Open Access

Table B.1.

Measurements of brightness and linear polarization of S4 0954+65 in optical bands via dedicated observations.

Ins. Band MJD m σm ΠO σΠO ΨO σΨO
NOT B 60088.944 13.3% 0.4% 69.3° 0.7°
B 60092.926 14.2% 0.3% 72.5° 0.5°
B 60097.899 10.8% 0.3% 150.6° 0.6°

V 60088.948 13.4% 0.2% 65.9° 0.4°
V 60092.930 13.6% 0.2% 69.0° 0.3°
V 60097.902 11.6% 0.2% 146.6° 0.3°

R 60088.939 13.8% 0.2% 63.1° 0.3°
R 60092.903 12.1% 0.1% 64.6° 0.2°
R 60097.893 11.9% 0.1% 141.0° 0.2°
I 60088.941 14.0% 0.2% 61.4° 0.3°
I 60092.906 11.8% 0.1% 63.0° 0.2°
I 60097.896 12.4% 0.1% 140.6° 0.3°

T90 B 60074.867 15.92 0.01
B 60075.988 15.31 0.01

V 60074.869 15.25 0.01
V 60075.990 14.73 0.01

R 60065.974 14.70 0.01
R 60067.878 14.13 0.01 36.3% 0.4% 89.6° 0.3°
R 60074.871 14.71 0.01
R 60075.992 14.21 0.01

X-200 I 60074.871 14.01 0.01
I 60075.993 13.55 0.01
R 60087.898 14.33 0.02 6.5% 0.5% 113.5° 2.1°
R 60088.887 14.35 0.02 17.87% 0.48% 67.8° 0.8°
R 60089.913 14.30 0.02 12.70% 0.56% 148.8° 1.3°
R 60090.900 14.08 0.02 16.09% 0.77% 108.1° 1.4°
R 60091.901 14.45 0.02 6.15% 0.60% 61.7° 2.8°
R 60092.906 14.12 0.02 13.83% 0.57% 67.3° 1.2°
R 60094.898 13.23 0.01 19.21% 0.36% 65.8° 0.6°
R 60094.917 13.24 0.02 19.28% 0.51% 69.0° 0.8°
R 60094.929 13.21 0.02 19.89% 0.44% 72.5° 0.7°

I 60087.910 13.69 0.02
I 60088.903 13.65 0.01
I 60089.944 13.63 0.03
I 60090.886 13.42 0.02
I 60091.913 13.80 0.01
I 60092.917 13.48 0.01
I 60094.907 12.64 0.01

RoboPol R 60082.835 14.28 0.02 13.98% 0.12% 149.0° 0.3°
R 60082.842 14.29 0.02 13.22% 0.16% 150.1° 0.4°
R 60083.802 14.13 0.02 10.40% 0.10% 143.0° 0.3°
R 60104.818 14.12 0.02 13.48% 0.10% 154.2° 0.2°
R 60105.811 13.95 0.02 27.09% 0.10% 176.5° 0.1°
R 60106.824 13.87 0.02 17.02% 0.09% 164.5° 0.2°

Notes. “Ins.” represents the instrument or telescope facility employed (see Sect. 3). “Band” gives the optical band. m and σm refer to the brightness and its error in magnitudes, respectively. ΠO and σΠO give the optical polarization degree and its error, respectively. ΨO and σΨO represent the optical polarization angle and its error, respectively. All errors are 1σ Gaussian. For brevity, in case of several equivalent (within 1σ) brightness entries per one night, only one one of them is shown.

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