Sub-Doppler resolution spectroscopy of CH$_{3}$D has been carried out for the $nu _1$ and $nu _4$ fundamental bands using a comb-referenced difference-frequency generation spectrometer. Thirty transitions from the low-$J''$ and $K'' = 3$ levels are observed with a resolution of 60 to 100 kHz, and the $A_1$-$A_2$ splitting is resolved for twenty-three of the thirty transitions. Most of them are overlapped in Doppler broadening and resolved for the first time, as far as we know. The absolute transition frequencies are determined with a typical uncertainty of 4 kHz. The $A_1$-$A_2$ splitting constant of the $K'' = 3$ levels is yielded as $2h_{3,v=0} = (1.5641 pm 0.0026)$ Hz for the ground vibrational state. Those of the $K' = 3$ levels for the...
$^{a}$C. Ishibashi and H. Sasada, Proc. of 54th Ohio State Univ. Int. Symp. Molec. Spectrosc. RJ04, ...
The near-IR spectrum, from 5000-8960 cm$^{-1}$, of isotopically pure CH$_3$D was taken at temperatur...
Author Institution: Department of Physics and Astronomy, University of Calgary; Steacie Institute fo...
Sub-Doppler resolution spectroscopy of CH$_{3}$D has been carried out for the $nu _1$ and $nu _4$ fu...
$^{a}$ O.N. Ulenikov. S. Alanko. M. Koivusaari. and R. Anttila. Chem. Phys. Lett. 268, p242-248 (199...
$^{a}$ Support by CREST is gratefully acknowledged $^{b}$ M. de Labachelerie, K. Nakagawa, and M. Oh...
D.E.Jennings and W.E.Blass,J.Mol.Spectrosc.,55, 445 (1975). H.C.Allen and E.K.Plyler, J.Res.Natl.Bur...
$^{1}$P. A. Jansson, R. H. Hunt, and R. K. Plyler, J. Opt. Soc. Am. 60,595 (1970). $^{2}$K. T. Hecht...
International audienceThe infrared spectrum of CH3D from 3250 to 3700 cm(-1) was studied for the fir...
The nu sub 2 fundamental band of CHD3, centered near 2143/cm, was recorded at a resolution of 0.015-...
High-energy overtone photoacoustic spectroscopy of gas phase CHD3 (ΔνCH=5,6, and 7), CH2D2, CH3D, an...
We have introduced a wide-beam-coupled enhanced-cavity absorption cell (ECAC) into a 3-$\mu $m diffe...
We report the measurement of sub-Doppler double-resonance transitions in methane using a 3.3 $\mu$m ...
Methane is the first organic molecule detected in hot-Jupiter exoplanets [1] and the observed spectr...
Methane is the first organic molecule detected in hot-Jupiter exoplanets [1] and the observed spectr...
$^{a}$C. Ishibashi and H. Sasada, Proc. of 54th Ohio State Univ. Int. Symp. Molec. Spectrosc. RJ04, ...
The near-IR spectrum, from 5000-8960 cm$^{-1}$, of isotopically pure CH$_3$D was taken at temperatur...
Author Institution: Department of Physics and Astronomy, University of Calgary; Steacie Institute fo...
Sub-Doppler resolution spectroscopy of CH$_{3}$D has been carried out for the $nu _1$ and $nu _4$ fu...
$^{a}$ O.N. Ulenikov. S. Alanko. M. Koivusaari. and R. Anttila. Chem. Phys. Lett. 268, p242-248 (199...
$^{a}$ Support by CREST is gratefully acknowledged $^{b}$ M. de Labachelerie, K. Nakagawa, and M. Oh...
D.E.Jennings and W.E.Blass,J.Mol.Spectrosc.,55, 445 (1975). H.C.Allen and E.K.Plyler, J.Res.Natl.Bur...
$^{1}$P. A. Jansson, R. H. Hunt, and R. K. Plyler, J. Opt. Soc. Am. 60,595 (1970). $^{2}$K. T. Hecht...
International audienceThe infrared spectrum of CH3D from 3250 to 3700 cm(-1) was studied for the fir...
The nu sub 2 fundamental band of CHD3, centered near 2143/cm, was recorded at a resolution of 0.015-...
High-energy overtone photoacoustic spectroscopy of gas phase CHD3 (ΔνCH=5,6, and 7), CH2D2, CH3D, an...
We have introduced a wide-beam-coupled enhanced-cavity absorption cell (ECAC) into a 3-$\mu $m diffe...
We report the measurement of sub-Doppler double-resonance transitions in methane using a 3.3 $\mu$m ...
Methane is the first organic molecule detected in hot-Jupiter exoplanets [1] and the observed spectr...
Methane is the first organic molecule detected in hot-Jupiter exoplanets [1] and the observed spectr...
$^{a}$C. Ishibashi and H. Sasada, Proc. of 54th Ohio State Univ. Int. Symp. Molec. Spectrosc. RJ04, ...
The near-IR spectrum, from 5000-8960 cm$^{-1}$, of isotopically pure CH$_3$D was taken at temperatur...
Author Institution: Department of Physics and Astronomy, University of Calgary; Steacie Institute fo...