2016
DOI: 10.1016/j.jms.2016.06.011
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Far-infrared 14NH3 line positions and intensities measured with a FT-IR and AILES beamline, Synchrotron SOLEIL

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Cited by 16 publications
(11 citation statements)
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“…Since this molecule is of great interest in astrophysical observations, its inversion-rotation spectra within the ground and excited vibrational states were the subjects of many works (see, e.g. , refs and references therein). Among the early results on the study of infrared spectra, let us cite the works by Urban et al where the low-lying fundamental band v 2 was studied using an effective vibration-inversion-rotation Hamiltonian.…”
Section: Validationmentioning
confidence: 99%
“…Since this molecule is of great interest in astrophysical observations, its inversion-rotation spectra within the ground and excited vibrational states were the subjects of many works (see, e.g. , refs and references therein). Among the early results on the study of infrared spectra, let us cite the works by Urban et al where the low-lying fundamental band v 2 was studied using an effective vibration-inversion-rotation Hamiltonian.…”
Section: Validationmentioning
confidence: 99%
“…On the basis of quantum chemical calculations, the and fundamentals are expected to be around 195 and 235 cm , respectively. Even though, for the latter one, the transition frequency has been experimentally confirmed by the observation of the difference band, the recording of their spectra may require a dedicated investigation through, e.g., the use of synchrotron radiation facilities [ 81 , 82 ]. Furthermore, at room temperature, the two lowest-lying vibrational levels and present a relative population of approximately 39% and 32%, respectively, with respect to the ground vibrational state.…”
Section: Results and Discussionmentioning
confidence: 99%
“…A number of new ammonia spectra have been reported in the last two years [8,9,10,11,12,13,14]. Of particular relevance to this work is the analysis by Barton et al [12] of a near-infrared Fourier transform spectrum [15], energy levels from the MARVEL study, and the method of branches [16] to assign 2474 lines in the 7400 -8600 cm −1 region; this is the first time any assignments had been made for ammonia spectra in this region.…”
Section: Introductionmentioning
confidence: 88%