Ames-296K Infrared Line Lists for Nitrous Oxide (N2O) and isotopologues (Ames-1 PES & DMS based)

[Supplementary data files to "Highly Accurate Potential Energy Surface and Dipole Moment Surface for Nitrous Oxide and Ames-296K Infrared Line Lists for ¹⁴N₂¹⁶O and Minor Isotopologues"]

First generation of Ames-296K Infrared line lists computed for each of 12 N₂O isotopologues of ^14/15N and ^16/17/18O in the full range of 0 – 15,000 cm^-1, with E' up to 20,000 cm^-1and intensity cutoff 1 x 10^-31 cm^-1/molecule.cm^-2 at room temperature (296 K), computed using Ames-1 PES (refined) and DMS. Each line list contains 1.3 – 1.6 million transitions. A 'natural' N₂O line list includes 3.19 million lines from all N₂O isotopologues with intensities scaled by their terrestrial abundances. Compared to HITRAN, HITEMP, NOSL-296, and recent high-resolution experiments. the line lists provide much more complete coverage, plus more reliable and more consistent predictions for those bands missing from current databases, e.g., weaker bands, high energy bands, or minor isotopologue bands. These line lists will enable the N₂O IR spectral analysis and opacity simulation required to enhance the scientific return from astronomical observations, and facilitate the chracterization of astrophysics environments containing N₂O, which is one of the important potential biosignature molecules in the atmosphere of those exoplanets that reside in habitable zones. These are the first-generation, highly accurate IR line lists generated from studies funded by NASA Grant 18-APRA18-0013 through NASA/SETI Institute Co-operative Agreement 80NSSC20K1358. See https://huang.seti.org/N2O/n2o.html and https://doi.org/10.5281/zenodo.7888194 for data format and abundance information.