The Emission Spectrum of the Hot Jupiter WASP-79b from HST/WFC3

Supplementary material for 'The Emission Spectrum of the Hot Jupiter WASP-79b from HST/WFC3'.

This repository contains posterior probability distributions for the two cases that were investigated using the 'white' light data of WASP-79b captured by the Hubble Space Telescope using the Wide Field Camera 3. It also contains the posterior probability distributions for three spectroscopic channels. 

The two 'white' light corner plots consider two scenarios: a fixed mid-eclipse time based on the expected occurrence time and a mid-eclipse time set as a free parameter. The three spectroscopic corner plots then look at the observations divided into three equal wavelength bins of width 0.20 μm centered at 1.18, 1.38, and 1.58 μm. The spectroscopic analysis was done under the scenario of a free mid-eclipse time.

《基于哈勃空间望远镜WFC3的热木星WASP-79b发射光谱》补充材料。本仓库包含两项基于哈勃空间望远镜（Hubble Space Telescope, HST）广角相机3（Wide Field Camera 3, WFC3）获取的WASP-79b‘白光’测光数据开展的研究案例对应的后验概率分布，同时还包含三个光谱通道的后验概率分布。两组‘白光’测光边角图对应两种分析场景：一种是基于理论预期时刻固定食中时刻，另一种则将食中时刻设为自由参数。三组光谱边角图则对应将观测数据按波长划分为三个宽度为0.20 μm的均等区间，中心波长分别为1.18 μm、1.38 μm与1.58 μm；光谱分析均采用将食中时刻设为自由参数的分析场景。