Table 1: Observed line parameters.

Line		 $\nu_{\rm obs}$ $S_\nu$ $\Delta V_{\rm FWHM}$ I Va L'/1010 Ref.
  [GHz] [mJy] [km s-1] [Jy km s-1] [km s-1] [K km s-1  pc2]  

12 CO(J=3$\to $2)		 97.1928 30.0 $\pm$ 1.7 416 $\pm$ 6 13.2 $\pm$ 0.2 -5.6 $\pm$ 2.4 18.0 $\pm$ 0.3 this paper
C  I $\rm (^3P_2\!\to^3{\hskip-0.8mm}P_1)$ 227.4376 13.2 $\pm$ 2.9 368 $\pm$ 25 5.2 $\pm$ 0.3 53 $\pm$ 20 1.30 $\pm$ 0.07 this paper
C  I $\rm (^3P_1\!\to^3{\hskip-0.8mm}P_0)$ 138.351 7.7 $\pm$ 0.8 430 $\pm$ 46 3.6 $\pm$ 0.4 -47 $\pm$ 24 2.4 $\pm$ 0.3 B97
Quoted errors are statistical errors from Gaussian fits. Systematic calibration uncertainty is 10%.
a The velocity is given relative to z=2.5579, the mean redshift of the CO lines determined by B97.
CO fluxes for 3-2, 4-3, 5-4, 7-6 are: 13.2, 21.1, 24.0, 47.3 [Jy km s-1]; all values except for 3-2 are from B97.
CO line luminosities L' are: 18.0, 16.1, 11.7, 10.9 [1010 $L_{\odot}$].

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