Probing cluster magnetism with embedded and background radio sources in Planck clusters

Open Access

Table 2.

Corrected standard deviation of RM in rad m⁻², as defined in Eq. (6) for different subsets and projected radii.

	< 0.5 R₅₀₀	0.5 − 1.0 R₅₀₀	< R₅₀₀	> R₅₀₀
All	244 ± 47	127 ± 30	209 ± 37	28 ± 5
Inside ^(a)	196 ± 40	219 ± 59	200 ± 33	27 ± 8
Behind ^(b)	312 ± 100	51 ± 6	219 ± 66	29 ± 6
CC ^(c)	159 ± 66	75 ± 24	133 ± 49	17 ± 3
NCC ^(d)	234 ± 42	60 ± 7	191 ± 35	17 ± 7

Notes. We refer to Fig. 6 for the corrected IQR as a function of radius.

^(a)

Sources located inside clusters.

^(b)

Sources located behind clusters.

^(c)

Only cool-core clusters.

^(d)

Only non-cool-core clusters.

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