All Figures

	Figure 1: Spectra of the 12 CO(J=32) and C  I   lines towardsH1413+117, superposed on their Gaussian fit profiles (see Table 1 for parameters). The velocity scale is relative to the tuning frequencies of 97.191 and 227.478 GHz corresponding to z=2.5579.
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In the text

	Figure 2: Integrated C  I   intensity distribution in H1413+117. Contours are plotted at -1.5, -1.0 and from 1.0 to 4.0 in steps of 0.5 Jy beam-1 km s-1. The rms noise is 0.5 Jy beam-1 km s-1, the peak flux density is 4.3 Jy beam-1 km s-1. The continuum has been subtracted.
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In the text

Figure 3: Radio-IR SED of H1413+117. Displayed flux densities were taken from Barvainis & Lonsdale (1997) (20, 6, 3, 2 cm, stars), Solomon et al.  (2003) (1.2 cm cross), this work (3 mm, 1.3 mm, 1.2 mm, filled squares), Barvainis et al.  (1995) (1.2 mm, 760 m, 438 m, 345 m, 100 m, 60 m, circles), Barvainis & Ivison (2002) (850 m, filled triangle), Hughes et al.  (1997) (800 m, filled circle), Benford et al.  (1999) (350 m, pentagon) and Rowan-Robinson (2000) (200 m, triangle). The dashed lines show the thermal dust continuum emission for a 50 and 115 K dust component. The solid line is the total emission from both components.

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In the text