K2和TESS同时观测到的M矮星耀斑候选者

Dylan S. Caudill, Thomas Slamecka, Jeffrey M. Gerber
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引用次数: 0

摘要

我们介绍利用 K2 和 TESS 数据识别 M 矮耀斑的研究结果。我们的样本包括这两个任务同时观测到的天体,因此我们也可以比较如何在两组数据中识别耀斑。我们使用两个开源 Python 软件包 Lightkurve 和 PyVAN 协同工作,以轻松访问数据并确定 39 个 M-矮星光变曲线的可变性。我们在TESS数据中发现了13个耀斑,而K2没有提供任何可靠的耀斑探测。我们描述了K2数据的不足之处,这些不足之处导致无法识别这些耀斑。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
M-Dwarf Flare Candidates Simultaneously Observed by K2 and TESS
We present results of a study on the identification of M-dwarf flares using K2 and TESS data. Our sample includes objects observed simultaneously by these two missions, so that we can also compare how flares are identified in the two sets of data. We implement two open-source Python packages, Lightkurve and PyVAN, to work in unison to easily access the data and determine variability in the light curves of 39 M-dwarfs. We identified 13 flare detections in the TESS data while K2 did not provide any reliable detections of flares. We describe the shortcomings of the K2 data that prevented these flares from being identified.
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