All Tables

Table 1: Orbital parameters for single-lined systems. Columns 2-9: Parameters of the orbital solution. P: revised period, $T_{\rm tr}$ (OGLE): epoch of the transit (fixed), $P_{\rm OGLE}$ : original OGLE period, $T_{\rm p}$ : epoch of periastron, w: omega angle, K: orbital semi-amplitude, V₀: systemic velocity, e: eccentricity. Column 10: projected rotation velocity from the cross-correlation function.
Table 2: Rotation velocity and radius estimates for primary and secondary components of single-lined suspected binaries without orbits. N: number of spectra; v sin i: projected rotational velocity of the primary; R and r: radius of the eclipsed and eclipsing bodies respectively.
Table 3: Orbital elements and rotation velocities for double-lined and triple-lined systems. Column 2: system components. By convention the eclipsing components are always "a'' and "b''. Columns 3-7: Parameters of the orbital solution. P: revised period, $T_{\rm tr}$ : epoch of the transits (fixed), $P_{\rm OGLE}$ : original OGLE period, K: orbital semi-amplitude, V₀: systemic velocity. The eccentricity was fixed to zero in all cases except for the second system ("cd'') of OGLE-TR-112, where $e=0.55\pm 0.02$ . Column 8: rotation velocity from the cross-correlation function.
Table 4: Number of measurements and rotation velocity for double-lined and triple-lined systems without orbital solution. Column 5 indicates the implied radius in case of synchronised rotation. Uncertainties on the v sin i are of the order of 10 percent. When indicated, the orbital period is twice the OGLE period.
Table 5: Data for objects with no significant orbital signal in phase with the transits. N: number of measurements, v sin i: projected rotation velocity, $\langle\epsilon_{V_r}\rangle$ mean radial velocity uncertainty, rms: dispersion of radial velocity residuals, $m_{\max}$ : upper limit on the mass of a transiting companion. In the case of OGLE-TR-124, the secular drift has been substracted.
Table 6: Data for objects with no detected signal in the CCF. N: number of measurements, $\sigma _{\rm CCF}$ : rms of the CCF continuum, ${\it SNR}$ : signal-to-noise ratio of the spectrum, $v^{\min}_{\sin i}$ : minimum projected rotation velocity compatible with the absence of CCF signal for a single, late-type star.
Table 7: Results of the lightcurve+spectroscopy solution for all objects in our sample. R,r,M,m: radii and masses of the primary and secondary. i: orbital inclination. The last column summarizes the nature of the system, with a number referring to the section where each case is treated. Question marks and brackets denote cases where the resolution is only tentative, colons (":") the values with high uncertainties.
Table 8: Radial velocity measurements (in the barycentric frame) and CCF parameters. Labels a, b and c indicate that several components are present in the CCF.