QUIJOTE scientific results - XVIII. New constraints on the polarisation of the anomalous microwave emission in bright Galactic regions: ρ Ophiuchi, Perseus, and W43

Open Access

Table B.7.

Same as Table B.5 but for W43.

Freq.	S_ν^AME or $S_{ν}^{dust}$ $S_{\nu}^{\mathrm{dust}}$	Q	U	P_db	Π_AME or Π_dust
(GHz)	(Jy)	(Jy)	(Jy)	(Jy)	(%)
	AME
16.8	187 ± 30	-0.16 ± 0.30	-1.02 ± 0.34	0.97 $_{- 0.33}^{+ 0.34}$ $^{+0.34}_{-0.33}$	< 0.85
18.8	207 ± 30	0.17 ± 0.76	1.69 ± 0.76	1.49 $_{- 0.77}^{+ 0.85}$ $^{+0.85}_{-0.77}$	< 1.41
22.8	205 ± 21	0.56 ± 0.18	-0.28 ± 0.11	0.61 ± 0.14	< 0.42
28.4	219 ± 22	0.20 ± 0.17	0.44 ± 0.11	0.47± 0.14	< 0.33
33.0	193 ± 21	0.20 ± 0.22	-0.22 ± 0.13	0.22 $_{- 0.12}^{+ 0.20}$ $^{+0.20}_{-0.12}$	< 0.28
40.6	164 ± 19	0.10 ± 0.11	-0.30 ± 0.18	0.28 $_{- 0.14}^{+ 0.15}$ $^{+0.15}_{-0.14}$	< 0.32
44.1	147 ± 18	0.12 ± 0.20	0.55 ± 0.14	< 0.82	< 0.57
60.5	86 ± 19	0.20 ± 0.37	0.22 ± 0.45	< 0.92	< 1.11
70.4	72 ± 23	-0.46 ± 0.33	1.34 ± 0.33	< 1.96	< 3.44
22.8 (stack)	189 ± 18	0.046 ± 0.091	0.461 ± 0.051	0.46 ± 0.09	< 0.31

	Thermal dust
100	306 ± 49	2.50 ± 0.255	-2.96 ± 0.27	3.87 ± 0.26	1.27 ± 0.22
143	1092 ± 185	8.46 ± 0.56	1.19 ± 0.54	8.54 ± 0.54	0.78 ± 0.14
217	4693 ± 863	36.3 ± 3.3	15 ± 3	39 ± 3	0.84 ± 0.16
353	24235 ± 5196	120 ± 14	39 ± 12	127 ± 13	0.53 ± 0.12

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