Filaments in and between galaxy clusters at low and mid-frequency with the SKA

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Table 2

Sensitivities corresponding to different frequency ranges and channel widths considered in this work for the SKA, its precursors, and pathfinders. See the text for more details.

Instrument	rms, 1 h, 10 MHz		t₁ = 10 h			t₂ = 100 h

	(mJy/beam)	σ_I,Q,U (μJy/beam)	σ_P (mJy/beam)	σ_P,ϕ (μJy/beam)	σ_I,Q,U (μJy/beam)	σ_P (mJy/beam)	σ_P,ϕ (μJy/beam)
ν=110–166 MHz, dν=45 kHz

LOFAR 2.0	0.41	54.9	5.9	77.6	17.3	1.9	24.5
SKA-LOW	0.048	6.3	0.7	8.9	2.0	0.2	2.8

ν=110–166 MHz, dν=12 kHz

SKA-LOW	0.048	6.3	1.3	8.9	2.0	0.4	2.8

ν=110–350 MHz, dν=45 kHz

SKA-LOW	0.042	2.7	0.4	3.8	0.9	0.1	1.2

ν=900–1670 MHz, dν=1 MHz

MeerKAT+	0.02	0.8	0.06	1.1	0.2	0.02	0.3

ν=950–1760 MHz, dν=1 MHz

SKA-MID	0.015	0.5	0.04	0.6	0.1	0.01	0.2

Instrument	rms, 1 h, 10 MHz			t = 15 min

	mJy/beam	σ_I,Q,U μJy/beam		σ_P mJy/beam		σ_P,ϕ μJy/beam

ν=950–1760 MHz, dν=1 MHz

SKA-MID	0.015	2.9		0.2		4.1

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