首页> 外文期刊>The Astrophysical journal >A STATISTICAL ANALYSIS OF THE ACCURACY OF THE DIGITIZED MAGNITUDES OF PHOTOMETRIC PLATES ON THE TIMESCALE OF DECADES WITH AN APPLICATION TO THE CENTURY-LONG LIGHT CURVE OF KIC 8462852
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A STATISTICAL ANALYSIS OF THE ACCURACY OF THE DIGITIZED MAGNITUDES OF PHOTOMETRIC PLATES ON THE TIMESCALE OF DECADES WITH AN APPLICATION TO THE CENTURY-LONG LIGHT CURVE OF KIC 8462852

机译:十年时间刻度上光度计数字化光度板的精度的统计分析及其在KIC 8462852的百年长光曲线中的应用

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We present a statistical analysis of the accuracy of the digitized magnitudes of photometric plates on the timescale of decades. In our examination of archival Johnson B photometry from the Harvard DASCH archive, we find a median rms scatter of light curves of the order of 0.15 mag over the range B ~ 9–17 for all calibrations. Slight underlying systematics (trends or flux discontinuities) are on a level of 0.2 mag per century (1889–1990) for the majority of constant stars. These historic data can be unambiguously used for processes that happen on scales of magnitudes, and need to be carefully examined in cases approaching the noise floor. The characterization of these limits in photometric stability may guide future studies in their use of plate archives. We explain these limitations for the example case of KIC 8462852, which has been claimed to dim by 0.16 mag per century, and show that this trend cannot be considered as significant.
机译:我们在几十年的时间尺度上对光度板的数字化量级的准确性进行了统计分析。在我们从哈佛大学DASCH档案馆对Johnson Johnson B测光档案进行的检查中,我们发现,在所有校准中,B〜9-17范围内的光曲线的均方根有效值散射为0.15 mag量级。对于大多数恒星来说,轻微的潜在系统学(趋势或通量不连续性)处于每世纪0.2 mag的水平(1889–1990年)。这些历史数据可以毫无疑问地用于发生在规模上的过程,并且在接近本底噪声的情况下需要仔细检查。这些对光度稳定性的限制的特征可能会指导将来使用印版档案的研究。我们以KIC 8462852的示例为例解释了这些局限性,该示例据称每世纪以0.16 mag的速度变暗,并表明该趋势不能被认为是重要的。

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