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Table 2.


Parameter J1038−37 J1013+01 J1115−36 J0339+03 J1403−32
Spectroscopic measurements of primary star
Teff (K)
[Fe/H] (dex)
log g1 (dex)
v sin i1 (km s−1) <5 <5
Parameters from bagemass iteration
System age (Gyr)
M1 (M)
Free parameters in MCMC sampling
P (d)
t0 (d)
W (d)
K (km s−1)
fs 0 (fixed) 0 (fixed) 0 (fixed)
fc 0 (fixed) 0 (fixed) 0 (fixed)
Derived parameters
M1 (M)
R1 (R)
M2 (M)
R2 (R)
log g2 (cgs)
fm (M)
e 0 (fixed) 0 (fixed) 0 (fixed)
a (au)
ω (deg) 0 (fixed) 0 (fixed) 0 (fixed)
i (deg)
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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