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Calibration issues in estimating variability of the fine structure constant (alpha) with cosmic time

机译:估计精细结构的可变性的校准问题   常数(alpha)与宇宙时间

摘要

Laser Comb Wavelength calibration shows that the ThAr one is locallyunreliable with possible deviations of up to 100 m/s within one order range,while delivering an overall 1 m/s accuracy (Wilken et al 2009). Such deviationcorresponds to delta alpha/alpha ~ 7E-6 for a FeII-MgII pair. Comparison ofline shifts among the 5 FeII lines, with almost identical sensitivity to finestructure constant changes, offers a clean way to directly test the presence ofpossible local wavelength calibration errors of whatever origin. We analyzed 5absorption systems, with zabs ranging from 1.15 to 2.19 towards 3 bright QSOs.The results show that while some lines are aligned within 20 m/s, others reveallarge deviations reaching 200 m/s or higher and corresponding to a deltaalpha/alpha > 1E-5 level. The origin of these deviations is not clearlyidentified but could be related to the adaptation of wavelength calibration toCCD manufacturing irregularities. These results suggest that to drawconclusions from delta alpha/alpha analysis based on one or only few lines mustbe done with extreme care.
机译:激光梳状波波长校准表明,ThAr激光器在局部不可靠,在一阶范围内可能存在高达100 m / s的偏差,而总体精度为1 m / s(Wilken等,2009)。对于FeII-MgII对,这种偏离对应于δalpha / alpha〜7E-6。比较5条FeII线之间的线位移,对精细结构常数变化几乎具有相同的敏感性,提供了一种直接测试任何来源的本地波长校准误差是否存在的干净方法。我们分析了5个吸收系统,朝着3个明亮的QSO的zab范围从1.15到2.19。结果显示,尽管某些线在20 m / s内对齐,但其他线则显示出大的偏差达到200 m / s或更高,对应于deltaalpha / alpha 1E-5级。这些偏差的起因尚不清楚,但可能与波长校准适应CCD制造不规则有关。这些结果表明,要根据一条或仅几条线从δalpha / alpha分析得出结论,必须格外小心。

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