Cite
An empirical line list for methane in the 1.26–1.71μm region for planetary investigations (T =80–300K). Application to Titan
MLA
Campargue, Alain, et al. “An Empirical Line List for Methane in the 1.26–1.71μm Region for Planetary Investigations (T =80–300K). Application to Titan.” ICARUS, vol. 219, no. 1, May 2012, pp. 110–28. EBSCOhost, https://doi.org/10.1016/j.icarus.2012.02.015.
APA
Campargue, A., Wang, L., Mondelain, D., Kassi, S., Bézard, B., Lellouch, E., Coustenis, A., Bergh, C. de, Hirtzig, M., & Drossart, P. (2012). An empirical line list for methane in the 1.26–1.71μm region for planetary investigations (T =80–300K). Application to Titan. ICARUS, 219(1), 110–128. https://doi.org/10.1016/j.icarus.2012.02.015
Chicago
Campargue, Alain, Le Wang, Didier Mondelain, Samir Kassi, Bruno Bézard, Emmanuel Lellouch, Athena Coustenis, Catherine de Bergh, Mathieu Hirtzig, and Pierre Drossart. 2012. “An Empirical Line List for Methane in the 1.26–1.71μm Region for Planetary Investigations (T =80–300K). Application to Titan.” ICARUS 219 (1): 110–28. doi:10.1016/j.icarus.2012.02.015.