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MaxEnt power spectrum estimation using the Fourier transform for irregularly sampled data applied to a record of stellar luminosity

机译:使用傅里叶变换对恒星光度记录中不规则采样的数据进行MaxEnt功率谱估计

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摘要

The principle of maximum entropy is applied to the spectral analysis of a data signal with general variance matrix and containing gaps in the record. The role of the entropic regularizer is to prevent one from overestimating structure in the spectrum when faced with imperfect data. Several arguments are presented suggesting that the arbitrary prefactor should not be introduced to the entropy term. The introduction of that factor is not required when a continuous Poisson distribution is used for the amplitude coefficients. We compare the formalism for when the variance of the data is known explicitly to that for when the variance is known only to lie in some finite range. The result of including the entropic measure factor is to suggest a spectrum consistent with the variance of the data which has less structure than that given by the forward transform. An application of the methodology to example data is demonstrated.
机译:最大熵原理适用于具有一般方差矩阵且记录中包含间隙的数据信号的频谱分析。熵调节器的作用是防止在面对不完善的数据时过高估计频谱结构。提出了一些论点,建议不应将任意前置因子引入熵项。当将连续泊松分布用于振幅系数时,不需要引入该因子。我们将形式主义用于当数据的方差是已知的时与将方差仅在某个有限范围内时的形式进行比较。包括熵度量因子的结果是建议一个与数据方差一致的频谱,该数据的结构比正向变换给出的结构少。演示了该方法在示例数据中的应用。

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