Table 2.
continued.
| 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) |  |
 |
 |
 |
 |
| D |  |
 |
 |
 |
 |
| W (d) |  |
 |
 |
 |
 |
| b |  |
 |
 |
 |
 |
| K (km s−1) |  |
 |
 |
 |
 |
| fs | 0 (fixed) | 0 (fixed) |  |
0 (fixed) |  |
| fc | 0 (fixed) | 0 (fixed) |  |
0 (fixed) |  |
| Derived parameters | |||||
| M1 (M⊙) |  |
 |
 |
 |
 |
| R1 (R⊙) |  |
 |
 |
 |
 |
| ρ1(ρ⊙) |  |
 |
 |
 |
 |
| 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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