Temporal and chromatic variation of polarized scattered light in the outer disk of PDS 70

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Table A.3.

Aperture count rates for the total intensity, I_⋆, the azimuthal polarization, Q_φ, and the ratio, Q_φ/I_⋆, for PDS 70 for each observing date.

Label	I_⋆ [×10⁴s⁻¹]	Q_φ [×10⁴s⁻¹]	Q_φ/I_⋆ [%]	${\hat{Q}}_{φ}$ $\hat{Q}_{\varphi}$ [×10⁴s⁻¹]	${\hat{Q}}_{φ} / I_{⋆}$ $\hat{Q}_{\varphi}/I_{\star}$ [%]	Proc ^a
NR	30.6 ± 0.2	0.029 ± 0.004	0.093 ± 0.012	0.050 ± 0.005	0.163 ± 0.016	A
VBB	124.6 ± 1.4	0.214 ± 0.016	0.171 ± 0.012	0.483 ± 0.006	0.388 ± 0.005	A
J16	80.0 ± 2.4	0.139 ± 0.023	0.174 ± 0.034	0.257 ± 0.044	0.321 ± 0.065	B2
J17	175.8 ± 0.6	0.336 ± 0.026	0.191 ± 0.015	0.585 ± 0.055	0.333 ± 0.031	A
H19	111.3 ± 5.6	0.187 ± 0.014	0.168 ± 0.021	0.302 ± 0.022	0.271 ± 0.033	B1
H21	234.8 ± 10.7	0.611 ± 0.020	0.260 ± 0.020	0.824 ± 0.028	0.355 ± 0.028	B2
Ks	73.6 ± 2.2	0.220 ± 0.017	0.299 ± 0.032	0.295 ± 0.023	0.401 ± 0.043	B2

^(a)

Notes. Correction method applied to the integrated polarized flux as described in Ma et al. (2024).

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