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Campaign 9 of the K2 Mission: Observational Parameters, Scientific Drivers, and Community Involvement for a Simultaneous Space- and Ground-based Microlensing Survey

机译:K2任务的战役9:观测参数,科学驱动力以及社区参与的同时进行的基于天地的微透镜调查

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K2's Campaign 9 (K2C9) will conduct a similar to 3.7 deg(2) survey toward the Galactic bulge from 2016 April 22 through July 2 that will leverage the spatial separation between K2 and the Earth to facilitate measurement of the microlens parallax pi(E) for greater than or similar to 170 microlensing events. These will include several that are planetary in nature as well as many short-timescale microlensing events, which are potentially indicative of free-floating planets (FFPs). These satellite parallax measurements will in turn allow for the direct measurement of the masses of and distances to the lensing systems. In this article we provide an overview of the K2C9 space-and ground-based microlensing survey. Specifically, we detail the demographic questions that can be addressed by this program, including the frequency of FFPs and the Galactic distribution of exoplanets, the observational parameters of K2C9, and the array of resources dedicated to concurrent observations. Finally, we outline the avenues through which the larger community can become involved, and generally encourage participation in K2C9, which constitutes an important pathfinding mission and community exercise in anticipation of WFIRST.
机译:从2016年4月22日到7月2日,K2的第9战役(K2C9)会对银河系凸起进行类似于3.7度(2)的调查,该调查将利用K2和地球之间的空间分离来方便测量微透镜视差pi(E)大于或类似于170个微透镜事件。这些将包括一些本质上是行星的,以及许多短时尺度的微透镜事件,这些事件可能表示自由漂浮的行星(FFP)。这些卫星视差测量将继而允许直接测量透镜系统的质量和与透镜系统的距离。在本文中,我们概述了K2C9太空和地面微透镜调查。具体来说,我们详细介绍了此程序可以解决的人口统计问题,包括FFP的频率和系外行星的银河分布,K2C9的观测参数以及专用于同时观测的资源阵列。最后,我们概述了更大的社区可以参与的渠道,并总体上鼓励人们参与K2C9,这构成了对WFIRST的重要寻路任务和社区实践。

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