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首页> 外文期刊>Publications of the Astronomical Society of the Pacific >Visual Binary Stars with Partially Missing Data: Introducing Multiple Imputation in Astrometric Analysis
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Visual Binary Stars with Partially Missing Data: Introducing Multiple Imputation in Astrometric Analysis

机译:具有部分缺少数据的视觉二进制星星:在星形分析中引入多重估算

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摘要

Partial measurements of relative position are a relatively common event during the observation of visual binary stars. However, these observations are typically discarded when estimating the orbit of a visual pair. In this article we present a novel framework to characterize the orbits from a Bayesian standpoint, including partial observations of relative position as an input for the estimation of orbital parameters. Our aim is to formally incorporate the information contained in those partial measurements in a systematic way into the final inference. In the statistical literature, an imputation is defined as the replacement of a missing quantity with a plausible value. To compute posterior distributions of orbital parameters with partial observations, we propose a technique based on Markov chain Monte Carlo with multiple imputation. We present the methodology and test the algorithm with both synthetic and real observations, studying the effect of incorporating partial measurements in the parameter estimation. Our results suggest that the inclusion of partial measurements into the characterization of visual binaries may lead to a reduction in the uncertainty associated to each orbital element, in terms of a decrease in dispersion measures (such as the interquartile range) of the posterior distribution of relevant orbital parameters. The extent to which the uncertainty decreases after the incorporation of new data (either complete or partial) depends on how informative those newly incorporated measurements are. Quantifying the information contained in each measurement remains an open issue.
机译:相对位置的部分测量是在观察视觉二元恒星期间的相对常见的事件。然而,当估计视觉对的轨道时通常丢弃这些观察。在本文中,我们提出了一种新颖的框架,以表征来自贝叶斯观点的轨道,包括与相对位置的部分观察作为估计轨道参数的输入。我们的目标是以系统的方式正式地将包含在这些部分测量中的信息纳入最终推理。在统计文献中,归纳被定义为用合理的值替换缺失的数量。为了用部分观测计算轨道参数的后部分布,我们提出了一种基于Markov Chain Monte Carlo的技术,具有多种估算。我们介绍了合成和实际观测的方法和测试算法,研究了在参数估计中结合局部测量的效果。我们的研究结果表明,将部分测量纳入视觉二进制文件的表征可能导致与每个轨道元件相关的不确定性的降低,就相关的分散措施(如间条件)的降低而言轨道参数。在纳入新数据(完整或部分)后不确定性减少的程度取决于新掺入的测量的信息。量化每个测量中包含的信息仍然是一个开放问题。

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