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Phase correction for ALMA. Investigating water vapour radiometer scaling: The long-baseline science verification data case study

机译:ALMA的相位校正。研究水蒸气辐射计的缩放比例:长期基线科学验证数据案例研究

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The Atacama Large millimetre/submillimetre Array (ALMA) makes use of water vapour radiometers (WVR), which monitor the atmospheric water vapour line at 183 GHz along the line of sight above each antenna to correct for phase delays introduced by the wet component of the troposphere. The application of WVR derived phase corrections improve the image quality and facilitate successful observations in weather conditions that were classically marginal or poor. We present work to indicate that a scaling factor applied to the WVR solutions can act to further improve the phase stability and image quality of ALMA data. We find reduced phase noise statistics for 62 out of 75 datasets from the long-baseline science verification campaign after a WVR scaling factor is applied. The improvement of phase noise translates to an expected coherence improvement in 39 datasets. When imaging the bandpass source, we find 33 of the 39 datasets show an improvement in the signal-to-noise ratio (S/N) between a few to ~30 percent. There are 23 datasets where the S/N of the science image is improved: 6 by <1%, 11 between 1 and 5%, and 6 above 5%. The higher frequencies studied (band 6 and band 7) are those most improved, specifically datasets with low precipitable water vapour (PWV), <1?mm, where the dominance of the wet component is reduced. Although these improvements are not profound, phase stability improvements via the WVR scaling factor come into play for the higher frequency (>450?GHz) and long-baseline (>5?km) observations. These inherently have poorer phase stability and are taken in low PWV (<1?mm) conditions for which we find the scaling to be most effective. A promising explanation for the scaling factor is the mixing of dry and wet air components, although other origins are discussed. We have produced a python code to allow ALMA users to undertake WVR scaling tests and make improvements to their data.
机译:阿塔卡马大型毫米/亚毫米级阵列(ALMA)利用水蒸气辐射计(WVR),该监测仪沿每个天线上方的视线监测183 GHz的大气水蒸气线,以校正由天线的湿分量引入的相位延迟。对流层。 WVR派生的相位校正的应用改善了图像质量,并有助于在通常为边际或较差的天气条件下进行成功的观察。我们目前的工作表明,应用于WVR解决方案的比例因子可以起到进一步改善ALMA数据的相位稳定性和图像质量的作用。在应用WVR缩放因子后,我们发现来自长期基线科学验证活动的75个数据集中的62个数据集中的相位噪声统计量减少了。相位噪声的改善转化为39个数据集中预期的相干性改善。在对带通源进行成像时,我们发现39个数据集中的33个数据集的信噪比(S / N)改善了几到30%。有23个数据集可改善科学图像的S / N:6个数据集小于1%,11个在1%至5%之间,以及6个在5%以上。研究的较高频率(频带6和频带7)是最改进的频率,特别是具有低可沉淀水蒸气(PWV)(<1?mm)的数据集,其中湿分量的优势减小了。尽管这些改进并不深刻,但通过WVR比例因子进行相位稳定性的改进对于更高频率(> 450?GHz)和长基线(> 5?km)的观测起作用。这些固有地具有较差的相位稳定性,并且在低PWV(<1?mm)条件下使用,对于这种情况,我们发现缩放是最有效的。比例因子的有前途的解释是干空气成分和湿空气成分的混合,尽管还讨论了其他来源。我们已经制作了一个python代码,以允许ALMA用户进行WVR缩放测试并改善其数据。

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