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Making cosmic microwave background temperature and polarization maps with MADAM

机译:用MADAM制作宇宙微波背景温度和极化图

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MADAM is a CMB map-making code, designed to maketemperature and polarization maps of time-ordered data of totalpowerexperiments like P LANCK. The algorithm is based on the destripingtechnique, but it also makes use of known noise properties in theform of a noise prior. The method in its early form was presented inan earlier work by Keih?nen etal.(2005, MNRAS, 360, 390).In this paper we present an update of the method, extended tonon-averaged data, and include polarization. In this method thebaseline length is a freely adjustable parameter, and destriping canbe performed at a different map resolution than that of the finalmaps. We show results obtained with simulated data. This study isrelated to P LANCK LFIactivities.Key words: cosmology: cosmic microwave background - methods: data analysis
机译:MADAM是CMB地图制作代码,旨在为诸如P LANCK之类的总功率实验的时间顺序数据制作温度和极化地图。该算法基于去条纹技术,但是它也以先验噪声的形式利用已知的噪声特性。 Keihnen et al。(2005,MNRAS,360,390)在较早的工作中提出了该方法的早期形式。在本文中,我们介绍了该方法的更新,扩展到非平均数据,包括极化。在此方法中,基线长度是一个可自由调整的参数,可以在与最终图不同的图分辨率下执行去条纹。我们显示了使用模拟数据获得的结果。这项研究与P LANCK LFI活性有关。关键词:宇宙学:宇宙微波背景-方法:数据分析

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