Identification of large (2–10 km) rayed craters on Mars in THEMIS thermal infrared images: Implications for possible Martian meteorite source regionsL. L. Tornabene, P. R. Christensen, J. L. Piatek et al.|Journal of Geophysical Research Atmospheres|2006Cited by 116
Surface and crater‐exposed lithologic units of the Isidis Basin as mapped by coanalysis of THEMIS and TES derived data productsL. L. Tornabene, P. R. Christensen, J. E. Moersch et al.|Journal of Geophysical Research Atmospheres|2008Cited by 109