论文标题
KMT-2021-BLG-0171LB和KMT-2021-BLG-1689LB:KMTNET高环境中的两个微透镜行星,带有后续观测值
KMT-2021-BLG-0171Lb and KMT-2021-BLG-1689Lb: Two Microlensing Planets in the KMTNet High-cadence Fields with Followup Observations
论文作者
论文摘要
高磁化重力微晶体事件的后续观察可以完全利用其内在灵敏度来检测出极地球的行星,尤其是质量比小的行星。为了使后续效率更加统一和高效,我们基于韩国微透镜望远镜网络(KMTNET)的实时数据开发一个系统,高磁化器,以自动提醒可能正在进行的高磁化事件。我们在2021年在HighMagfinder的帮助下开始了一个新的后续观察阶段。在这里,我们报告了在高磁化微透明事件中发现了两个行星,KMT-2021-BLG-0171和KMT-2021-BLG-1689,这些行星由HighMagFinder鉴定出来。我们发现这两个事件都遭受了``中央谐振''的腐蚀性堕落性。 Planet-host质量比率为$ q \ sim4.7 \ times10^{ - 5} $或$ q \ sim 2.2 \ sim 2.2 \ times10^{ - 5} $ for KMT-2021-Blg-0171,$ q \ sim2.5 \ sim2.5 \ times10^{ - 4} $ q \ sim $ q \ sim 1.8} $ \ sim 1.8 \ \ s.8 \ \ \ s.8 \ \ 44 KMT-2021-BLG-1689。以及Ryu等人报道的两个事件。 (2022),仅在2021季节就发现了四个遭受这种堕落的病例,这表明在以前的一些研究中可能错过了退化解决方案。我们还提出了一个新因素,以加权从相位空间中每个溶液的概率。在此考虑的情况下,对这两个事件的共振解释不利。该因素可以包含在未来的统计研究中,以使溶液重量退化。
Follow-up observations of high-magnification gravitational microlensing events can fully exploit their intrinsic sensitivity to detect extrasolar planets, especially those with small mass ratios. To make followup more uniform and efficient, we develop a system, HighMagFinder, based on the real-time data from the Korean Microlensing Telescope Network (KMTNet) to automatically alert possible ongoing high-magnification events. We started a new phase of follow-up observations with the help of HighMagFinder in 2021. Here we report the discovery of two planets in high-magnification microlensing events, KMT-2021-BLG-0171 and KMT-2021-BLG-1689, which were identified by the HighMagFinder. We find that both events suffer the ``central-resonant'' caustic degeneracy. The planet-host mass-ratio is $q\sim4.7\times10^{-5}$ or $q\sim 2.2\times10^{-5}$ for KMT-2021-BLG-0171, and $q\sim2.5\times10^{-4}$ or $q\sim 1.8\times10^{-4}$ for KMT-2021-BLG-1689. Together with two events reported by Ryu et al. (2022), four cases that suffer such degeneracy have been discovered in the 2021 season alone, indicating that the degenerate solutions may have been missed in some previous studies. We also propose a new factor for weighting the probability of each solution from the phase-space. The resonant interpretations for the two events are disfavored under this consideration. This factor can be included in future statistical studies to weight degenerate solutions.