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The infrared solar spectrum contains a wealth of physical data about the Sunand is being explored using modern detectors and technology with newground-based solar telescopes. One such instrument will be the ground-basedCryogenic Near-IR Spectro-Polarimeter of the Daniel K. Inouye Solar Telescopethat will be capable of sensitive imaging of the faint infrared solar coronalspectra with full Stokes I, Q, U, and V polarization states. Highly ionizedmagnetic dipole emission lines have been observed in galaxies and the solarcorona. Quantifying the accuracy of spectral inversion procedures requires aprecise spectroscopic calibration of observations. A careful interpretation ofthe spectra around prominent magnetic dipole lines is essential for derivingphysical parameters, and particularly, for quantifying the off-limb solarcoronal observations from DKIST. In this work, we aim to provide an analysis ofthe spectral regions around the infrared coronal emission lines of Fe XIII1074.68 nm, Fe XIII 1079.79 nm, Si X 1430.10 nm, and Si IX 3934.34 nm, aligningwith the goal of identifying solar photospheric and telluric lines that willhelp facilitate production of reliable inversions and data products from foursets of solar coronal observations. The outputs will be integrated in theprocessing pipeline to produce Level-2 science-ready data that will be madeavailable to DKIST observers.

A spectroscopic survey of infrared 1-4{\mu}m spectra in regions of prominent solar coronal emission lines of Fe XIII, Si X, and Si IX