deletions | additions       diff --git a/section_Datasets_While_various_very__.tex b/section_Datasets_While_various_very__.tex  index 3ab1c40..3389274 100644  --- a/section_Datasets_While_various_very__.tex  +++ b/section_Datasets_While_various_very__.tex 
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\section{Datasets}  While various very-high ($\lambda/\delta\lambda>50\,000$) resolution spectrographs covering most or all of the near-infrared domain at once are currently under design or construction (e.g., Carmenes, SPIRou, PRVS), none is currently in operation. As a result, very-high resolution spectra available in archives only cover relatively short wavelength intervals. The only publicly available spectrum of an M dwarf at a resolution sufficient to resolve the intrinsic stellar line width ($\sim5\,km/s$ or $\lambda/\delta\lambda>60\,000$) is that available through the CRIRE-POP\footnote{http://www.univie.ac.at/crirespop/} spectral library for the Barnard star ({\color{red} refcrirespop}). These observations cover the entire $Y$, $J$, $H$, $K_s$, $L$ and $M$ bands; of specific interest here being the $\lt 2.38\mu$m domain that is amenable to m/s-level accuracy velocimetry.