ExoMol Line List XXI: Nitric Oxide (NO)
arXiv:1705.05955 · doi:10.1093/mnras/stx1211
Abstract
Line lists for the ground electronic ground state for six major isotopologues of nitric oxide are presented. The line lists are constructed using empirical energy levels (and line positions) and high-level {\it ab inito} intensities. The energy levels were obtained using a combination of two approaches, from an effective Hamiltonian and from solving the rovibronic Schrödinger equation variationally. The effective hamiltonian model was obtained through a fit to the experimental line positions of NO available in the literature for all six isotopologues using the programs SPFIT and SPCAT. The variational model was built through a least squares fit of the \textit{ab inito} potential and spin-orbit curves to the experimentally derived energies and experimental line positions of the main isotopologue only using the Duo program. The \textit{ab inito} potential energy, spin-orbit and dipole moment curves (PEC, SOC and DMC) are computed using high-level {\it ab inito} methods and the MARVEL method is used to obtain energies of NO from experimental transition frequencies. Each line list covers a wavenumber range from 0 - 40,000 \cm with approximately 22,000 rovibronic states and 2.3-2.6 million transitions extending to and . Partition functions are also calculated up to a temperature of 5000 K. The calculated absorption line intensities at 296 K using these line lists show excellent agreement with those included in the HITRAN and HITEMP databases. The computed NO line lists are the most comprehensive to date, covering a wider wavenumber and temperature range compared to both the HITRAN and HITEMP databases. These line lists are also more accurate than those used in HITEMP. The full line lists are available from the CDS and ExoMol databases; data will also be available from CDMS.
References in corpus (37)
- CODATA Recommended Values of the Fundamental Physical Constants: 2010
- The ExoMol database: molecular line lists for exoplanet and other hot atmospheres
- ExoMol: molecular line lists for exoplanet and other atmospheres
- The Discovery of Y Dwarfs Using Data from the Wide-field Infrared Survey Explorer (WISE)
- Thermal Emission and Albedo Spectra of Super Earths with Flat Transmission Spectra
- Model atmospheres of irradiated exoplanets: The influence of stellar parameters, metallicity, and the C/O ratio
- A 2 mm spectral line survey of the starburst galaxy NGC 253
- ExoMol line lists XVIII. The high temperature spectrum of VO
- Detection of an atmosphere around the super-Earth 55 Cancri e
- Duo: a general program for calculating spectra of diatomic molecules
- Line Intensities and Molecular Opacities of the FeH Transition
- Simultaneous Detection of Water, Methane and Carbon Monoxide in the Atmosphere of Exoplanet HR8799b
- Water Clouds in Y Dwarfs and Exoplanets
- ExoMol line lists II: The ro-vibrational spectrum of SiO
- ExoMol molecular line lists V: The ro-vibrational spectra of NaCl and KCl
- New CrH Opacities for the Study of L and Brown Dwarf Atmospheres
- ExoMol molecular line lists: IX The spectrum of AlO
- The spectrum of hot methane in astronomical objects using a comprehensive computed line list
- Methane in the atmosphere of the transiting hot Neptune GJ436b?
- ExoMol molecular line lists - XIII: The spectrum of CaO
- Spectroscopic Constants, Abundances, and Opacities of the TiH Molecule
- ExoMol molecular line lists XIX: high accuracy computed hot line lists for HO and HO
- First detections of extragalactic SO2, NS and NO
- The {\it ab initio} calculation of spectra of open shell diatomic molecules
- MARVEL analysis of the measured high-resolution rovibronic spectra of TiO
- ExoMol molecular line lists X: The spectrum of sodium hydride
- Methane and Ammonia in the near-infrared spectra of late T dwarfs
- Radiative lifetimes and cooling functions for astrophysically important molecules
- Experimental energy levels and partition function of the C molecule
- The calculated rovibronic spectrum of scandium hydride, ScH
- ExoMol molecular line lists XII: Line Lists for 8 isotopologues of CS
- The rovibrational spectrum of BeH, MgH and CaH at high temperatures in the state: a theoretical study
- Exomol molecular line lists VI: A high temperature line list for Phosphorus Nitride
- Lightning Chemistry on Earth-like Exoplanets
- Predicted Landé -factors for open shell diatomic molecules
- Terahertz spectroscopy of NO and isotopic invariant fit of several nitric oxide isotopologs
- Revised spectroscopic parameters of SH from ALMA and IRAM 30 m observations
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- The 2020 release of the ExoMol database: molecular line lists for exoplanet and other hot atmospheres
- ExoCross: a general program for generating spectra from molecular line lists
- 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
- Self-luminous and irradiated exoplanetary atmospheres explored with HELIOS
- Spectroscopic line parameters of NO, NO, and NO for the HITEMP database
- PLATON II: New Capabilities And A Comprehensive Retrieval on HD 189733b Transit and Eclipse Data
- ExoMol molecular line lists - XXIII: spectra of PO and PS
- TRIDENT: A Rapid 3D Radiative Transfer Model for Exoplanet Transmission Spectra
- The ExoMol Atlas of Molecular Opacities
- ExoMol line lists XXXI: Spectroscopy of lowest eights electronic states of C
- Laboratory spectra of hot molecules: data needs for hot super-Earth exoplanets
- An update to the MARVEL dataset and ExoMol line list for 12C2
- ExoMol molecular line lists - XXVI: spectra of SH and NS
- ExoMol molecular line lists -- XLII: Rovibronic molecular line list for the low-lying states of NO
- Developing a self-consistent AGB wind model: II. Non-classical, non-equilibrium polymer nucleation in a chemical mixture
- Atmospheric compositions and observability of nitrogen dominated ultra-short period super-Earths
- Data availability and requirements relevant for the Ariel space mission and other exoplanet atmosphere applications
- The NewEra model grid
- A method for the variational calculation of hyperfine-resolved rovibronic spectra of diatomic molecules
- Prebiosignature Molecules Can Be Detected in Temperate Exoplanet Atmospheres with JWST
- A spectroscopic model for the low-lying electronic states of NO
- Diatomic rovibronic transitions as potential probes for proton-to-electron mass ratio across cosmological time
- Vibrationally resolved NO dissociative excitation cross sections by electron impact
- Characterising the Atmosphere of 55 Cancri e: 1D Forward Model Grid for Current and Future JWST Observations
- Submillimeter-wave spectroscopy of the CHO radical