ExoMolOP数据库:高温系外行星大气中感兴趣的分子的横截面和k表

K. Chubb, M. Rocchetto, S. Yurchenko, M. Min, I. Waldmann, J. Barstow, P. Mollière, A. Al-Refaie, M. Phillips, J. Tennyson
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引用次数: 40

摘要

基于ExoMol、HITEMP和MoLLIST数据库中最新的谱表数据,ExoMolOP是一个公开可用的天体物理学兴趣分子不透明数据库,已经汇编了超过80个物种。这些数据通常适用于描述高温系外行星或凉爽的恒星/亚恒星大气,并且在各种压力和温度下计算,仅在HITRAN数据库中包含室温下的一些分子。数据以不同的方式格式化为四种不同的系外行星大气检索代码;ARCiS, TauREx, NEMESIS和petitRADTRANS,并包括0.3 - 50 $\mu$ m波长区域的横截面(R = $\frac{\lambda}{\Delta \lambda}$ = 15,000)和k表(R = $\frac{\lambda}{\Delta \lambda}$ = 1000)。不透明度文件可以下载并直接用于这些代码。碱金属Na和K的原子数据也包括在内,使用来自NIST数据库的数据和最新的共振线形状。展宽参数已从文献中获得,或从具有类似分子性质的已知分子中获得,但没有展宽数据。数据可以从这个http URL获得。
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The ExoMolOP database: Cross sections and k-tables for molecules of interest in high-temperature exoplanet atmospheres
A publicly available database of opacities for molecules of astrophysical interest, ExoMolOP, has been compiled for over 80 species, based on the latest line list data from the ExoMol, HITEMP and MoLLIST databases. These data are generally suitable for characterising high temperature exoplanet or cool stellar/substellar atmospheres, and have been computed at a variety of pressures and temperatures, with a few molecules included at room-temperature only from the HITRAN database. The data are formatted in different ways for four different exoplanet atmosphere retrieval codes; ARCiS, TauREx, NEMESIS and petitRADTRANS, and include both cross-sections (at R~=~$\frac{\lambda}{\Delta \lambda}$~=~15,000) and k-tables (at R~=~$\frac{\lambda}{\Delta \lambda}$~=~1000) for the 0.3~-~50$\mu$m wavelength region. Opacity files can be downloaded and used directly for these codes. Atomic data for alkali metals Na and K are also included, using data from the NIST database and the latest line shapes for the resonance lines. Broadening parameters have been taken from the literature where available, or from those for a known molecule with similar molecular properties where no broadening data are available. The data are available from this http URL.
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