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Single site observations of TESS single transit detections

机译:TESS单次运输检测的单站点观测

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Context. The Transiting Exoplanet Survey Satellite (TESS) has been successfully launched and has begin data acquisition. To expedite the science that may be performed with the resulting data it is necessary to gain a good understanding of planetary yields. Given the observing strategy employed by TESS the probability of detecting single transits in long period systems is increased. These systems require careful consideration. Aims. We aim to simulate the number of TESS transit detections during its two-year mission with a particular emphasis on single transits. We also aim to determine the feasibility of ground-based follow-up observations from a single site. Methods. A distribution of planets was simulated around the approximately four million stars in the TESS candidate target list. These planets were tested for detectable transits and characterised. Based on simulated parameters the single transit detections were further analysed to determine which are amenable to ground-based follow-up. Results. TESS will discover an approximate lower bound of 4700 planets with around 460 being single transits. A large fraction of these will be observable from a single ground-based site. This paper finds that, in a single year, approximately 1000 transit events of around 320 unique TESS single transit detections are theoretically observable. Conclusions. As we consider longer period exoplanets, the need for exploring single transit detections increases. For periods ?45 days the number of single transit detections outnumber multitransits by a factor of three (82 ± 18 and 25 ± 7, respectively) a factor which only grows as longer period detections are considered. Therefore, based on this paper, it is worth expending the extra effort required to follow-up these more challenging, but potentially very rewarding, discoveries. Additionally, we conclude that a large fraction of these targets can be theoretically observed from a single ground-based site. However, further work is required to determine whether these follow-up efforts are feasible when accounting for target specific criteria.
机译:上下文。过境系外行星测量卫星(TESS)已成功发射,并已开始进行数据采集。为了加快可能对结果数据执行的科学性,有必要对行星的产量有一个很好的了解。给定TESS所采用的观察策略,在长周期系统中检测单次运输的可能性增加了。这些系统需要仔细考虑。目的我们的目标是模拟TESS在执行为期两年的任务期间发现的次数,特别着重于单次过境。我们还旨在确定从单个站点进行地面后续观察的可行性。方法。在TESS候选目标列表中,模拟了大约四百万颗恒星周围的行星分布。对这些行星进行了可探测的过境测试并进行了表征。基于模拟参数,对单次运输检测进行进一步分析,以确定哪些方法适合地面跟踪。结果。 TESS将发现大约4700个行星的下界,其中约460个为单次过境。这些中的很大一部分将可以从单个地面站点观察到。本文发现,从理论上讲,在一年中,可以观察到大约320次TESS唯一一次过境检测中的大约1000次过境事件。结论。随着我们考虑到更长时间的系外行星,探索一次过境探测的需求增加了。在大约45天的时间内,单次运输检测的次数比多运输次数多3倍(分别为82±18和25±7),这个因素仅在考虑到更长的时间检测时才会增加。因此,根据本文,有必要花费额外的精力来跟进这些更具挑战性但可能非常有意义的发现。此外,我们得出的结论是,从理论上讲,可以从单个地面站点观察到很大一部分目标。但是,在考虑目标特定标准时,需要进一步的工作来确定这些后续工作是否可行。

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