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The Transit Light Curve (TLC) Project. II. Two Transits of the Exoplanet OGLE-TR-111b

机译:Transit Light Curve(TLC)项目。 II。系外行星的两次转换   OGLE-TR-111B

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摘要

As part of our ongoing effort to measure exoplanet sizes and transit timeswith greater accuracy, we present I band observations of two transits ofOGLE-TR-111b. The photometry has an accuracy of 0.15-0.20% and a cadence of 1-2minutes. We derive a planetary radius of 1.067 +/- 0.054 Jupiter radii and astellar radius of 0.831 +/- 0.031 solar radii. The uncertainties are dominatedby errors in the photometry, rather than by systematic errors arising fromuncertainties in the limb darkening function or the stellar mass. Both thestellar radius and the planetary radius are in agreement with theoreticalexpectations. The transit times are accurate to within 30 seconds, and allow usto refine the estimate of the mean orbital period: 4.0144479 +/- 0.0000041days.
机译:为了更精确地测量系外行星的大小和飞行时间,我们提出了OGLE-TR-111b两次飞行的I波段观测结果。光度法的精度为0.15-0.20%,节奏为1-2分钟。我们得出的行星半径为1.067 +/- 0.054木星半径,而星际半径为0.831 +/- 0.031太阳半径。不确定性主要由光度学误差决定,而不是由肢体变暗功能或恒星质量不确定性引起的系统误差决定。星际半径和行星半径均与理论预期相符。渡越时间精确到30秒以内,并允许我们完善平均轨道周期的估算:4.0144479 +/- 0.0000041天。

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