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Table 1:

Parameters of linear fits of FIR surface brightness versus the HI line area.
Field $\lambda$ Offset Slope
  ($\mu $m) (MJy sr-1) (10-3 MJy sr-1 K-1 km-1 s)
EBL22 90 5.53 (0.30) 35.15 (4.26)
EBL22 150 3.56 (0.34) 38.91 (4.38)
EBL22 180 3.10 (0.38) 27.95 (5.42)
EBL261 90 18.66 (1.22) 17.28 (6.57)
EBL261 150 6.38 (1.33) 27.42 (7.36)
EBL261 180 6.00 (1.30) 25.76 (7.41)
NGP 90 6.31 (0.17) 24.60 (3.98)
NGP 150 3.53 (0.23) 28.61 (5.58)
NGP 180 3.20 (0.19) 31.91 (4.22)
The 1-$\sigma$ error estimates determined with the bootstrap method are given in parentheses. For NGP, the results correspond to a fit to the combined data of the northern and southern sub-fields (see Appendix B.2).
1 Fit to data with $W({\rm HI})<$ 200 K km s-1 only.

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