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Table 3:

WD solutions from the 1988 light curve observations (261 per band). See Table 2.
  y b v u

i ($^\circ$)
89.56 89.55 89.56 89.40
  $\pm $3 $\pm $3 $\pm $3 $\pm $2

$\Omega_{\rm p}$

14.495 14.470 14.455 14.477
  $\pm $23 $\pm $20 $\pm $25 $\pm $27

$\Omega_{\rm s}$

14.656 14.639 14.707 14.623
  $\pm $27 $\pm $25 $\pm $14 $\pm $19

$r_{\rm p}$

0.0738 0.0739 0.0740 0.0739
$r_{\rm s}$ 0.0604 0.0605 0.0602 0.0606
k 0.818 0.819 0.814 0.820
$r_{\rm p} + r_{\rm s}$ 0.1342 0.1344 0.1342 0.1345
$T_{\rm s}$ (K) 4940 4959 4897 4914
  $\pm $4 $\pm $4 $\pm $4 $\pm $6

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

0.282 0.250 0.195 0.163

LO1 ($^\circ$)

107.9 118.8 116.5 122.0
  $\pm $1.6 $\pm $1.2 $\pm $1.4 $\pm $2.6

AR1 ($^\circ$)

25.9 28.7 31.8 31.1
  $\pm $0.4 $\pm $0.4 $\pm $0.4 $\pm $0.6

LO2 ($^\circ$)

202.4 212.1 209.9 214.9
  $\pm $1.7 $\pm $1.6 $\pm $1.6 $\pm $2.4

AR2 ($^\circ$)

25.7 23.8 28.6 29.9
  $\pm $0.6 $\pm $0.7 $\pm $0.7 $\pm $0.9

$\sigma$ (mmag.)

6.5 5.9 6.8 9.7

Source LaTeX | All tables | In the text

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