Updated forecast for TRAPPIST-1 times of transit for all seven exoplanets incorporating JWST data

Eric Agol, Natalie H. Allen, Björn Benneke, Laetitia Delrez, René Doyon, Elsa Ducrot, Néstor Espinoza, Amélie Gressier, David Lafrenière, Olivia Lim, Jacob Lustig-Yaeger, Caroline Piaulet-Ghorayeb, Michael Radica, Zafar Rustamkulov, Kristin S. Sotzen
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Abstract

The TRAPPIST-1 system has been extensively observed with JWST in the near-infrared with the goal of measuring atmospheric transit transmission spectra of these temperate, Earth-sized exoplanets. A byproduct of these observations has been much more precise times of transit compared with prior available data from Spitzer, HST, or ground-based telescopes. In this note we use 23 new timing measurements of all seven planets in the near-infrared from five JWST observing programs to better forecast and constrain the future times of transit in this system. In particular, we note that the transit times of TRAPPIST-1h have drifted significantly from a prior published analysis by up to tens of minutes. Our newer forecast has a higher precision, with median statistical uncertainties ranging from 7-105 seconds during JWST Cycles 4 and 5. Our expectation is that this forecast will help to improve planning of future observations of the TRAPPIST-1 planets, whereas we postpone a full dynamical analysis to future work.
结合 JWST 数据更新预测 TRAPPIST-1 所有七颗系外行星的过境时间
JWST 对 TRAPPIST-1 系统进行了广泛的近红外观测,目的是测量这些温带、地球大小的系外行星的大气过境透射谱图。与之前从斯皮策、HST 或地面望远镜获得的数据相比,这些观测的一个副产品是更为精确的凌日时间。在这篇论文中,我们利用 JWST 五个观测项目中对全部七颗行星进行的 23 次新的近红外定时测量,更好地预测和限制了该系统未来的凌日时间。我们特别注意到,TRAPPIST-1h的凌日时间与之前发表的分析结果相比有了显著偏差,偏差达数十分钟。我们最新的预测精度更高,在 JWST 周期 4 和 5 中,统计不确定性中值为 7-105 秒。我们期望这一预测将有助于改进 TRAPPIST-1 行星未来观测的规划,而我们将把全面的动力学分析推迟到今后的工作中。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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