Rotational variation in the He i EW and the mass accretion rate. The mass accretion rate errors come from the relation between the He i (5876 Å) luminosity and the accretion luminosity by Fang et al. (2009). Filled symbols are from HARPS data and open ones from ESPaDOnS. Different colors represent different rotational cycles identified as the integer part of the observational phase in Table 1: black – cycle 0, green – cycle 1, red – cycle 2, aqua – cycle 3, dark blue – cycle 4, pink – cycle 5.