天基微透镜视差退化中的密切圆与相交圆

A. Gould
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引用次数: 7

摘要

我研究了卫星微透镜视差pi_E测量中弧简并的起源,仅使用晚时间数据,例如从卫星上看到的t >到0 + t_E。我证明了这些是由于pi_E平面上一系列紧密的、完全圆形的简并的部分重叠,每一个都来自一次测量。在有较早数据的事件中,这些长弧分成两个弧,或者(更早的数据)两个点,因为这些较早的测量产生的是相交而不是相交的圆。这两个点构成了众所周知的天基微透镜视差四重简并中的一对简并。使用这种相交圆的框架,我展示了下一代微透镜卫星实验可以产生良好的pi_E测定,每个事件只有大约5次测量,即每天大约30次观测,每年监测1500个事件。这似乎可以用一个小的(因此便宜,本着Gould & Yee 2012的精神)卫星望远镜来完成,例如20厘米。
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Osculating Versus Intersecting Circles in Space-Based Microlens Parallax Degeneracies
I investigate the origin of arc degeneracies in satellite microlens parallax pi_E measurements with only late time data, e.g., t > t0 + t_E as seen from the satellite. I show that these are due to partial overlap of a series of osculating, exactly circular, degeneracies in the pi_E plane, each from a single measurement. In events with somewhat earlier data, these long arcs break up into two arclets, or (with even earlier data) two points, because these earlier measurements give rise to intersecting rather than osculating circles. The two arclets (or points) then constitute one pair of degeneracies in the well-known four-fold degeneracy of space-based microlens parallax. Using this framework of intersecting circles, I show that next-generation microlens satellite experiments could yield good pi_E determinations with only about five measurements per event, i.e., about 30 observations per day to monitor 1500 events per year. This could plausibly be done with a small (hence cheap, in the spirit of Gould & Yee 2012) satellite telescope, e.g., 20 cm.
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