“…The data were originally published and made available 1,5 in 2004, and thousands of copies were distributed on a web site, with many of the molecular absorption cross-sections more recently made available as a new product on the HITRAN web site. 8 The spectral data have been used for applications including ambient 9,10 and laboratory monitoring, 11,12 input to radiative transfer models, 13,14 and other endeavors such as atmospheric chemistry, 15,16 gas-phase chemical kinetics, 17,18 combustion science, 19,20 and even fundamental vibrational assignments. 21 Recently, Bernath, Hewett, and co-workers 22−25 have investigated the structure and band strengths of isobutane, C 4 H 10 , for possible monitoring of this species on gas-giant planets such as Jupiter and Saturn as well as the gas-phase composition of their moons such as Saturn's largest, Titan.…”