All Tables

Table 1: $\it JHK$ differential photometry of the eclipsing component RXJ 0529.4+0041 A with respect to component B, with running Heliocentric Julian Day (-2, 400, 000). The corresponding orbital phase is computed using the new ephemeris given in Sect. 4.1 (only in electronic form).
Table 2: Absolute photometry for the visual components, A (eclipsing binary) and B (companion), of RXJ 0529.4+0041. All magnitudes involving component A refer to out-of-eclipse phases, thus providing the mean maximum-light level.
Table 3: Orbital elements and stellar parameters of RXJ 0529.4+0041A from the spectroscopic orbits. The Epoch T₀ refers to the time of maximum velocity of the primary.
Table 4: Best-fit parameters from model solutions of the $\it JHK$ light-curves with 2 spots on the primary component and $\it BV,JHK$ (rectified) light-curves, corresponding to an effective temperature of the Primary component of 5200 K. The quoted uncertainties are formal mean standard errors to the solution.
Table 5: Adopted stellar physical parameters for the eclipsing components of RXJ 0529.4+0041A.
Table 6: Fundamental stellar properties for the components of RX J0529.4+0041A, NTT 045251+3016 (Steffen et al. 2001) and V1174 Ori (Stassun et al. 2004).
Full Version
Table 1: JHK differential photometry of the eclipsing component RXJ 0529.4+0041 A with respect to component B, with running Heliocentric Julian Day (-2,400,000). The corresponding orbital phase is computed using the new ephemeris given in Sec. 4.1 (Only in electronic form.)