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HIGH RESOLUTION INFRARED SPECTROSCOPY OF THE $\nu_{2}$ and $\nu_{4}$ SILANE BANDS

John J. Keady, Don E. Jennings

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Abstract

The Fourier Transform Spectrometer at the McMath complex at Kitt Peak National Observatory has been used to obtain high resolution $(2.5 \\cdot 10^{-3} cm^{-1})$ spectra of the $\\nu_{2}$ and $\\nu_{4}$ bands of silane $(SiH_{4})$. A preliminary linelist along with line strengths will be presented. Silane has recently been detected in an astronomical source, and an application of the laboratory data involving the calculation of a synthetic astronomical spectrum will also be presented.

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What this paper is about

The Fourier Transform Spectrometer at the McMath complex at Kitt Peak National Observatory has been used to obtain high resolution $(2.5 \\cdot 10^{-3} cm^{-1})$ spectra of the $\\nu_{2}$ and $\\nu_{4}$ bands of silane $(SiH_{4})$. A preliminary linelist along with line strengths will be presented. Silane has recently been detected in an astronomical source, and an application of the laboratory data involving the calculation of a synthetic astronomical spectrum will also be presented.

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Available abstract

The Fourier Transform Spectrometer at the McMath complex at Kitt Peak National Observatory has been used to obtain high resolution $(2.5 \\cdot 10^{-3} cm^{-1})$ spectra of the $\\nu_{2}$ and $\\nu_{4}$ bands of silane $(SiH_{4})$. A preliminary linelist along with line strengths will be presented. Silane has recently been detected in an astronomical source, and an application of the laboratory data involving the calculation of a synthetic astronomical spectrum will also be presented.

Key concepts: Infrared spectroscopy, Infrared, Spectroscopy, Resolution (logic), Silane, Materials science, Analytical Chemistry (journal), Chemistry

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