Why is it so Cold in Here? - Posteriors

Supplementary material for '<em>Why is it so Cold in Here?: Explaining the Cold Temperatures Retrieved from Transmission Spectra of Exoplanet Atmospheres</em>' - ApJL (2020). This repository contains the posterior probability distributions from the retrievals in Sections 3 and 4 of MacDonald, Goyal, &amp; Lewis (2020). The case studies are a typical 'warm', 'hot', and 'ultra-hot' Jupiter, along with self-consistent models of WASP-17b and WASP-12b. For each retrieval, the corner plot depicts correlations between pairs of retrieved parameters and marginalised histograms for each parameter. Red dashed lines and green squares indicate the true terminator-averaged parameter values used to generate the synthetic observations. The table inset compares the true values with retrieved inferences. Where parameters have clear upper and lower bounds, the median retrieved values and ±1σ confidence levels are given. Otherwise, parameter constraints are expressed as 2σ upper or lower bounds. For any questions, please contact: [e-mail]本数据集为《这里为何如此寒冷？——系外行星大气透射光谱反演所得低温温度的成因阐释》一文的补充材料，该文发表于《天体物理学杂志快报》(ApJL, 2020)。本仓库包含MacDonald、Goyal与Lewis（2020）论文第3、4节中大气反演流程所得的后验概率分布。本数据集的案例研究涵盖典型的暖类木行星、热类木行星与超热类木行星，以及WASP-17b和WASP-12b的自洽模型。针对每一次反演，边角图（corner plot）会展示各反演参数间的两两相关性，以及各参数的边际化直方图。红色虚线与绿色方块代表生成合成观测所用的真实晨昏线平均参数值。内嵌表格将真实参数值与反演得到的推断结果进行对比。对于存在明确上下限的参数，我们会给出反演所得的中位数值以及±1σ置信区间；其余参数的约束则以2σ上限或下限形式表示。如有任何疑问，请联系：[e-mail]