NSVS Star

 Fill

Q

Inclination

Teff

Separation

Reff

 

Star1

Star2

 M2/M1

 (degs)

Star1

Star2

 (Rsun)

Star1

Star2

01667524

0.75

0.94

0.925

80.612

4229

4300

11.542

0.350

0.376

01690749

0.99

0.33

2.190

81.762

4868

5750

0.767

0.318

0.195

04239237

1.00

0.49

1.518

77.186

5339

5800

0.509

0.348

0.265

05168710

0.99

0.33

3.343

81.641

4058

5500

11.919

0.284

0.205

05873479

0.98

0.52

0.784

78.388

4109

4250

11.233

0.407

0.241

06983718

0.97

0.47

0.750

68.166

3887

5000

0.648

0.410

0.217

08044036

1.00

0.53

6.251

84.984

4413

5200

11.624

0.239

0.357

10054338

1.00

0.71

3.745

75.388

3927

5750

8.511

0.275

0.428

10081872

0.97

0.39

1.067

75.696

4263

5000

9.356

0.379

0.197

14139046

1.00

0.45

2.738

77.653

4127

4700

4.906

0.300

0.270

 

The temperature of star 2 was set constant in ELC.  Temperatures are in Kelvin. All other parameters were found as the best chi-squared solution to the given light curve by ELC.  The fill of the star is given as the fraction of the Roche lobe filled by its star.  The effective radius is the radius of each star divided by the separation of the centers of the two stars.