Complied data for specific heat capacity of lunar regolith

This is the complied data for specific heat capacity used in Figure 8 of: Woods‐Robinson, R., Siegler, M. A., &amp; Paige, D. A. (2019). A Model for the Thermophysical Properties of Lunar Regolith at Low Temperatures. <em>Journal of Geophysical Research: Planets</em>, <em>124</em>(7), 1989-2011. Recorded data originally come from papers: Apollo 11 soil 10021: Robie, R. A., Hemingway, B. S., &amp; Wilson, W. H. (1970). Specific heats of lunar surface materials from 90 to 350 degrees Kelvin. <em>Science</em>, <em>167</em>(3918), 749-750. Apollo 14 (14163), 15 (15301), 16 (60601) soils: Hemingway, B. S., Robie, R. A., &amp; Wilson, W. H. (1973). Specific heats of lunar soils, basalt, and breccias from the Apollo 14, 15, and 16 landing sites, between 90 and 350 K. In <em>Lunar and Planetary Science Conference Proceedings</em> (Vol. 4, p. 2481). Breccia Rock 10046: Morrison, J. A., &amp; Norton, P. R. (1970). The heat capacity and thermal conductivity of Apollo 11 lunar rocks 10017 and 10046 at liquid helium temperatures. <em>Journal of Geophysical Research</em>, <em>75</em>(32), 6553-6557.