MoLLIST: Molecular Line Lists, Intensities and Spectra

被引：108

作者：

Bernath, Peter F. ^{[1
]}

机构：

[1] Old Dominion Univ, Dept Chem & Biochem, Norfolk, VA 23529 USA

来源：

JOURNAL OF QUANTITATIVE SPECTROSCOPY & RADIATIVE TRANSFER | 2020年 / 240卷

关键词：

Line lists; Line strengths; Absorption cross sections; Exoplanets; Cool stars; High-resolution spectra; COMPUTER-PROGRAM; VIBRATIONAL SPECTRA; GROUND-STATE; STRENGTHS; TRANSITION; ABUNDANCES; EQUATION; NITROGEN; ATLAS; WATER;

D O I：

10.1016/j.jqsrt.2019.106687

中图分类号：

O43 [光学];

学科分类号：

070207 ; 0803 ;

摘要：

The simulation of astronomical spectra of cool stars, brown dwarfs and exoplanets requires high resolution line lists and absorption cross sections of many molecules. Similar data sets are needed for the Earth's atmosphere and other planets in our solar system. The requirements for line lists are reviewed and methods used to create them are discussed. Equations to convert between different units are provided. The MoLLIST (Molecular Line Lists, Intensities and Spectra) data compilation is presented and used as an example. (C) 2019 Elsevier Ltd. All rights reserved.

引用

页数：8

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