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PreProFit: Pressure Profile Fitter for galaxy clusters

机译:PreProFit:银河星团的压力剖面拟合器

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摘要

Galaxy cluster analyses based on high-resolution observations of the Sunyaev–Zeldovich (SZ) effect have become common in the last decade. We present PreProFit , the first publicly available code designed to fit the pressure profile of galaxy clusters from SZ data. PreProFit is based on a Bayesian forward-modelling approach, allows the analysis of data coming from different sources, adopts a flexible parametrization for the pressure profile, and fits the model to the data accounting for Abel integral, beam smearing, and transfer function filtering. PreProFit is computationally efficient, is extensively documented, has been released as an open source Python project, and was developed to be part of a joint analysis of X-ray and SZ data on galaxy clusters. PreProFit returns χ ~(2), model parameters and uncertainties, marginal and joint probability contours, diagnostic plots, and surface brightness radial profiles. PreProFit also allows the use of analytic approximations for the beam and transfer functions useful for feasibility studies.
机译:在过去的十年中,基于对Sunyaev–Zeldovich(SZ)效应的高分辨率观测的银河星团分析变得很普遍。我们展示了PreProFit,这是第一个公开的代码,旨在根据SZ数据拟合星系团的压力分布。 PreProFit基于贝叶斯正向建模方法,可以分析来自不同来源的数据,对压力曲线采用灵活的参数化,并使模型适合于考虑Abel积分,束拖影和传递函数滤波的数据。 PreProFit计算效率高,已被广泛记录,已经作为开源Python项目发布,并且被开发为对银河星团上X射线和SZ数据进行联合分析的一部分。 PreProFit返回χ〜(2),模型参数和不确定性,边际和联合概率等高线,诊断图和表面亮度径向轮廓。 PreProFit还允许对光束和传递函数进行解析近似,这对于可行性研究很有用。

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