Notes. Dataset labels refers to Table 1. The models were obtained by solving the inverse problem for the Roche model with an accretion disk around the more massive (hotter) gainer in a critical nonsynchronous rotation regime (Djurašević 1992a,b, 1996). Mean values are also given. FIXED PARAMETERS: q = ℳ_c/ℳ_h = 0.52 – mass ratio of the components; T_c = 22 700 K – temperature of the less massive (cooler) donor; F_c = 1.0 – filling factor for the critical Roche lobe of the donor; f_c = 1.00 – nonsynchronous rotation coefficients of the donor; F_h = R_h/R_zc – filling factor for the critical nonsynchronous lobe of the hotter, more massive gainer (ratio of the stellar polar radius to the critical Roche lobe radius along the z-axis for a star in a critical nonsynchronous rotation regime); β_h, c = 0.25 – gravity-darkening coefficients of the components; A_h, c = 1.0 – albedo coefficients of the components. Note: Origin of the photometric observations; photometric band; q – mass ratio of the components;i – orbit inclination (in arc degrees); F_d = R_d/R_yc – disk dimension factor (the ratio of the disk radius to the critical Roche lobe radius along y-axis); T_d – disk-edge temperature; d_e, d_c, – disk thicknesses (at the edge and at the center of the disk, respectively) in the units of the distance between the components; a_T – disk temperature distribution coefficient; f_g – nonsynchronous rotation coefficient of the more massive gainer (in the synchronous rotation regime); T_h – temperature of the more-massive (hotter) gainer; A_hs, bs = T_hs, bs/T_d – hot and bright spots’ temperature coefficients; θ_hs, bs and λ_hs, bs – spots’ angular dimensions and longitudes (in arc degrees, the longitude is measured in the direction of the orbital motion); θ_rad – angle between the line perpendicular to the local disk edge surface and the direction of the hot-spot maximum radiation; Ω_h, c – dimensionless surface potentials of the hotter gainer and cooler donor; ℳ_〈,⌋[ℳ_⊙], ℛ_〈,⌋[ℛ_⊙] – stellar masses and mean radii of stars in solar units; log g_h, c – logarithm (base 10) of the system components effective gravity; – absolute stellar bolometric magnitudes; a_orb [R_⊙], ℛ_⌈[ℛ_⊙], d_e[R_⊙], d_c[R_⊙] – orbital semimajor axis, disk radius, and disk thicknesses at its edge and center, respectively, given in solar units.