On the unique solution of planet and star parameters from an extrasolar planet transit light curve

被引：0
|
作者：
Seager, S [1 ]
Mallén-Ornelas, G [1 ]
机构：
[1] Inst Adv Study, Princeton, NJ 08540 USA
来源：
SCIENTIFIC FRONTIERS IN RESEARCH ON EXTRASOLAR PLANETS | 2003年 / 294卷
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D O I：
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中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
A unique analytical solution of planet and star parameters can be derived from an extrasolar planet transit light curve under a number of assumptions. This analytical solution can be used to choose the best planet transit candidates for radial velocity follow-up measurements. In practice, high photometric precision (< 0.005 mag) and high time sampling (< 5 minutes) are needed for this method. See Seager & Mallen-Ornelas (2003) for full details.
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页码：419 / 422
页数：4
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