In this work, we present the spectral analysis of 1 H- and 2 H-1,2,3-triazole vibrationally excited states alongside provisional and practical computational predictions of the excited-state quartic centrifugal distortion constants. The low-energy fundamental vibrational states of 1 H-1,2,3-triazole and five of its deuteriated isotopologues ([1- 2 H]-, [4- 2 H]-, [5- 2 H]-, [4,5- 2 H]-, and [1,4,5- 2 H]-1 H-1,2,3-triazole), as well as those of 2 H-1,2,3-triazole and five of its deuteriated isotopologues ([2- 2 H]-, [4- 2 H]-, [2,4- 2 H]-, [4,5- 2 H]-, and [2,4,5- 2 H]-2 H-1,2,3-triazole), are studied using millimeter-wave spectroscopy in the 130–375 GHz frequency region. The normal and [2- 2 H]-isotopologues of 2 H-1,2,3-triazole are also analyzed using high-resolution infrared spectroscopy, determining the precise energies of three of their low-energy fundamental states. The resulting spectroscopic constants for each of the vibrationally excited states are reported for the first time. Coupled-cluster vibration–rotation interaction constants are compared with each of their experimentally determined values, often showing agreement within 500 kHz. Newly available coupled-cluster predictions of the excited-state quartic centrifugal distortion constants based on fourth-order vibrational perturbation theory are benchmarked using a large number of the 1,2,3-triazole tautomer isotopologues and vibrationally excited states studied.
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LIGHTCURVES AND ROTATIONAL PERIODS OF FOUR MAIN BELT ASTERIODS
Lightcurves and rotational periods were determined for the following four asteroids: 1120 Cannonia: 3.810 ± 0.003 h; 6801 Strekov: 6.171 ± 0.016 h; (28885) 2000 KH56: 3.326 ± 0.001 h; and 87312 Akirasuzuki: 3.0439 ± 0.0007 h.
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- Award ID(s):
- 1643567
- PAR ID:
- 10187905
- Date Published:
- Journal Name:
- The Minor planet bulletin
- Volume:
- 47
- ISSN:
- 1052-8091
- Page Range / eLocation ID:
- 166-167
- Format(s):
- Medium: X
- Sponsoring Org:
- National Science Foundation
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