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This article has an erratum: [https://doi.org/10.1051/0004-6361/200810284e]

 

 

Table 6:

Comparison of our results (NGBR) with the light-curves solutions of Wyithe & Wilson (2001,2002, WW01, WW02) and Graczyk (2003, dG03).

Object 		Ref. Model q $R_{\rm P}/a$ $R_{\rm S}/a$ $i (\hbox{$^\circ$ })$ e $(L_{\rm S}/L_{\rm P})_{I}$ Fe l3,I
4 117831 NGBR d $0.981\pm0.013$ $0.261\pm0.008$ $0.287\pm0.008$ $78.2\pm0.4$ 0 1.175 0.599 0
  WW02 sd $0.157\pm0.054$ $0.357\pm0.032$ $0.209\pm0.021$ $77.9\pm2.1$ $0.049\pm0.019$ 0.372 0.853 0
4 163552 NGBR d $0.952\pm0.015$ $0.339\pm0.011$ $0.305\pm0.010$ $80.9\pm0.2$ 0 0.798 0.797 $0.119\pm0.006$
  dG03 d $0.98\pm0.09 $ $0.338\pm0.006$ $0.326\pm0.008$ $85.4\pm0.9$ 0 0.951 0.895 $0.263\pm0.007$
  WW02 sd $0.207\pm0.010$ $0.383\pm0.004$ $0.234\pm0.003$ $82.8\pm0.7$ $0.004\pm0.002$ 0.397 1.051 0
4 175333 NGBR d $0.781\pm0.014$ $0.237\pm0.008$ $0.203\pm0.007$ $80.4\pm0.5$ $0.022\pm0.007$ 0.582 0.675 0
  WW01 d 1.0 $0.253\pm0.009$ $0.143\pm0.007$ $85.0\pm1.5$ $0.012\pm0.003$   1.080 0
5 016658 NGBR d $0.889\pm0.011$ $0.320\pm0.011$ $0.255\pm0.010$ $80.3\pm0.2$ 0 0.609 0.798 0
  WW01 d 1.0 $0.345\pm0.007$ $0.200\pm0.004$ $85.7\pm1.3$ $0.002\pm0.002$   1.175 0
5 038089 NGBR d $0.899\pm0.011$ $0.273\pm0.004$ $0.226\pm0.003$ $77.1\pm0.2$ 0 0.693 0.609 0
  dG03 d $1.12 \ ^{\rm a}$ $0.246\pm0.009$ $0.255\pm0.007$ $76.8\pm1.9$ 0 1.053 0.554 0
5 196565 NGBR d $0.803\pm0.007$ $0.200\pm0.005$ $0.150\pm0.005$ $83.5\pm0.2$ $0.138\pm0.006$ 0.43 0.789 0
  WW01 d 1.0 $0.204\pm0.006$ $0.116\pm0.003$ $88.7\pm2.5$ $0.085\pm0.002$   1.282 0
5 266015 NGBR sd $0.441\pm0.005$ $0.332\pm0.005$ $0.310\pm0.005$ $78.5\pm0.1$ 0 0.494 0.714 0
  WW02 sd $1.014\pm0.051$ $0.183\pm0.003$ $0.357\pm0.004$ $80.8\pm0.4$ $0.000\pm0.002$ 2.564 1.039 0
5 266131 NGBR d $0.864\pm0.013$ $0.281\pm0.010$ $0.242\pm0.009$ $83.5\pm0.2$ $0.042\pm0.001$ 0.647 0.847 0
  WW01 d 1.0 $0.332\pm0.008$ $0.216\pm0.009$ $85.1\pm1.5$ $0.003\pm0.003$   1.071 0
5 283079 NGBR d $1.003\pm0.013$ $0.243\pm0.007$ $0.242\pm0.007$ $87.7\pm0.3$ 0 0.987 0.918 0
  WW01 d 1.0 $0.272\pm0.006$ $0.233\pm0.007$ $88.5\pm1.8$ $0.001\pm0.001$   1.028 0

Notes. The following parameters are listed: model of the system, mass ratio, relative radii, inclination, eccentricity, I luminosity ratio, eclipse parameter (see Eq. (2) in WW01) and third light (normalized to total flux at phase 0.25).
(a) From HHH03.


Source LaTeX | All tables | In the text

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