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The mass and radius of the unseen m dwarf companion in the single lined eclipsing binary HAT TR 205 013

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Figure

Fig. 1.—Mass-radius diagram for 10 stars in five double-lined eclipsing binaries, each composed of two M dwarfs and with errors better than 3%.
Fig. 2.—Phase-folded HATnet light curve for HAT-TR-205-013.
Fig. 3.—Velocity curve for our orbital solution for HAT-TR-205-013, to- to-gether with the individual observed velocities
TABLE 6 Light-Curve Fit Results
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