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Ground-based photometric follow-up for exoplanet detections with the PLATO mission PLATO 飞行任务对系外行星探测的地基光度跟踪
Pub Date : 2024-01-09 DOI: 10.31577/caosp.2024.54.2.142
H. Deeg, R. A. I. D. A. D. Canarias, U. L. Laguna
Detections of transiting planets from the upcoming PLATO mission are expected to face significant contamination from contaminating eclipsing binaries, resulting in false positives. To counter this, a ground-based programme to acquire time-critical photometry is pursued. Its principal aim is to obtain time-series observations of the planet candidate and its surrounding stars at the times of expected transits. This programme is part of the PLATO Ground-based Observations Programme, which also covers spectroscopic and imaging observations. The current photometric follow-up programme is assembling the required observational resources, executing benchmark observations, and defining strategies for the observations and their reporting. Post-launch, it will focus on coordinating photometric data collection and analysis, and will update candidate statuses in the PLATO follow-up database. Its work packages are outlined, covering specific tools, citizen contributions, standard and multi-colour observations, secondary eclipses, and reprocessing of archival photometry. Ground-based follow-up photometry will likely concentrate on longer-period candidates, given that false positives of short-period candidates will likely become identifiable in timeseries available from GAIA in the near future. Geographical considerations for follow-up observations from the first PLATO long-observation field LOPS2 are outlined, which lies in the southern hemisphere, with later fields expected to be more suitable for northern observers.
即将进行的 PLATO 飞行任务对凌日行星的探测预计将面临来自日食双星的严重污染,从而造成假阳性。为了解决这个问题,正在实施一项获取时间关键光度计的地面计划。其主要目的是在预计的凌日时间获得候选行星及其周围恒星的时间序列观测数据。该方案是 PLATO 地面观测方案的一部分,该方案还包括光谱和成像观测。目前的测光跟踪计划正在汇集所需的观测资源,执行基准观测,并确定观测和报告战略。发射后,该计划将重点协调测光数据的收集和分析工作,并更新 PLATO 后续行动数据库中的候选状态。它的工作包包括特定工具、公民贡献、标准和多色观测、二次日食以及档案光度测量的再处理。地基跟踪测光可能会集中在较长周期的候选天体上,因为在不久的将来,短周期候选天体的假阳性可能会在 GAIA 提供的时间序列中被识别出来。概述了从 PLATO 第一个长期观测场 LOPS2 进行后续观测的地理考虑因素,该观测场位于南半球,预计以后的观测场更适合北方观测者。
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Contributions of the Astronomical Observatory Skalnaté Pleso
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