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.6.

Same as Table B.5 but for Perseus.

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
11.1	6.8 ± 2.5	-0.24 ± 0.09	-0.29 ± 0.14	< 0.56	< 10.5
12.9	10.4 ± 2.4	-0.05 ± 0.26	-0.08 ± 0.21	< 0.48	< 4.7
16.8	21.1 ± 3.7	0.21 ± 0.31	0.04 ± 0.32	< 0.69	< 3.4
18.8	26.8 ± 4.0	-0.10 ± 0.56	0.13 ± 0.33	< 0.89	< 3.4
22.8	30.3 ± 2.8	-0.03 ± 0.15	-0.08 ± 0.14	< 0.31	< 1.0
28.4	30.4 ± 2.8	-0.07 ± 0.12	0.08 ± 0.13	< 0.29	< 0.9
33.0	27.9 ± 3.0	0.14 ± 0.18	-0.05 ± 0.24	< 0.47	< 1.7
40.6	22.6 ± 4.0	-0.25 ± 0.40	-0.34 ± 0.27	< 0.89	< 4.1
44.1	20.5 ± 4.7	0.07 ± 0.45	-0.61 ± 0.38	< 1.21	< 6.3
22.8 (stack)	29.80 ± 1.60	0.031 ± 0.087	0.073 ± 0.076	< 0.20	< 0.67

	Thermal dust
60.5	9.6 ± 2.1	1.14 ± 0.90	-0.88 ± 0.75	1.04 $_{- 0.58}^{+ 0.98}$ $^{+0.98}_{-0.58}$	< 29.5
70.4	16.4 ± 3.6	0.49 ± 0.62	-0.02 ± 0.73	< 1.51	< 9.7
93.5	44.1 ± 10.1	0.76 ± 1.55	-2.33 ± 2.44	< 5.24	< 12.6
100	55.7 ± 12.8	1.10 ± 0.47	-0.40 ± 0.71	0.98 $_{- 0.54}^{+ 0.66}$ $^{+0.66}_{-0.54}$	1.8 ± 1.2
143	191 ± 47	7.02 ± 1.07	-6.25 ± 1.89	9.40 ± 1.58	5.1 ± 1.4
217	776 ± 208	31.07 ± 3.76	-29.9 ± 8.0	43.1 ± 6.3	5.9 ± 1.6
353	3703 ± 1203	172 ± 17	-125 ± 34	212 ± 29	6.1 $_{- 2.0}^{+ 1.8}$ $^{+1.8}_{-2.0}$

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