Improved near-infrared methane band models and k-distribution parameters from 2000 to 9500 cm−1 and implications for interpretation of outer planet spectra
P. G. J. Irwin(University of Oxford), J. J. Remedios(University of Leicester), Kimberly Strong(University of Toronto), K. Sihra(Government of the United Kingdom), S. B. Calcutt(University of Oxford), Neil E. Bowles(University of Oxford), L. A. Sromovsky(University of Wisconsin–Madison), N. A. Teanby(University of Bristol)
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