Open Access

Table A.1

Observation log of V530 Per in 17, 18, 22, 23 Oct 2018).

Date (Oct 2018) HJD (2458400+) Phase Peak S/N
17 8.99494 0.9655 105
17 9.02392 0.0559 106
17 9.05458 0.1516 105
17 9.08355 0.2420 106
17 9.11393 0.3368 98
17 9.14289 0.4271 97

18 9.90980 0.8200 100
18 9.93932 0.9121 100
18 9.96921 0.0053 99
18 9.99874 0.0975 98
18 10.02863 0.1907 99
18 10.05815 0.2828 103
18 10.08808 0.3762 100
18 10.11764 0.4685 98

22 13.85090 0.1167 108
22 13.88046 0.2089 102
22 13.91070 0.3033 100
22 13.94026 0.3955 88
22 13.97037 0.4895 94
22 13.99993 0.5817 91
22 14.03189 0.6814 91
22 14.06144 0.7736 95
22 14.09169 0.8680 97
22 14.12124 0.9602 97

23 14.83713 0.1939 106
23 14.86665 0.2860 108
23 14.89699 0.3806 110
23 14.92654 0.4728 107
23 14.95677 0.5671 109
23 14.98633 0.6594 110
23 15.01713 0.7555 107
23 15.04668 0.8477 107
23 15.07681 0.9417 108
23 15.10637 0.0339 103

Note: Every Stokes V spectra consisted of 4 individual unpolarized subexposures with fixed exposure time equal to 600s. From left to right,we list the date, the Julian date, the rotational phases calculated with Eq.1, and the peak S/N.

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