All Tables

Table 1: Journal of new $U\!B{}V$ photoelectric observations of V360 Lac. Observing stations are identified by their file numbers used in the Praha/Ondrejov data archives (see column "File No.'') as follows:
1... Hvar 0.65-m reflector, EMI6256 tube; 4... Ondrejov 0.65-m reflector, EMI6256 tube; 30... San Pedro Mártir 0.84-m reflector, Cuenta-pulsos photon-counting photometer with RCA 31034 tube; 61... Hipparcos satellite H_p broadband photometry transformed to Johnson V and B magnitudes.
Table 2: Comparison and check stars used by various photometric observers of V360 Lac and their $U\!B{}V$ magnitudes adopted here, based on the latest standardization of Hvar and SPM all-sky $U\!B{}V$ observations.
Table 3: Individual $U\!B{}V$ observations of V360 Lac . Data from individual stations are identified by their numbers in column "station'', identical to those given in Table 1, and filters are coded as follows: 3 = V, 4 = B, and 5 = U. Original (O) observations, smoothed values derived by the HEC13 program (C) and residuals after smoothing ( $\rm O{-}C$ ) are all tabulated.
Table 4: Mean RVs of the primary and secondary from the KOREL solutions, derived via cross-correlation of the disentangled line profiles with the individual spectra.
Table 5: Orbital solutions derived with KOREL (see the text for details).The orbital period was fixed at 10 $^{\rm d}\!\!.$ 085408 derived in Paper 17. $T_{\rm sc}$ denotes the epoch of the superior conjunction in RJD-52 000.
Table 6: System parameters used to simulate photometric observations and spectra for the system model.