Astronomy & Astrophysics

All Tables

Table 1: Radial velocity measurements (in the barycentric frame) and CCF parameters. Labels a and b indicate that 2 components are present in the CCF. BJD in the range [522-557], [750-798] and [809-812] correspond respectively to UVES, FLAMES and HARPS measurements.
Table 2: Parameters from the spectroscopic analysis. Rotation velocities v sin i are computed from the analysis of the CCF. $T_{\rm eff}$ , $\log{g}$ , [Fe/H]: temperature, gravity and metallicity are computed from the analysis of the spectral lines in case of low v sin i. For high rotation, $T_{\rm eff}$ was estimated roughly by comparison with a synthetic spectrum. It was not possible to determine the spectral types of binaries (identified with label a and b) that include two moving components in the spectra.
Table 3: Parameters from the transit light curve fit: $\overline {r}$ ratio of the radii of the primary and secondary bodies, V_T/R transit velocity in units of the radius of the primary, b impact parameter, P revised period according to the radial velocity measurements. We deliberately do not provide the results for the 4 unsolved cases suspected to be false positives, OGLE-TR-19, 48, 49 and 58. For the two cases of SB2, stellar parameters were deduced from the spectroscopic orbits and the rotational velocities.
Table 4: Orbital parameters of the low-mass-star-transiting companions, the grazing eclipsing binaries and the triple systems. For the triple systems, the component a corresponds here to the contaminating third body with fixed parameters and component b to the primary of an eclipsing binary with fitted parameters. ¹ Residuals of OGLE-TR-17 without and with eccentricity (e=0.074). ² This value corresponds to the anti-transit epoch, the revised value is 74.65125.
Table 5: Orbital parameters of planetary candidates, unsolved cases and false positives.
Table 6: Summary table with the physical parameters r, R, m and M, the orbital angle i and the identification of the system.