Online Material
Appendix: A
Table 7:
Results of the IR/HI correlations in the atomic phase for all sky
regions.
Cols. 1-2: central position of each studied regions in degree.
Column 3: number of pixels used for the correlations in each
studied regions. Columns 4-11:
results of the correlations in 
for 
.
Columns 12-13: emissivity
spectral indices in the range 100-240
(
)
and in the range 550-2100
(
). Column 14: derived
dust temperature in Kelvin. Errors bars represent the 1-
uncertainty estimates.
Table 8:
Results of the IR/CO correlations in the molecular phase for all sky
regions.
Columns 1-2: central position of each studied regions in
degree. Column 3: number of pixels used for the correlations
in each studied regions. Columns 4-11: results of the
correlations in
for 
.
Colums 12-13: emissivity
spectral indices in the range 100-240
(
)
and in the range 550-2100
(
). Column 14: derived
dust temperature in Kelvin. Errors bars represent the 1-
uncertainty estimates. Uncertainties equal to 0.0 are inferior
to 0.05.