Notes. Rotation periods are adopted from Pope et al. (2021) unless otherwise noted. All other values are from this work unless otherwise noted. The cross-validation uncertainties for the stellar effective temperature, log g, and the metallicity are σ_Teff = 59 K, σ_{log g} = 0.04, and σ_Fe/H = 0.16. The method used to derive v sin i_⋆ is annotated, where α is a result from HPF-SpecMatch, β is obtained through the CCF method and γ is obtained from the broadening function. References are annotated with letters a-d. ⁽¹⁾Targets shortened for space: 2MASS J09481615+5114518 (2M J094), 2MASS J14333139+3417472 (2M J143), LSPM J1024+3902E (LSPM J102), and 2MASS J10534129+5253040 (2M J105). ⁽²⁾The highly broadened lines of target 2MASS J14333139+3417472 makes it difficult for HPF-SpecMatch to find matching spectra, and thus produces highly uncertain results. Therefore, we here show the stellar properties listed in the Tess Input Catalog. ⁽³⁾G 240-45 and 2MASS J10534129+5253040 are likely binaries, but do not show obvious double lines and so we report the HPF-SpecMatch results here. We suggest caution in interpreting these results. ^a Pope et al. (2021), ^b This work, ^c Morin et al. (2008), ^d Newton et al. (2017), ^e Callingham et al. (2021b).