Analysis of Exoplanet Light Curves

被引：0

作者：

Erdem, A. ^{[1
]}

Budding, E. ^{[1
,2
,3
,4
]}

Rhodes, M. D. ^{[5
]}

Puskullu, Q. ^{[1
]}

Soydugan, F. ^{[1
]}

Soydugan, E. ^{[1
]}

Tuysuz, M. ^{[1
]}

Demircan, O. ^{[1
]}

机构：

[1] Canakkale Onsekiz Mart Univ, Astrophys Res Ctr & Observ, Terzioglu Kampusu, TR-17020 Canakkale, Turkey

[2] Carter Observ, Wellington, New Zealand

[3] Victoria Univ Wellington, SCPS, Wellington, New Zealand

[4] Univ Canterbury, Dept Phys & Astron, Christchurch 8140, New Zealand

[5] Brigham Young Univ, Dept Ancient Scripture, Provo, UT 84602 USA

来源：

LIVING TOGETHER: PLANETS, HOST STARS, AND BINARIES | 2015年 / 496卷

关键词：

D O I：

暂无

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We have applied the close binary system analysis package WINFITTER to a variety of exoplanet transiting light curves taken both from the NASA Exoplanet Archive and our own groundbased observations. WINFITTER has parameter options for a realistic physical model, including gravity brightening and structural parameters derived from Kopal's applications of the relevant Radau equation, and it includes appropriate tests for determinacy and adequacy of its best fitting parameter sets. We discuss a number of issues related to empirical checking of models for stellar limb darkening, surface maculation, Doppler beaming, microvariability, and transit time variation (TTV) effects. The Radau coefficients used in the light curve modeling, in principle, allow structural models of the component stars to be tested.

引用

页码：365 / 369

页数：5

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