Table 1: Observed CO and $\mbox{\rm C {\scriptsize I}}$ line parameters towards F10214.
Line Telescope $\nu_{\rm obs}$ $S_\nu$a $\Delta$ $V_{\rm FWHM}$b Ia Vb L'/10$^{\rm 10}$  c
    [GHz] [mJy] [km s-1] [Jy km s-1] [km s-1] [K km s-1 pc2]
avg. profile IRAM 30 m ... ... 246 $\pm$ 10 ... 20 $\pm$ 4 ...
CO(3-2) IRAM 30 m 105.25230 15.5 $\pm$ 3.5 174 $\pm$ 23 3.80 $\pm$ 0.45 25 $\pm$ 11 10.83 $\pm$ 1.28
CO(3-2) PdBI 105.25160 13.5 $\pm$ 0.6 224 $\pm$ 12 3.40 $\pm$ 0.19 4 $\pm$ 4 9.70 $\pm$ 0.54
CO(4-3) IRAM 30 m 140.33020 21.7 $\pm$ 4.0 245 $\pm$ 28 5.32 $\pm$ 0.51 17 $\pm$ 11 8.53 $\pm$ 0.82
CO(6-5) IRAM 30 m 210.46850 28.8 $\pm$ 3.3 203 $\pm$ 16 7.09 $\pm$ 0.47 20 $\pm$ 7 5.06 $\pm$ 0.34
CO(7-6) IRAM 30 m 245.52621 22.1 $\pm$ 4.6 248 $\pm$ 30 5.43 $\pm$ 0.56 18 $\pm$ 14 2.84 $\pm$ 0.29
C I $(^3{\rm P}_1 \to ~\! ^3{\rm P}_0)$ IRAM 30 m 149.80235 8.3 $\pm$ 2.4 156 $\pm$ 26 2.03 $\pm$ 0.36 -5 $\pm$ 14 2.86 $\pm$ 0.51d
C I $(^3{\rm P}_2 \to ~\!^3{\rm P}_1)$ PdBI 246.34500 18.7 $\pm$ 2.3 182 $\pm$ 30 4.59 $\pm$ 0.66 -6 $\pm$ 10 2.39 $\pm$ 0.34
a The values are derived from Gaussian fits with the fixed line width and center velocity of the averaged CO line profile.
b The values are obtained from Gaussian fits to each spectrum. The velocity offsets are centered at a redshift of 2.2854 (Downes et al. 1995).
c We use a $\Lambda$ cosmology with $H_{\rm0}$ = 73  $\rm\mbox{{km~s$^{-1}$ }}~Mpc^{-1}$, $\rm\Omega_\Lambda$ = 0.74 and $\rm\Omega_{\rm m}$ = 0.26 (Spergel et al. 2007).
d The data are from Weiß et al. (2005a), but fitted with the fixed line width and central velocity.

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