Reply to Comment by A. G. Davies on “Io Hot Spot Distribution Detected by Juno/JIRAM” by F. Zambon, A. Mura, F. Tosi

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Ring‐Mold Craters on Ceres: Evidence for Shallow Subsurface Water Ice Sources by K. Krohn, A. Neesemann, R. Jaumann, K. A. Otto, K. Stephan, R. J. Wagner, F. Tosi, F. Zambon, O. Ruesch, D. A. Williams, C. A. Raymond, C. T. Russell

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Pitted terrains on (1) Ceres and implications for shallow subsurface volatile distribution by H. G. Sizemore, T. Platz, N. Schorghofer, T. H. Prettyman, M. C. De Sanctis, D. A. Crown, N. Schmedemann, A. Neesemann, T. Kneissl, S. Marchi, P. M. Schenk, M. T. Bland, B. E. Schmidt, K. H. G. Hughson, F. Tosi, F. Zambon, S. C. Mest, R. A. Yingst, D. A. Williams, C. T. Russell, C. A. Raymond

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