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Table 2

Parameters of the 288P components obtained for the different variants of light curve fitting.

Component T (h) b/a a (km) b (km)
1. AR = 0.07, c = b, ∆m0
A 15.8580.228+0.226$15.858_{ - 0.228}^{ + 0.226}$ 0.6140.016+0.013$0.614_{ - 0.016}^{ + 0.013}$ 1.1240.013+0.015$1.124_{ - 0.013}^{ + 0.015}$ 0.6900.008+0.009$0.690_{ - 0.008}^{ + 0.009}$
B 3.3660.026+0.036$3.366_{ - 0.026}^{ + 0.036}$ 0.8550.030+0.030$0.855_{ - 0.030}^{ + 0.030}$ 0.6700.013+0.013$0.670_{ - 0.013}^{ + 0.013}$ 0.5730.011+0.011$0.573_{ - 0.011}^{ + 0.011}$
2. AR = 0.05, c = b, ∆m0
A 15.8610.218+0.258$15.861_{ - 0.218}^{ + 0.258}$ 0.6090.014+0.014$0.609_{ - 0.014}^{ + 0.014}$ 1.3360.016+0.017$1.336_{ - 0.016}^{ + 0.017}$ 0.8130.010+0.010$0.813_{ - 0.010}^{ + 0.010}$
B 3.3650.028+0.035$3.365_{ - 0.028}^{ + 0.035}$ 0.8550.032+0.029$0.855_{ - 0.032}^{ + 0.029}$ 0.7960.015+0.016$0.796_{ - 0.015}^{ + 0.016}$ 0.6800.014+0.013$0.680_{ - 0.014}^{ + 0.013}$
3. AR = 0.10, c = b, ∆m0
A 15.8490.224+0.232$15.849_{ - 0.224}^{ + 0.232}$ 0.6170.014+0.014$0.617_{ - 0.014}^{ + 0.014}$ 0.9330.011+0.011$0.933_{ - 0.011}^{ + 0.011}$ 0.5750.007+0.007$0.575_{ - 0.007}^{ + 0.007}$
B 3.3700.029+0.034$3.370_{ - 0.029}^{ + 0.034}$ 0.8590.029+0.029$0.859_{ - 0.029}^{ + 0.029}$ 0.5570.011+0.011$0.557_{ - 0.011}^{ + 0.011}$ 0.4790.009+0.009$0.479_{ - 0.009}^{ + 0.009}$
4. AR = 0.07, c = b, ∆m0 − 0.2
A 15.8570.220+0.223$15.857_{ - 0.220}^{ + 0.223}$ 0.5890.015+0.015$0.589_{ - 0.015}^{ + 0.015}$ 1.1160.015+0.015$1.116_{ - 0.015}^{ + 0.015}$ 0.6570.009+0.009$0.657_{ - 0.009}^{ + 0.009}$
B 3.3660.026+0.037$3.366_{ - 0.026}^{ + 0.037}$ 0.8700.026+0.028$0.870_{ - 0.026}^{ + 0.028}$ 0.7010.012+0.012$0.701_{ - 0.012}^{ + 0.012}$ 0.6100.010+0.011$0.610_{ - 0.010}^{ + 0.011}$
5. AR = 0.07, c = b, ∆m0 + 0.2
A 15.8540.226+0.229$15.854_{ - 0.226}^{ + 0.229}$ 0.6330.015+0.013$0.633_{ - 0.015}^{ + 0.013}$ 1.1370.012+0.014$1.137_{ - 0.012}^{ + 0.014}$ 0.7190.009+0.008$0.719_{ - 0.009}^{ + 0.008}$
B 3.3660.027+0.038$3.366_{ - 0.027}^{ + 0.038}$ 0.8400.035+0.034$0.840_{ - 0.035}^{ + 0.034}$ 0.6390.014+0.015$0.639_{ - 0.014}^{ + 0.015}$ 0.5640.013+0.013$0.564_{ - 0.013}^{ + 0.013}$
6. AR = 0.07, c/a = 0.3, ∆m0
A 15.8690.234+0.229$15.869_{ - 0.234}^{ + 0.229}$ 0.6150.016+0.013$0.615_{ - 0.016}^{ + 0.013}$ 1.6330.008+0.008$1.633_{ - 0.008}^{ + 0.008}$ 1.0050.027+0.022$1.005_{ - 0.027}^{ + 0.022}$
B 3.3640.027+0.035$3.364_{ - 0.027}^{ + 0.035}$ 0.8560.031+0.030$0.856_{ - 0.031}^{ + 0.030}$ 0.6710.013+0.013$0.671_{ - 0.013}^{ + 0.013}$ 0.5750.011+0.011$0.575_{ - 0.011}^{ + 0.011}$

Notes. T is the sidereal rotation period, a, b, c are the semi-axes of an ellipsoidal asteroid (cb < a, c is arranged along the rotation axis, if b = c we have to do with a spheroid prolonged lengthwise the semi-axis a), AR is the geometric albedo of the object in R photometric band, and ∆m0 is the original magnitude difference of the mean magnitudes of components B and A (∆m0 = mBmA) taken from Agarwal et al. (2020).

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