Companion mass and host star effective temperature T_eff for transiting brown dwarfs and low-mass stellar companions (gray circles) with the five new companions of this work shownwith red error bars. We also display giant planets that have both RV and transit data from the NASA exoplanet archive (https://exoplanetarchive.ipac.caltech.edu) (1089 giant planets) with blue circles. The circles are inversely sized by the companion period to highlight a higher proportion of brown dwarfs and low-mass stars in close orbit around F dwarfs. The histograms at the top display the number of relative companions in 500 K T_eff bins. The vertical dashed green lines display approximate T_eff borders of stellar types.