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Table 1

Summary of SPHERE-ZIMPOL observations for IK Tau and its PSF reference star HIP 20188.

# tobs DIT NDIT Nexp Npol Ndither Filter Seeing AM Strehl Strehl
(UTC) (s) (cam1/cam2) (′′) (H) (visible)
IK Tau: 2016 Nov 20 (UTC)
1 02:40:58 80.0 2 1 2 3 CntHa/NHa 0.62 1.38 0.74 0.14
2 03:21:54 10.0 2 1 7 3 TiO717/Cnt748 0.91 1.25 0.71 0.18
3 06:57:36 5.0 4 1 3 3 Cnt820/Cnt820 0.68 1.6 0.73 0.28

HIP 20188: 2016 Nov 20 (UTC)
C1 05:21:49 4.0 40 1 1 3 CntHa/NHa 0.75 1.23 0.77 0.22
C2 05:59:43 2.0 6 1 7 3 TiO717/Cnt748 1.16 1.28 0.79 0.28
C3 06:30:04 2.0 8 1 3 3 Cnt820/Cnt820 0.76 1.34 0.82 0.41

Notes. DIT: detector integration time. NDIT:number of frames. Nexp: number of exposures of each polarization component in each polarization cycle at each dithering position. Npol: number of polarization cycles at each dithering position. Ndither: number of dithering positions. The seeing was measured in the visible. AM: airmass. The Strehl ratios in the visible were calculated from the H-band Strehl ratiosfor IK Tau, while they were measured from the observed ZIMPOL images for HIP 20188.

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