GJ 436b and XO-1b transits
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Currently the only technique sensitive to Earth mass planets around nearby stars (that are too close for microlensing) is the monitoring of the transit time variations of the...
当前,针对距离过近而无法采用微引力透镜(microlensing)开展探测的邻近恒星周围的地球质量行星,唯一具备有效探测灵敏度的技术为凌星时间变化(transit time variations)监测法……



