Semi-classical H2-broadening coefficients of 12CH3D rovibrational lines and their temperature dependence for planetary atmosphere modeling
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Theoretical J and K dependences of CH3D-H2 line-broadening coefficients.

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Temperature exponents for the range of atmospheric interest 200–300 K.

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Negligible vibrational and sub-branch dependence of CH3D-H2 line-widths.

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