Table 2
CIB field description: centre (in Galactic coordinates), size, mean and dispersion of Hi column density.
Radio telescope | Field name | l | b | Area | Mean N(Hi) | σN(Hi) |
[deg] | [deg] | [deg2] | [1020 cm-2] | [1020 cm-2] | ||
|
||||||
Effelsberg | EBHIS | 225 | 63 | 91.6 | 1.6 | 0.3 |
|
||||||
GBT | N1 | 85 | 44 | 26.4 | 1.2 | 0.3 |
AG | 165 | 66 | 26.4 | 1.8 | 0.6 | |
SP | 132 | 48 | 26.4 | 1.2 | 0.3 | |
LH2 | 152 | 53 | 16.2 | 0.7 | 0.2 | |
Bootes | 58 | 69 | 54.6 | 1.1 | 0.2 | |
NEP4 | 92 | 34 | 15.7 | 2.4 | 0.4 | |
SPC5 | 132 | 31 | 24.6 | 2.3 | 0.6 | |
SPC4 | 133 | 33 | 15.7 | 1.7 | 0.3 | |
MC | 57 | −82 | 31.2 | 1.4 | 0.2 | |
|
||||||
Parkes | GASS Mask1 | 225 | −64 | 1914 | 1.4 | 0.3 |
GASS Mask2 | 202 | −59 | 4397 | 2.0 | 0.8 |
Notes. The given area is the size used for the CIB power spectrum computation (i.e., removing the area lost by the masking). The “GASS Mask2” is not used for CIB power spectrum analysis but for some tests on the quality of our component separation, and for the measurement of the bispectrum. Mask2 includes all of Mask1.
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