A new ‘spectroscopic’ potential energy surface (PES) for14NH3has been generated by refinement of a high accuracy ab initio PES to experimental data. The quality of the PES is reflected in the excellent agreement between calculated rovibrational energy levels and the empirical values of MARVEL. The PES is used in conjunction with two different DMSs to generate room temperature line lists up to 12 000 and 20 000 cm−1, including all transitions from lower states up to 4000 cm−1, with total angular momentum up to J=20. Several strong bands are found to be missing from HITRAN 2016 in the 5700–6200 cm−1 region. Using the line lists, 769 transitions in the 7400–8000 cm−1 are assigned by ground state combination difference (GSCDs), along with empir...
An {\it ab initio} potential energy surface (PES) for NH$_3$ is computed using the methodology pione...
Author Institution: SETI Institute, 189 Bernardo Ave, Suite 100, Mountain View, CA, 94043; MS T27B-1...
Author Institution: Department of Physics and Astronomy, University College London, London, WC1E 6BT...
We present a new spectroscopic potential energy surface (PES) for $^{14}$NH$_3$, produced by refinin...
AbstractThe data incorporated in the HITRAN database for 14NH3 are analyzed using a comprehensive an...
A Fourier Transform (FT) absorption spectrum of room temperature NH3 in the region 7400 - 8600 cm-1 ...
We present a new spectroscopic potential energy surface (PES) for $^{14}$NH$_3$, produced by refinin...
An ab initio potential energy surface (PES) for gas-phase ammonia NH3 has been computed using the me...
Room temperature NH 3 absorption spectra recorded at the Kitt Peak National Solar Observatory in 198...
Room temperature NH3 absorption spectra recorded at the Kitt Peak National Solar Observatory in 1980...
Author Institution: Department of Chemistry, University of York, Heslington, York YO10 5DD, UK; Russ...
Author Institution: Department of Chemistry, University of York, Heslington, York YO10 5DD, UK; Russ...
X. Huang, D.W. Schwenke, and T.J. Lee, \textit{J. Chem. Phys.Author Institution: MS 245-6, NASA Am...
Two sets of NH3 absorption spectra covering the 0.793 μm region are recorded using two Bruker IFS 12...
X. Huang, D.W. Schwenke, and T.J. Lee, \textit{J. Chem. Phys.Author Institution: MS 245-6, NASA Am...
An {\it ab initio} potential energy surface (PES) for NH$_3$ is computed using the methodology pione...
Author Institution: SETI Institute, 189 Bernardo Ave, Suite 100, Mountain View, CA, 94043; MS T27B-1...
Author Institution: Department of Physics and Astronomy, University College London, London, WC1E 6BT...
We present a new spectroscopic potential energy surface (PES) for $^{14}$NH$_3$, produced by refinin...
AbstractThe data incorporated in the HITRAN database for 14NH3 are analyzed using a comprehensive an...
A Fourier Transform (FT) absorption spectrum of room temperature NH3 in the region 7400 - 8600 cm-1 ...
We present a new spectroscopic potential energy surface (PES) for $^{14}$NH$_3$, produced by refinin...
An ab initio potential energy surface (PES) for gas-phase ammonia NH3 has been computed using the me...
Room temperature NH 3 absorption spectra recorded at the Kitt Peak National Solar Observatory in 198...
Room temperature NH3 absorption spectra recorded at the Kitt Peak National Solar Observatory in 1980...
Author Institution: Department of Chemistry, University of York, Heslington, York YO10 5DD, UK; Russ...
Author Institution: Department of Chemistry, University of York, Heslington, York YO10 5DD, UK; Russ...
X. Huang, D.W. Schwenke, and T.J. Lee, \textit{J. Chem. Phys.Author Institution: MS 245-6, NASA Am...
Two sets of NH3 absorption spectra covering the 0.793 μm region are recorded using two Bruker IFS 12...
X. Huang, D.W. Schwenke, and T.J. Lee, \textit{J. Chem. Phys.Author Institution: MS 245-6, NASA Am...
An {\it ab initio} potential energy surface (PES) for NH$_3$ is computed using the methodology pione...
Author Institution: SETI Institute, 189 Bernardo Ave, Suite 100, Mountain View, CA, 94043; MS T27B-1...
Author Institution: Department of Physics and Astronomy, University College London, London, WC1E 6BT...