“…The correction was performed using a spectrum data processing software (GRAMS/AI) and the files containing the relative intensity correction factor. In this study, using the software, baseline correction was performed with liner function between 1,200 and 1,450 cm −1 , and then each CO 2 band was fitted to a Gaussian and Lorentzian mixing curve . Spectra were collected in a single window between 989 and 1,511 cm −1 , which covers the main peaks of the Fermi diad of CO 2 (see Figure ) and six well‐established reference peaks of neon: 18,403.8, 18,353.6, 18,200.3, 18,071.2, 18,054.9, and 17,976.7 cm −1 .…”