& Gaia2018\
Spectral type & & M1V & Ga2014\
B & \[mag\] & 12.45$\pm$0.19 & Ho2000\
V & \[mag\] & 11.02$\pm$0.06 & Ho2000\
B$_A$ & \[mag\] & 12.460$\pm$0.025 & He2016\
V$_A$ & \[mag\] & 11.005$\pm$0.018 & He2016\
g$_A$ & \[mag\] & 11.752$\pm$0.032 & He2016\
r$_A$ & \[mag\] & 10.416$\pm$0.028 & He2016\
i$_A$ & \[mag\] & 9.675 & He2016\
W$_1$ & \[mag\] & 6.928$\pm$0.060 & Cu2013\
W$_2$ & \[mag\] & 6.984$\pm$0.020 & Cu2013\
W$_3$ & \[mag\] & 6.906$\pm$0.016 & Cu2013\
W$_4$ & \[mag\] & 6.897$\pm$0.074 & Cu2013\
T && 9.2298$\pm$0.0073 & St2018\
J & &7.941$\pm$0.019 & Cu2003\
H & &7.320$\pm$0.053 & Cu2003\
K$_s$ & &7.082$\pm$0.031 & Cu2003\
B$_p$ & &11.2811$\pm$0.0016 & Gaia2018\
G & & 10.2316$\pm$0.0008 & Gaia2018\
R$_p$ & &9.2523$\pm$0.0011 & Gaia2018\
$\pi$ & \[mas\] & 39.762$\pm$0.038 & Gaia2018\
Distance & \[pc\] & 25.150 $\pm$ 0.024 & Gaia2018\
$\mu_\alpha$ & \[mas/yr\] & -319.96$\pm$0.10 & Gaia2018\
$\mu_\delta$ & \[mas/yr\] & -127.78$\pm$0.12 & Gaia2018\
$dv_r/dt$ &\[m/s/yr\] & 0.06865$\pm$0.00011 & this work\
M$_s$ & \[M$_\odot$\] & 0.62$\pm$0.03 & Ma2019\
R$_s$ & \[R$_\odot$\] & 0.600 $\pm$0.022 & Sect. \[subsec:stellarparam\]\
T$_{\rm eff}$ & \[K\] & 3800$\pm$70 & Sect. \[subsec:stellarparam\]\
L$_s$ & \[L$_{\odot}$\] & 0.0673$\pm$0.0024 & Sect. \[subsec:stellarparam\]\
${log(g)}$ & \[g/cm$^{-3}$\] &4.04$\pm$0.49 & Sect. \[subsec:stellarparam\]\
$[\mathrm{Fe/H}]$ 