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Table 3

CO line properties obtained with EMIR on the IRAM 30-m telescope.

Source Transition Line flux μICO Line luminosity μL μ M mol FWHM

[Jy km s-1] [1011 K km s-1 pc2] [1011 M] [km s-1]

PLCK_G045.1+61.1 4–3 22.9 ± 0.3 6.9 ± 0.1 5.6 ± 0.1 213 ± 11
PLCK_G080.2+49.8 3–2 9.2 ± 0.5 3.2 ± 0.2 2.6 ± 0.2 265 ± 12
PLCK_G092.5+42.9 4–3 34.3 ± 0.2 9.7 ± 0.1 7.8 ± 0.2 453 ± 3
PLCK_G102.1+53.6 3–2 5.7 ± 1.8 2.4 ± 0.7 2.0 ± 0.2 252 ± 10
PLCK_G113.7+61.0 3–2 16.5 ± 0.2 5.0 ± 0.1 4.0 ± 0.2 528 ± 5
PLCK_G138.6+62.0 3–2 22.0 ± 1.1 6.8 ± 0.3 5.4 ± 0.1 514 ± 40
PLCK_G145.2+50.9 3–2 21.9 ± 0.8 12.7 ± 0.6 10.2 ± 0.2 685 ± 17
PLCK_G165.7+67.0 3–2 25.4 ± 0.3 6.8 ± 0.1 5.4 ± 0.1 576 ± 4
PLCK_G200.6+46.1 3–2 11.2 ± 0.1 4.9 ± 0.1 3.8 ± 0.1 458 ± 9
PLCK_G231.3+72.2 3–2 9.4 ± 0.2 3.9 ± 0.1 3.0 ± 0.1 257 ± 8
PLCK_G244.8+54.9 3–2 7.4 ± 1.0 3.3 ± 0.4 2.6 ± 0.2 382 ± 10

Notes. The columns are source name; CO transition; integrated line flux; line luminosity μL (in brightness temperature units) derived using Eq. (1); molecular gas mass (see Sect. 9 for details); and full width at half maximum of the emission lines.

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