Table 18: Photometric solutions for WZ Oph from the WD code adopting linear limb darkening coefficients by van Hamme (1993); see Table 17. Gravity darkening exponents of 0.33 and bolometric albedo coefficients of 0.5 were adopted, as appropriate for convective envelopes. $T_{\rm {eff},p}$ was assumed to be 6165 K.
  y b v u
i   ($^\circ$) 89.11 89.11 89.08 89.14
  $\pm$1 $\pm$1 $\pm$2 $\pm$3

$\Omega_{\rm p}$

 11.454 11.510 11.554 11.444
  $\pm$11 $\pm$15 $\pm$14 $\pm$32

$\Omega_{\rm s}$

 11.334 11.299 11.310 11.276
  $\pm$12 $\pm$14 $\pm$17 $\pm$30

$r_{\rm p}$

 0.0957 0.0952 0.0948 0.0958

$r_{\rm s}$

 0.0963 0.0967 0.0966 0.0969

k

 1.007 1.016 1.019 1.012

$r_{\rm p} + r_{\rm s}$

 0.1920 0.1919 0.1914 0.1927

$T_{\rm {eff},s}$

 6149 6141 6141 6121
  $\pm$2 $\pm$2 $\pm$3 $\pm$5

$L_{\rm s}/L_{\rm p}$

 1.0023 1.0126 1.0180 0.9936

$\sigma$   (mag)

 0.0053 0.0057 0.0065 0.0104


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