Table 1: Characteristics of the three types of experiments considered. We run our extraction method on 100 sky patches of $3 \times 3$ square degrees (for AMI and SPT) and $12 \times 12$ square degrees (for Planck).
Type Frequencies Res. FWHM Inst. noise Area

[GHz] [arcmin] [ $\mu {\rm K/beam}$ ] [ ${\rm deg}^{2}$ ]

AMI 15 1.5 8 10

SPT 150 1 10

220 0.7 60 4000

275 0.6 100

Planck 143 7.1 6

217 5 13 41253

353 5 40

**Table 1:** Characteristics of the three types of experiments considered. We run our extraction method on 100 sky patches of $3 \times 3$ square degrees (for AMI and SPT) and $12 \times 12$ square degrees (for Planck).
Type	Frequencies	Res. FWHM	Inst. noise	Area
	[GHz]	[arcmin]	[ $\mu {\rm K/beam}$ ]	[ ${\rm deg}^{2}$ ]
AMI	15	1.5	8	10
SPT	150	1	10
	220	0.7	60	4000
	275	0.6	100
Planck	143	7.1	6
	217	5	13	41253
	353	5	40

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