Table 3: Characteristics of the multi-sinusoidal fit of individual runs of observations of BG CMi (continuation of Table 2).
T₀₇-2 400 000 $\langle I\rangle$ R₇ $\Delta m$

V 52635.32067 $\pm$ 0.00047 3.492 0.320: $\pm$ 0.126

V 52638.30276 $\pm$ 0.00022 3.861 0.444 $\pm$ 0.056

V 53035.10202 $\pm$ 0.00020 3.536 0.457 $\pm$ 0.055 0 $.\!\!^{\rm m}$ 46

V 53036.19093 $\pm$ 0.00021 3.832 0.385 $\pm$ 0.048 0 $.\!\!^{\rm m}$ 39

V 53053.02230 $\pm$ 0.00018 3.597 0.433 $\pm$ 0.047 0 $.\!\!^{\rm m}$ 38

V 53383.09882 $\pm$ 0.00777 3.508 $0.284:\pm0.176$

V 53384.14518 $\pm$ 0.00057 3.976 $0.802:\pm0.297$

V 53386.06917 $\pm$ 0.00037 3.524 $0.561\pm0.126$ 0 $.\!\!^{\rm m}$ 45

V 53405.04680 $\pm$ 0.00043 3.440 $0.467\pm0.117$ 0 $.\!\!^{\rm m}$ 44

R 53383.09798 $\pm$ 0.00078 277750 $34337\pm14845$

R 53384.14560 $\pm$ 0.00067 311765 $57053\pm22282$

R 53386.06915 $\pm$ 0.00036 276381 $41497\pm8917$ 0 $.\!\!^{\rm m}$ 47

R 53405.04708 $\pm$ 0.00044 267748 $34647\pm8946$ 0 $.\!\!^{\rm m}$ 43

**Table 3:** Characteristics of the multi-sinusoidal fit of individual runs of observations of BG CMi (continuation of Table 2).
T₀₇-2 400 000	$\langle I\rangle$	R₇	$\Delta m$
V 52635.32067 $\pm$ 0.00047	3.492	0.320: $\pm$ 0.126
V 52638.30276 $\pm$ 0.00022	3.861	0.444 $\pm$ 0.056
V 53035.10202 $\pm$ 0.00020	3.536	0.457 $\pm$ 0.055	0 $.\!\!^{\rm m}$ 46
V 53036.19093 $\pm$ 0.00021	3.832	0.385 $\pm$ 0.048	0 $.\!\!^{\rm m}$ 39
V 53053.02230 $\pm$ 0.00018	3.597	0.433 $\pm$ 0.047	0 $.\!\!^{\rm m}$ 38
V 53383.09882 $\pm$ 0.00777	3.508	$0.284:\pm0.176$
V 53384.14518 $\pm$ 0.00057	3.976	$0.802:\pm0.297$
V 53386.06917 $\pm$ 0.00037	3.524	$0.561\pm0.126$	0 $.\!\!^{\rm m}$ 45
V 53405.04680 $\pm$ 0.00043	3.440	$0.467\pm0.117$	0 $.\!\!^{\rm m}$ 44
R 53383.09798 $\pm$ 0.00078	277750	$34337\pm14845$
R 53384.14560 $\pm$ 0.00067	311765	$57053\pm22282$
R 53386.06915 $\pm$ 0.00036	276381	$41497\pm8917$	0 $.\!\!^{\rm m}$ 47
R 53405.04708 $\pm$ 0.00044	267748	$34647\pm8946$	0 $.\!\!^{\rm m}$ 43

Source LaTeX | All tables | In the text

	1 Introduction
	2 Observations and comparison stars
	3 Separation of spin and orbital variability
	4 Color variability with the phase of orbital and spin period
	5 194-minute orbital period
	6 Variability of the spin period
	7 Conclusions
	References