- Table 1:
Orbital parameters for single-lined systems.
Columns 2-9: Parameters of the orbital solution.
*P*: revised period, (OGLE): epoch of the transit (fixed), : original OGLE period, : epoch of periastron,*w*: omega angle,*K*: orbital semi-amplitude,*V*_{0}: 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, : epoch of the transits (fixed), : original OGLE period,*K*: orbital semi-amplitude,*V*_{0}: systemic velocity. The eccentricity was fixed to zero in all cases except for the second system ("cd'') of OGLE-TR-112, where . 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, mean radial velocity uncertainty, rms: dispersion of radial velocity residuals, : 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, : rms of the CCF continuum, : signal-to-noise ratio of the spectrum, : 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.