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Two-color speckle imaging of M dwarfs with the Discovery Channel telescope

机译:发现频道望远镜对M个小矮人进行双色散斑成像

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Lowell Observatory and Southern Connecticut State University are currently involved in a joint project to determine the stellar multiplicity rates and the fundamental stellar parameters of M dwarf stars using the Differential Speckle Survey Instrument (DSSI) at Lowell's Discovery Channel Telescope (DCT). DSSI observes speckle patterns simultaneously at two separate wavelengths, allowing color measurements of the components of a binary system to be made in a single observation. This paper will describe the initial data gathering process, which began in 2016. Since then, over 1000 stars have been observed. We summarize the analysis on these objects so far, and discuss the relevance of these observations for existing and future space missions such as TESS, JWST, and Gaia.
机译:洛厄尔天文台和南康涅狄格州立大学目前正在参与一个联合项目,目的是使用洛厄尔发现频道望远镜(DCT)上的差分散斑测量仪(DSSI)确定M矮星的恒星多重率和基本恒星参数。 DSSI在两个独立的波长上同时观察斑点图案,从而允许在一次观察中对二元系统的组件进行颜色测量。本文将描述始于2016年的初始数据收集过程。自那时以来,已观测到超过1000颗恒星。到目前为止,我们总结了对这些物体的分析,并讨论了这些观测结果与现有和未来的太空飞行任务(如TESS,JWST和Gaia)的相关性。

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