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Table 5

Results from the light curve study for those central stars with negligible or minimal contamination analysed with models including reflection, ellipsoidal, and Doppler beaming.

Name BestModel Period T0-2458300 Aref Abeam Aellip
(days) (days) (ppt) (ppt) (ppt)
PG1034+001(*) 3E 1.8567960.000012+0.000012$1.856796_{ - 0.000012}^{ + 0.000012}$ 55.22500.0062+0.0061$55.2250_{ - 0.0062}^{ + 0.0061}$ 0.00910.0068+0.015$0.0091_{ - 0.0068}^{ + 0.015}$ 4.2020.064+0.063$4.202_{ - 0.064}^{ + 0.063}$ 3.0510.062+0.063$3.051_{ - 0.062}^{ + 0.063}$
NGC 246(*) 3E 4.995740.00073+0.00072$4.99574_{ - 0.00073}^{ + 0.00072}$ 61.0300.093+0.096$61.030_{ - 0.093}^{ + 0.096}$ 0.2380.035+0.035$0.238_{ - 0.035}^{ + 0.035}$ 0.1030.037+0.037$0.103_{ - 0.037}^{ + 0.037}$ 0.2560.035+0.034$0.256_{ - 0.035}^{ + 0.034}$
IC 2149 3E 1.312740.00065+0.00066$1.31274_{ - 0.00065}^{ + 0.00066}$ 80.3000.230+0.227$80.300_{ - 0.230}^{ + 0.227}$ 7.5450.127+0.126$7.545_{ - 0.127}^{ + 0.126}$ 1.0300.255+0.249$1.030_{ - 0.255}^{ + 0.249}$ 2.0910.133+0.136$2.091_{ - 0.133}^{ + 0.136}$
NGC 1501 3E 3.28300.0043+0.0053$3.2830_{ - 0.0043}^{ + 0.0053}$ 80.050.72+0.59$80.05_{ - 0.72}^{ + 0.59}$ 1.740.12+0.12$1.74_{ - 0.12}^{ + 0.12}$ 0.500.13+0.13$0.50_{ - 0.13}^{ + 0.13}$ 2.030.12+0.12$2.03_{ - 0.12}^{ + 0.12}$
IC 4593 3E 2.503690.00064+0.00061$2.50369_{ - 0.00064}^{ + 0.00061}$ 63.700.33+0.34$63.70_{ - 0.33}^{ + 0.34}$ 12.7720.053+0.051$12.772_{ - 0.053}^{ + 0.051}$ 0.00490.0037+0.0087$0.0049_{ - 0.0037}^{ + 0.0087}$ 2.6830.055+0.058$2.683_{ - 0.055}^{ + 0.058}$
K 1-16 3E 3.866240.00043+0.00046$3.86624_{ - 0.00043}^{ + 0.00046}$ 80.690.16+0.14$80.69_{ - 0.16}^{ + 0.14}$ 0.560.15+0.15$0.56_{ - 0.15}^{ + 0.15}$ 0.990.13+0.13$0.99_{ - 0.13}^{ + 0.13}$ 0.680.12+0.12$0.68_{ - 0.12}^{ + 0.12}$

Notes. (*) Targets already analysed in Cycle 1 (Aller et al. 2020).

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