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Table 4

Physical and geometrical parameters of the CoRoT-33 system.

Determined from photometry

Epoch of transit T0 [BJD−2 450 000] 6676.3992 ± 0.0037
Epoch of periastron T0 [BJD−2 450 000] 6677.7130 ± 0.0140
Orbital period (days) 5.819143 ± 0.000018
Duration of the transit (h) 1.4 h
Depth of the transit (%) 0.28%

Determined from RV measurements

Orbital eccentricity e 0.0700 ± 0.0016
Argument of periastron ω [deg] 179.3 ± 0.87
RV semi-amplitude K [ km s-1] 7.0609 ± 0.0094
Systemic velocity Vγ [ km s-1], HARPS 21.5375 ± 0.0158
Systemic velocity Vγ [ km s-1], FIES 21.5544 ± 0.0222
O−C residualsa [ m s-1] 36

Determined from spectral analysis of the star

Teff [K] 5225 ± 80
log g [cgs] 4.4 ± 0.1
[Fe/H] 0.44 ± 0.1
[Ni/H] 0.4 ± 0.1
[V/H] 0.4 ± 0.1
[Mg/H] 0.4 ± 0.1
[Ca/H] 0.3 ± 0.1
[Si/H] 0.2 ± 0.1
vsini [km s-1] 5.7 ± 0.4
Spectral type G9V
V mic 0.86 ± 0.1 km s-1
2.7 ± 0.6 km s-1

Determined from light curve modeling

a / R star 13.23 ± 1.17
b 1.04 ± 0.06
iplanet [deg] 85.5 ± 0.5
k 0.12 ± 0.04
Contamination [%] 13 ± 4c

Combined results

Stellar mass Mst [solar] 0.86
Stellar radius Rst [solar] 0.94
Stellar age [Gyr] >4.6
Orbital semi-major axis a [AU] 0.0579d
Brown dwarf mass MBD [MJ] 59.0
Brown dwarf radius RBD [RJ] 1.10 ± 0.53
Brown dwarf mean density ρBD [g cm-3] 55 ± 29

Notes. Inclination (i) was calculated from the a/Rstar ratio and from the impact parameter b. The parameter M1/3/R can be calculated from the orbital period and from the a/Rstar value (see e.g. Winn 2010).

(a)

Root mean square of the residuals of the RV curve.

(b)

Fixed at this value, based on the calibration by Doyle et al. (2014).

(c)

Calculated from period and masses via Kepler’s third law, not from RV.

(d)

From modeling results.

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