Accurate Wavenumbers for Mid-Infrared Fine-Structure Lines

Abstract
We present accurate new wavenumbers for a set of 13 mid-infrared fine-structure lines. The wavenumbers were determined from observations of the planetary nebula NGC 7027 and of the red supergiant α Scorpii. Most of the new wavenumbers are good to within 0.0025%, or 8 km s-1. We provide details on the measurements and present an analysis of the errors. In addition, we present the first observations of hyperfine splitting in the [Na IV] 1106 cm-1 line.
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