A Fourier Transform (FT) absorption spectrum of room temperature NH3 in the region 7400 - 8600 cm-1 is analysed using a variational line list and ground state energies determined using the MARVEL procedure. The spectrum was measured by Dr Catherine de Bergh in 1980 and is available from the Kitt Peak data center. The centers and intensities of 8468 ammonia lines were retrieved using a multiline fitting procedure. 2474 lines are assigned to 21 bands providing 1692 experimental energies in the range 7000 - 9000 cm-1. The spectrum was assigned by the joint use of the BYTe variational line list and combination differences. The assignments and experimental energies presented in this work are the first for ammonia in the region 7400 - 8600 cm-1, ...
AbstractThe data incorporated in the HITRAN database for 14NH3 are analyzed using a comprehensive an...
Ammonia (NH$_3$) has been found ubiquitous, $it{e.g.}$, in the interstellar medium, low-mass stars, ...
Author Institution: Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Dr...
Two sets of NH3 absorption spectra covering the 0.793 μm region are recorded using two Bruker IFS 12...
High-resolution absorption spectra of NH3 in the region 2100–5500 cm⁻¹ at 1027 °C and approximately ...
Infrared absorption spectra of NH3 have been obtained at high resolution (0.02 cm−1) at seven temper...
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...
International audienceRoom temperature absorption spectra of ammonia were recorded by high-resolutio...
International audienceRoom temperature absorption spectra of ammonia were recorded by high-resolutio...
Room temperature NH3 absorption spectra recorded at the Kitt Peak National Solar Observatory in 1980...
Ammonia (NH$_3$) has been found ubiquitous, $it{e.g.}$, in the interstellar medium, low-mass stars, ...
Room temperature NH 3 absorption spectra recorded at the Kitt Peak National Solar Observatory in 198...
Ammonia is an important “weed” molecule in interstellar medium, planetary and exoplanetary atmospher...
A new ‘spectroscopic’ potential energy surface (PES) for14NH3has been generated by refinement of a h...
AbstractThe data incorporated in the HITRAN database for 14NH3 are analyzed using a comprehensive an...
Ammonia (NH$_3$) has been found ubiquitous, $it{e.g.}$, in the interstellar medium, low-mass stars, ...
Author Institution: Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Dr...
Two sets of NH3 absorption spectra covering the 0.793 μm region are recorded using two Bruker IFS 12...
High-resolution absorption spectra of NH3 in the region 2100–5500 cm⁻¹ at 1027 °C and approximately ...
Infrared absorption spectra of NH3 have been obtained at high resolution (0.02 cm−1) at seven temper...
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...
International audienceRoom temperature absorption spectra of ammonia were recorded by high-resolutio...
International audienceRoom temperature absorption spectra of ammonia were recorded by high-resolutio...
Room temperature NH3 absorption spectra recorded at the Kitt Peak National Solar Observatory in 1980...
Ammonia (NH$_3$) has been found ubiquitous, $it{e.g.}$, in the interstellar medium, low-mass stars, ...
Room temperature NH 3 absorption spectra recorded at the Kitt Peak National Solar Observatory in 198...
Ammonia is an important “weed” molecule in interstellar medium, planetary and exoplanetary atmospher...
A new ‘spectroscopic’ potential energy surface (PES) for14NH3has been generated by refinement of a h...
AbstractThe data incorporated in the HITRAN database for 14NH3 are analyzed using a comprehensive an...
Ammonia (NH$_3$) has been found ubiquitous, $it{e.g.}$, in the interstellar medium, low-mass stars, ...
Author Institution: Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Dr...