Exomol molecular line lists VI: A high temperature line list for Phosphorus Nitride
arXiv:1504.02804 · doi:10.1093/mnras/stu1854
Abstract
Accurate rotational-vibrational line lists for PN and PN in their ground electronic states are computed. The line lists are produced using an empirical potential energy curve obtained by fitting to the experimental transition frequencies available in the literature in conjunction with an accurate, high level \textit{ab initio} dipole moment curve. In these calculations the programs DPotFit and LEVEL~8.0 were used. The new line lists reproduce the experimental wavenumbers with a root-mean-square error of 0.004~cm. The line lists cover the frequency range 0--51000 cm, contain almost 700~000 lines each and extend up to a maximum vibrational level of =66 and a maximum rotational level of =357. They should be applicable for a large range of temperature up to, at least, 5000~K. These new line lists are used to simulate spectra for PN at a range of temperatures and are deposited in the Strasbourg data centre. This work is performed as part of the ExoMol project.
arXiv comment12 pages. 5 figures, 8 Tables
References in corpus (5)
- ExoMol: molecular line lists for exoplanet and other atmospheres
- ExoMol line lists II: The ro-vibrational spectrum of SiO
- ExoMol molecular line lists V: The ro-vibrational spectra of NaCl and KCl
- Temperature-dependent molecular absorption cross sections for exoplanets and other atmospheres
- The rovibrational spectrum of BeH, MgH and CaH at high temperatures in the state: a theoretical study
Cited by in corpus (30)
- The ExoMol database: molecular line lists for exoplanet and other hot atmospheres
- Early Release Science of the Exoplanet WASP-39b with JWST NIRSpec G395H
- 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
- HELIOS-K 2.0 Opacity Calculator and Open-source Opacity Database for Exoplanetary Atmospheres
- ExoMol molecular line lists: IX The spectrum of AlO
- ExoMol molecular line lists - XIII: The spectrum of CaO
- ExoMol molecular line lists - XXIII: spectra of PO and PS
- The ExoMol project: Software for computing large molecular line lists
- ExoMol Line List XXI: Nitric Oxide (NO)
- TRIDENT: A Rapid 3D Radiative Transfer Model for Exoplanet Transmission Spectra
- The {\it ab initio} calculation of spectra of open shell diatomic molecules
- The ExoMol Atlas of Molecular Opacities
- ExoMol molecular line lists X: The spectrum of sodium hydride
- ExoMol molecular line lists XX: a comprehensive line list for H
- Radiative lifetimes and cooling functions for astrophysically important molecules
- Laboratory spectra of hot molecules: data needs for hot super-Earth exoplanets
- Relativistic Internally Contracted Multireference Electron Correlation Methods
- The calculated rovibronic spectrum of scandium hydride, ScH
- ExoMol molecular line lists XII: Line Lists for 8 isotopologues of CS
- Exoplanet atmosphere retrievals in 3D using phase curve data with ARCiS: application to WASP-43b
- ExoMol line lists XXV: A hot line list for silicon sulphide, SiS
- Low-Temperature Gas Opacities with AESOPUS 2.0
- ExoMol line list XXXIV: A Rovibrational Line List for Phosphinidene (PH) in its and Electronic States
- The NewEra model grid
- Computational Infrared Spectroscopy of 958 Phosphorus-bearing Molecules
- Rovibronic spectroscopy of PN from first principles
- Molecular line shape parameters for exoplanetary atmospheric applications
- Characterising the Atmosphere of 55 Cancri e: 1D Forward Model Grid for Current and Future JWST Observations
- A grid of self-consistent MSG (MARCS-StaticWeather-GGchem) cool stellar, sub-stellar, and exoplanetary model atmospheres