A spectroscopic census of titanium lines in the near-infrared
Context. The adverse effects of interstellar extinction makes the optical range unsuitable for spectroscopic analysis of stellar populations in dust-obscured regions of the Milky Way. With new instruments available, high-quality spectroscopy in the near-infrared (near-IR or NIR) range is now feasible. However, this region of the electromagnetic spectrum is relatively unexplored for the purpose of
