& & 0.04$\pm$0.17 & Ne2014\
${log(R^\prime_{HK})}$ & & -4.562$\pm$0.043 & As2017A\
P$_{\text{rot}}$ & \[days\] & $29.8\pm1.3$ & Sect. \[subsec:rotation\]\

Gaia2018 – @Gaia2018; Ga2014 – @Gaidos2014; Ho2000 – @Tycho-2; H22016 – @apass; Cu2013 – @wise; St2018 – @StassunTIC:2018; Cu2003 – @Cutri2003; Ma2019 – @Mann:2019; Ne2014 – @Neves2014; As2017a – @Astudillo2017a

L 168-9, also known as CD-60 8051, HIP 115211, 2MASS J23200751-6003545, with the entry 234994474 of the TESS Input Catalog (TIC) or 134 of the Tess Object of Interest (TOI) list, is a red dwarf of spectral type M1V. It appears in the southern sky, and resides at a distance of 25.150$\pm$0.024 $pc$ from the Sun [@Gaidos2014; @Gaia2018]. Table \[tab:stellarprop\] lists the key parameters of the star, namely its position, visual and near-infrared apparent magnitudes, parallax, proper motion, secular acceleration, and its essential physical properties.

Derived stellar properties {#subsec:stellarparam}
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We performed an analysis of the broadband spectral energy distribution (SED) together with the [*Gaia*]{} DR2 parallax in order to determine an empirical measurement of the stellar radius, following the procedures described by @Stassun:2016 [@Stassun:2017; @Stassun:2018]. We took the $B_T V_T$ magnitudes from [*Tycho-2*]{}, the $BVgri$ magnitudes from APASS, the $JHK_S$ magnitudes from [*2MASS*]{}, the W1–W4 magnitudes from [*WISE*]{}, and the 