SKA 时代大尺度结构旋转量网格分析的统计方法
宇宙学与河外天体物理
2015-01-05 v1
摘要
为了更好地理解宇宙磁场的起源和性质，详细了解宇宙大尺度结构（星系团、纤维状结构）中的磁场至关重要。我们提出了一种新的统计方法，利用新一代射电干涉仪将获得的旋转量网格数据来研究大尺度磁场。
引用
@article{arxiv.1501.00415,
title = {Statistical methods for the analysis of rotation measure grids in large scale structures in the SKA era},
author = {Valentina Vacca and Niels Oppermann and Torsten Ensslin and Marco Selig and Henrik Junklewitz and Maksim Greiner and Jens Jasche and Christopher Hales and Martin Reinecke and Ettore Carretti and Luigina Feretti and Chiara Ferrari and Gabriele Giovannini and Federica Govoni and Cathy Horellou and Shinsuke Ideguchi and Melanie Johnston-Hollitt and Matteo Murgia and Rosita Paladino and Roberto Francesco Pizzo and Scaife Anna},
journal= {arXiv preprint arXiv:1501.00415},
year = {2015}
}
备注
9 pages; to appear as part of 'Cosmic Magnetism' in Proceedings 'Advancing Astrophysics with the SKA (AASKA14)', PoS(AASKA14)114