JWST-Jupiter MIRI Exogenous molecules (HCN, CO2 and H2O)

In these files you will find the dataset used for the refered article. You will find three main directories noted 'obsX', where X is the JWST observation 1, 2 or 3, each of them for a specific longitude (335W, 70W and 135W). Within these files you will find the directories to HCN, CO2 and H2O. We remind that for CO2 you will find the retrieved profiles in the .inv files for each spaxel of the MRS FOV. For HCN and H2O you will find the mean latitude spectra. The comparison between the observed and synthetic spectrum is found in the .res files. For more information regarding this dataset, please contact [e-mail] or [e-mail]

本数据集文件包含所提及学术论文所使用的实验数据集。您将看到三个命名为`obsX`的主目录，其中X代表詹姆斯·韦布空间望远镜（James Webb Space Telescope, JWST）的3次观测计划（分别为1、2、3号），对应经度335W、70W与135W。各主目录下均包含针对HCN、CO₂与H₂O的专项子目录。需注意：针对CO₂，您可在`.inv`格式文件中获取中分辨率光谱仪（Medium Resolution Spectrometer, MRS）视场（Field of View, FOV）内每个空间像素（spaxel）的反演廓线；针对HCN与H₂O，您可获取对应的纬向平均光谱。观测光谱与合成光谱的对比结果可在`.res`格式文件中查阅。如需获取该数据集的更多相关信息，请联系邮箱[e-mail]或[e-mail]。