摘要：Figure 5 in the originally published version of the paper incorrectly stated that stars with parallaxes available from the Gaia first data release (DR1) are included in the CTL only if their estimated surface gravity (log g) is consistent with being a dwarf (i.e., log g 4.1). The correct procedure, shown in the corrected Figure 5 below, instead uses the stellar radius as the criterion and includes both dwarfs and subgiants according to the relation shown by the blue curve in the Figure 13 inset (right). This is for the sake of consistency between the parallax-based method and the RPMJ-based method, and this also preserves potentially int eresting subgiant targets as discussed in Section4.3.3.
