|Spectroscopic measurements of primary star|
|log g1 (dex)|
|v sin i1 (km s−1)||<5||<5|
|Parameters from bagemass iteration|
|System age (Gyr)|
|Free parameters in MCMC sampling|
|K (km s−1)|
|fs||0 (fixed)||0 (fixed)||0 (fixed)|
|fc||0 (fixed)||0 (fixed)||0 (fixed)|
|log g2 (cgs)|
|e||0 (fixed)||0 (fixed)||0 (fixed)|
|ω (deg)||0 (fixed)||0 (fixed)||0 (fixed)|
|Prot, primary (d)(*)||–||–|
|Instruments and fit properties|
|Instruments||Eu, COR||TR, COR||TR, SP, W, COR||TR, COR||Eu, COR|
|Radial velocity baseline||cubic time||–||–||–|
|Flux baseline||linear time||–||–||linear time||lin. centroid-y(**)|
Notes. The high precision of the orbital period of EBLM J2017+02Ab and EBLM J1115-36Ab is due to the use of the WASP discovery light curves in the fit, together with radial velocities and transits observed with TRAPPIST. (*)Assuming a negligible inclination of the primary star spin axis. (**)Linear baseline in the y-coordinate of the centroid position on the detector.
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