ± 4.7
CO(5–4) (135.48) (3.2535) 234 ± 35 16.0 ± 1.4 18.6 ± 1.6 30.3 ± 2.7
(135.35) (3.2575) 253 ± 35 19.6 ± 1.5 22.8 ± 1.7 37.2 ± 2.8
CO(6–5) (162.57) (3.2535) 257 ± 49 16.4 ± 2.7 22.9 ± 3.8 21.6 ± 3.6
(162.41) (3.2575) 280 ± 92 9.3 ± 2.8 13.0 ± 3.9 12.3 ± 3.7
CO(8–7) (216.72) (3.2535) 270 ± 34 15.5 ± 1.8 28.8 ± 3.3 11.5 ± 1.3
(216.51) (3.2575) 182 ± 23 13.4 ± 1.5 24.9 ± 2.8 9.9 ± 1.1
CO(9–8) (243.78) (3.2535) 229 ± 18 12.4 ± 0.9 25.9 ± 1.9 7.3 ± 0.5
(243.55) (3.2575) 258 ± 20 15.5 ± 1.0 32.4 ± 2.1 9.1 ± 0.6
CO(10–9) (270.83) (3.2535) 261 ± 114 9.0 ± 2.9 20.9 ± 6.7 4.3 ± 1.4
(270.58) (3.2575) 255 ± 59 10.6 ± 2.5 24.6 ± 5.8 5.0 ± 1.2
PLCK_G102.1+53.6 CO(3–2) 88.29 ± 0.01 2.9166 ± 0.0004 215 ± 58 5.1 ± 1.8 3.0 ± 1.0 22.4 ± 7.9
CO(5–4) 147.12 ± 0.01 2.9171 ± 0.0002 324 ± 89 11.0 ± 1.8 10.7 ± 1.7 17.4 ± 2.9
CO(7–6) 205.93 ± 0.01 2.9172 ± 0.0002 186 ± 42 5.0 ± 0.9 6.8 ± 1.2 4.0 ± 0.7
PLCK_G113.7+61.0 CO(3–2) 101.21 ± 0.01 2.4166 ± 0.0002 537 ± 44 18.2 ± 1.4 7.7 ± 0.6 58.2 ± 4.5
CO(4–3) 134.94 ± 0.01 2.4166 ± 0.0002 541 ± 43 20.5 ± 1.5 11.6 ± 0.8 36.9 ± 2.7
CO(5–4) 168.66 ± 0.01 2.4168 ± 0.0003 484 ± 54 21.2 ± 2.1 15.0 ± 1.5 24.4 ± 2.4
CO(7–6) 236.09 ± 0.01 2.4167 ± 0.0001 482 ± 26 20.7 ± 1.1 20.4 ± 1.1 12.2 ± 0.6
CO(8–7) 269.83 ± 0.03 2.4162 ± 0.0004 426 ± 85 21.6 ± 3.6 24.4 ± 4.1 9.7 ± 1.6
PLCK_G138.6+62.0 CO(3–2) 100.46 ± 0.01 2.4420 ± 0.0002 487 ± 56 22.4 ± 2.1 9.7 ± 0.9 73.0 ± 6.8
CO(4–3) 133.95 ± 0.01 2.4420 ± 0.0002 537 ± 35 26.9 ± 1.6 15.5 ± 0.9 49.3 ± 2.9
CO(5–4) 167.44 ± 0.02 2.4416 ± 0.0005 630 ± 103 28.1 ± 3.6 20.2 ± 2.6 33.0 ± 4.2
CO(7–6) 234.37 ± 0.01 2.4418 ± 0.0002 472 ± 33 26.5 ± 1.9 26.7 ± 1.9 15.9 ± 1.1
PLCK_G145.2+50.9 CO(4–3) 101.38 ± 0.01 3.5477 ± 0.0002 397 ± 79 25.6 ± 1.8 27.4 ± 1.9 87.2 ± 6.1
101.20 ± 0.02 3.5557 ± 0.0009 355 ± 28 10.3 ± 1.9 11.0 ± 2.0 35.2 ± 6.5
CO(6–5) (152.04) (3.5477) 370 ± 39 32.4 ± 3.6 51.9 ± 5.8 49.0 ± 5.4
(151.78) (3.5557) 290 ± 70 8.9 ± 3.0 14.2 ± 4.8 13.5 ± 4.6
PLCK_G165.7+67.0 CO(3–2) 106.85 ± 0.01 2.2363 ± 0.0004 655 ± 86 26.8 ± 3.2 9.9 ± 1.2 75.0 ± 9.0
CO(4–3) 142.47 ± 0.01 2.2362 ± 0.0002 547 ± 40 29.2 ± 2.0 14.4 ± 1.0 46.0 ± 3.1
CO(6–5) 213.64 ± 0.01 2.2367 ± 0.0002 640 ± 39 29.8 ± 1.5 22.1 ± 1.1 20.9 ± 1.0
CO(7–6) 249.23 ± 0.02 2.2365 ± 0.0002 580 ± 48 18.6 ± 1.3 16.1 ± 1.1 9.6 ± 0.7
PLCK_G200.6+46.1 CO(3–2) 87.04 ± 0.01 2.9726 ± 0.0004 505 ± 57 13.3 ± 1.4 8.0 ± 0.8 60.4 ± 6.4
CO(4–3) (500) < 17.0 < 13.6 < 43.4
CO(5–4) 145.06 ± 0.01 2.9727 ± 0.0003 481 ± 45 12.7 ± 1.2 12.7 ± 1.2 20.7 ± 2.0
CO(7–6) 203.00 ± 0.02 2.9735 ± 0.0003 333 ± 41 6.6 ± 0.9 9.2 ± 1.3 5.5 ± 0.8
CO(8–7) (500) < 9.7 < 15.5 < 6.2
PLCK_G231.3+72.2 CO(3–2) 89.61 ± 0.01 2.8589 ± 0.0003 445 ± 62 12.9 ± 1.3 7.3 ± 0.7 54.9 ± 5.5
CO(5–4) 149.32 ± 0.01 2.8592 ± 0.0002 350 ± 36 18.4 ± 1.5 17.3 ± 1.4 28.2 ± 2.3
CO(7–6) 209.02 ± 0.02 2.8592 ± 0.0003 469 ± 71 12.4 ± 1.4 16.3 ± 1.8 9.7 ± 1.1
PLCK_G244.8+54.9 CO(3–2) 86.38 ± 0.01 3.0033 ± 0.0004 282 ± 56 8.3 ± 0.8 5.1 ± 0.5 38.3 ± 3.7
86.28 ± 0.02 3.0078 ± 0.0008 403 ± 75 9.5 ± 1.2 5.8 ± 0.7 44.0 ± 5.6
CO(4–3) (115.17) (3.0033) 293 ± 51 13.3 ± 2.2 10.8 ± 1.8 34.5 ± 5.7
(115.04) (3.0078) 316 ± 60 13.6 ± 2.3 11.1 ± 1.9 35.4 ± 6.0
CO(5–4) (143.95) (3.0033) 283 ± 23 13.2 ± 1.2 13.5 ± 1.2 21.9 ± 2.0
(143.79) (3.0078) 525 ± 47 20.5 ± 1.6 20.9 ± 1.6 34.1 ± 2.7
CO(6–5) (172.73) (3.0033) 323 ± 98 14.2 ± 3.7 17.4 ± 4.5 16.4 ± 4.3
(172.53) (3.0078) 667 ± 180 22.7 ± 3.8 27.7 ± 4.6 26.3 ± 4.4
CO(8–7) (230.26) (3.0033) 461 ± 125 12.1 ± 3.0 19.7 ± 4.9 7.9 ± 1.9
(230.00) (3.0078) 640 ± 131 18.5 ± 3.1 30.1 ± 5.1 12.0 ± 2.0
CO(9–8) (259.01) (3.0033) 321 ± 35 14.2 ± 1.5 26.0 ± 2.8 7.3 ± 0.8
(258.72) (3.0078) 466 ± 51 18.9 ± 1.9 34.6 ± 3.5 9.7 ± 1.0
CO(10–9) (287.76) (3.0033) 297 ± 34 18.1 ± 1.9 36.9 ± 3.9 7.5 ± 0.8
(287.44) (3.0078) 341 ± 46 13.5 ± 1.8 27.5 ± 3.7 5.6 ± 0.8
CO(11–10) 316.22 ± 0.06 3.0066 ± 0.0008 579 ± 89 24.8 ± 4.3 55.5 ± 9.6 8.5 ± 1.5

Notes. Columns are: source name; CO transition; observed frequency; redshift of the line or spectral component; line FWHM; velocity-integrated flux density μIline, used for the line-excitation analysis and uncorrected for lensing magnification; observed line luminosity in solar luminosities and in K km s−1 pc2. For the sources fitted with two Gaussians, we fixed the central velocity of each spectral component to those measured on the lowest-J CO transition.

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