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Table 2.

[CI] line properties.

Source Line νobs Redshift FWHM μTK μI[CI] μL μL
(GHz) (km s−1) (mK) (Jy km s−1) (1011 K km s−1 pc2) (108L)
PLCK_G045.1+61.1 [CI] 1–0 111.133 ± 0.024 3.4280 ± 0.0002 589 ± 145 2.3 8.4 ± 1.7 2.3 ± 0.5 8.6 ± 1.7

PLCK_G080.2+49.8 [CI] 1–0 136.767 ± 0.008 2.5985 ± 0.0002 242 ± 61 3.8 6.2 ± 0.9 1.1 ± 0.2 4.0 ± 0.7
PLCK_G080.2+49.8 [CI] 2–1 224.847 ± 0.025 2.5995 ± 0.0003 312 ± 24 2.3 5.8 ± 1.0 0.37 ± 0.08 6.2 ± 1.2

PLCK_G092.5+42.9 [CI] 1–0 115.641 ± 0.016 3.2559 ± 0.0006 475 ± 128 4.5 13.5 ± 2.6 3.3 ± 0.6 12.8 ± 2

PLCK_G102.1+53.6 [CI] 2–1 206.608 ± 0.006 2.9173 ± 0.0001 220 ± 21 2.3 4.0 ± 0.4 0.3 ± 0.3 5.2 ± 0.5

PLCK_G113.7+61.0 [CI] 1–0 144.019 ± 0.020 2.41730 ± 0.0003 639 ± 100 2.3 10.2 ± 1.2 1.5 ± 0.2 5.9 ± 0.7
PLCK_G113.7+61.0 [CI] 2–1 237.395 ± 0.002 2.40927 ± 0.0001 504 ± 10 2.9 9.2 ± 1.0 0.5 ± 0.05 8.6 ± 0.9

PLCK_G138.6+62.0 [CI] 1–0 142.974 ± 0.020 2.4423 ± 0.0003 575 ± 86 2.4 9.5 ± 1.5 1.5 ± 0.2 5.6 ± 0.9
PLCK_G138.6+62.0 [CI] 2–1 235.129 ± 0.003 2.4421 ± 0.0001 526 ± 5 4.5 18.8 ± 0.2 1.1 ± 0.01 18.0 ± 0.1

PLCK_G145.2+50.9 [CI] 1–0 108.204 ± 0.009 3.5485 ± 0.0003 405 ± 63 5.8 14.8 ± 3.5 4.2 ± 1.0 16.0 ± 3.8

PLCK_G165.7+67.0 [CI] 1–0 152.079 ± 0.009 2.2362 ± 0.0001 629 ± 46 2.6 11.1 ± 2.8 1.5 ± 0.4 5.6 ± 1.4
PLCK_G165.7+67.0 [CI] 2–1 250.059 ± 0.025 2.2366 ± 0.0002 418 ± 6 2.6 8.3 ± 0.2 0.4 ± 0.09 6.8 ± 0.1

PLCK_G200.6+46.1 [CI] 2–1 203.697 ± 0.018 2.97326 ± 0.0001 412 ± 5 2.5 8.3 ± 0.1 0.7 ± 0.01 11.1 ± 0.1

PLCK_G231.3+72.2 [CI] 2–1 209.729 ± 0.015 2.85899 ± 0.0001 319 ± 18 2.7 6.9 ± 0.4 0.5 ± 0.03 8.7 ± 0.5

PLCK_G244.8+54.9 [CI] 2–1 202.113 ± 0.002 3.00440 ± 0.0001 586 ± 5 4.5 21.0 ± 0.2 1.7 ± 0.02 28.6 ± 0.3

Notes. We list the source name, the line, observed frequency, redshift, full-width at half maximum of the line, main-beam brightness temperature, integrated line flux, and the line luminosity in units proportional to brightness temperature and energy, respectively. We give observed values here, where μ indicates the gravitational magnification factor. Luminosity-weighted average gravitational correction factors are given in Table 1 of C18, and are repeated in our Table 3 for convenience.

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