Identifying frequency de-correlated dust residuals in B-mode maps by exploiting the spectral capability of bolometric interferometry

Open Access

Table 1.

Parameters used for analyzing simulations with FGBuster for all dust models.

Map N_side	256
Multipole range	21–335
Δℓ	35
Input r	0, 0.006
Residual lensing fraction ^(a)	10%
Sky fraction [%]	3%
Sky patch center ^(b)
[Equatorial coord.]	RA = 0°
	Dec = −45°

Notes.

^(a)

This is the fraction of the lensing signal left in the CMB map.

^(b)

Center of the CMB-S4 sky patch.

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