Table 1.

Optical photometric periods in J1820 (from Fig. 2).

Day Nos.bFreq. (d−1)P (d)aNotes
87–1021.422410.70303(1)Psh
103–1121.447970.69062(5)
113–1601.453010.68823(2)PW
113–2531.453010.68823(5)PW
Day Nos.bFreq. (d−1)P (d)aNotes
87–1021.422410.70303(1)Psh
103–1121.447970.69062(5)
113–1601.453010.68823(2)PW
113–2531.453010.68823(5)PW

Notes. a1σ uncertainties in last digit given in parentheses.

bThese are the same time intervals as used in Fig. 2.

Note that Porb  = 0.68549(1) d (freq. 1.4588 d−1; Torres et al. 2019).

Table 1.

Optical photometric periods in J1820 (from Fig. 2).

Day Nos.bFreq. (d−1)P (d)aNotes
87–1021.422410.70303(1)Psh
103–1121.447970.69062(5)
113–1601.453010.68823(2)PW
113–2531.453010.68823(5)PW
Day Nos.bFreq. (d−1)P (d)aNotes
87–1021.422410.70303(1)Psh
103–1121.447970.69062(5)
113–1601.453010.68823(2)PW
113–2531.453010.68823(5)PW

Notes. a1σ uncertainties in last digit given in parentheses.

bThese are the same time intervals as used in Fig. 2.

Note that Porb  = 0.68549(1) d (freq. 1.4588 d−1; Torres et al. 2019).

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