Empirical Line Lists in the ExoMol Database
arXiv:2002.06939 · doi:10.3390/atoms8010007
Abstract
The ExoMol database aims to provide comprehensive molecular line lists for exoplanetary and other hot atmospheres. The data are expanded by inclusion of empirically derived line lists taken from the literature for a series of diatomic molecules, namely CH, NH, OH, AlCl, AlF, OH, CaF, MgF, KF, NaF, LiCl, LiF, MgH, TiH, CrH, FeH, C, CP, CN, CaH, and triplet N. Generally, these line lists are constructed from measured spectra using a combination of effective rotational Hamiltonian models for the line positions and ab initio (transition) dipole moments to provide intensities. This work results in the inclusion of 22 new molecules (36 new isotopologues) in the ExoMol database.
References in corpus (28)
- The Cologne Database for Molecular Spectroscopy, CDMS, in the Virtual Atomic and Molecular Data Centre, VAMDC
- The ExoMol database: molecular line lists for exoplanet and other hot atmospheres
- ExoMol: molecular line lists for exoplanet and other atmospheres
- A variationally computed line list for hot NH3
- Planetary Spectrum Generator: an accurate online radiative transfer suite for atmospheres, comets, small bodies and exoplanets
- ExoMol line lists III: An improved hot rotation-vibration line list for HCN and HNC
- CH in stellar atmospheres: an extensive linelist
- The 2020 release of the ExoMol database: molecular line lists for exoplanet and other hot atmospheres
- Duo: a general program for calculating spectra of diatomic molecules
- ExoCross: a general program for generating spectra from molecular line lists
- Line Intensities and Molecular Opacities of the FeH Transition
- Line strengths and updated molecular constants for the C2 Swan system
- Partition functions and equilibrium constants for diatomic molecules and atoms of astrophysical interest
- A room temperature CO line list with ab initio computed intensities
- CRIRES spectroscopy and empirical line-by-line identification of FeH molecular absorption in an M dwarf
- Spectroscopic Constants, Abundances, and Opacities of the TiH Molecule
- The ExoMol project: Software for computing large molecular line lists
- Molecular astronomy of cool stars and sub-stellar objects
- The {\it ab initio} calculation of spectra of open shell diatomic molecules
- ExoMol line lists XXXI: Spectroscopy of lowest eights electronic states of C
- The spectrum of N from 4,500 to 15,700 cm revisited with PGOPHER
- Laboratory spectra of hot molecules: data needs for hot super-Earth exoplanets
- Radiative lifetimes and cooling functions for astrophysically important molecules
- Experimental energy levels and partition function of the C molecule
- Predicted Landé -factors for open shell diatomic molecules
- Ab initio calculations to support accurate modelling of the rovibronic spectroscopy calculations of vanadium monoxide (VO)
- Analysis of first overtone bands of isotopologues of CO and SiO in stellar spectra
- Spectral line lists of a nitrogen gas discharge for wavelength calibration in the range cm
Cited by in corpus (13)
- The 2020 release of the ExoMol database: molecular line lists for exoplanet and other hot atmospheres
- The ExoMolOP Database: Cross-sections and k-tables for Molecules of Interest in High-Temperature Exoplanet Atmospheres
- Aluminium oxide in the atmosphere of hot Jupiter WASP-43b
- The TW Hya Rosetta Stone Project II: Spatially resolved emission of formaldehyde hints at low-temperature gas-phase formation
- ExoMol line lists -- XLV. Rovibronic molecular line lists of calcium monohydride (CaH) and magnesium monohydride (MgH)
- Experimental energy levels of 12C14N through MARVEL analysis
- Spectroscopy on the Transition of Buffer-Gas Cooled AlCl
- Data availability and requirements relevant for the Ariel space mission and other exoplanet atmosphere applications
- ExoMol line lists -- XL. Ro-vibrational molecular line list for the hydronium ion (HO)
- Computational Infrared Spectroscopy of 958 Phosphorus-bearing Molecules
- Radial and vertical constraints on the icy origin of HCO in the HD 163296 Protoplanetary Disk
- Molecular diatomic spectroscopy data
- Hyperfine structure of the state of AlCl and its relevance to laser cooling and trapping