Table 1:

Fitted and physical parameters found after fitting photometric and spectroscopic data of CoRoT-3b and of HD 189733b.
Parameters (units) CoRoT-3b HD 189733b
Fitted parameters    
D $ 0.004398 ^{\rm + 0.000084}_{- 0.000091}$ $ 0.0200^{\rm + 0.00015}_{- 0.00017} $
K $({\rm m~s}^{-1})$ $ 2169.9 ^{\rm + 35.1}_{- 22.7}$ $ 201.96^{\rm + 1.07 }_{- 0.63 } $
b $(R_{\star})$ $ 0.54 ^{\rm + 0.041}_{- 0.081}$ $ 0.6873 ^{\rm + 0.0047 }_{- 0.0078 } $
W (days) $ 0.1566 ^{\rm + 0.0012}_{- 0.0014 }$ $ 0.07527^{\rm + 0.00020}_{- 0.00037} $
P (days) $ 4.2567994 ^{\rm + 0.0000039}_{- 0.0000031}$ $2.21857312^{\rm + 0.00000036}_{- 0.00000076} $
T0 (bjd) $ 54283.13388 ^{\rm + 0.00026}_{- 0.00022}$ $53988.80339^{\rm + 0.000072}_{- 0.000039} $
$e~\cos(\omega_0)$ $ -0.0083 ^{\rm + 0.0054}_{- 0.0041}$ $0.0038^{\rm +0.0020}_{-0.0020}$
$e~\sin(\omega_0)$ $ 0.000 ^{\rm + 0.021}_{- 0.020}$ $-0.0017^{\rm +0.0024}_{-0.0034}$
$V~\sin(I)~\cos(\beta)$ $ 28.4 ^{\rm + 6.5}_{- 5.6}$ $3.316^{\rm +0.017}_{-0.068}$
$V~\sin(I)~\sin(\beta)$ $ 21.9 ^{\rm + 8.3}_{- 14.1}$ $0.049^{\rm +0.018}_{-0.017}$
$\Gamma$ $({\rm m~s}^{-1}~{\rm yr}^{-1})$ - $ -0.2 ^{\rm + 2.7}_{- 3.9}$
Derived parameters    
$R_{\rm p} / R_{\star}$ $ 0.06632 ^{\rm + 0.00063}_{- 0.00069} $ $ 0.15812 ^{\rm + 0.00046}_{- 0.00052}$
$R_{\star} / a$ $ 0.1257^{\rm + 0.0057 }_{- 0.0064} $ $ 0.1142 ^{\rm + 0.0006}_{- 0.0012} $
$\rho_{\star}$ $(\rho_{\odot})$ $ 0.372^{\rm + 0.064 }_{- 0.047} $ $ 1.831 ^{\rm + 0.059}_{- 0.029}$
$R_{\star}$ $(R_{\odot})$ 1.5400.0830.078 $ 0.766 ^{\rm + 0.007}_{- 0.013} $
$M_{\star}$ $(M_{\odot})$ $ 1.359^{\rm + 0.059 }_{- 0.043}$ $ 0.823 ^{\rm + 0.022}_{- 0.029} $
$V~\sin(I)$ $({\rm km~s}^{-1})$ $ 35.8 ^{\rm + 8.2}_{- 8.3}$ $ 3.316 ^{\rm + 0.017}_{- 0.067}$
$R_{\rm p} / a$ $ 0.00834^{\rm + 0.00042 }_{- 0.00050} $ $ 0.01805 ^{\rm + 0.00011}_{- 0.00025} $
$R_{\rm p}$ (RJ) $ 0.9934^{\rm + 0.058}_{- 0.058} $ $ 1.178 ^{\rm + 0.016}_{- 0.023} $
$M_{\rm p}$ (MJ) $21.23 ^{\rm + 0.82}_{- 0.59}$ $ 1.138 ^{\rm + 0.022}_{- 0.025} $
a (AU) $ 0.05694 ^{\rm + 0.00096}_{- 0.00079} $ $ 0.03120 ^{\rm + 0.00027}_{- 0.00037} $
i $(^{\circ})$ $ 86.10 ^{\rm + 0.73}_{- 0.52} $ $ 85.508 ^{\rm + 0.10}_{- 0.05} $
e $ 0.008 ^{\rm + 0.015}_{- 0.005} $ $ 0.0041 ^{\rm + 0.0025}_{- 0.0020} $
$\omega_0$ $(^{\circ})$ $179 ^{\rm + 170}_{- 170}$ $ -24.1 ^{\rm + 33.9}_{- 34.5}$
$\beta$ $(^{\circ})$ $37.6^{\rm +10.0}_{-22.3}$ $ 0.85 _{- 0.32}^{\rm + 0.28}$
$\gamma$ Velocities ( ${\rm m~s}^{-1}$)    
Sophie -56182.46 -2273.59
TLS -56652.08  
Keck - -15.84
Harps -56156.08 -2161.14
Harps (RM) -56160.84 -2191.92
  - -2225.44
  - -2204.07
Normalisation factors    
CoRoT 0.9999998 -
FLWO 1.2 m z-band - 0.99974
T10 (b+y)/2 band - 0.99977
MAGNUM 2 m V-band - 0.99979
Wise 1 m I-band - 0.99977
$\chi^2_{\rm reduced}$ $1.17\pm0.08$ $ 1.21\pm 0.03$
The reduced $\chi ^2$ were calculated with 414 degrees of freedom for CoRoT-3b and 2890 for HD 189773b.
Nota Bene: $\beta = -\lambda$; $\beta$ is used since the first reference of a projected spin-orbit angle was named thus, in Hosokawa (1953). $V~\sin(I)$s are probably overestimated, see Sect. 4 for details.

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