Interior composition, structure and dynamics of the Galilean satellites

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Sulfur's impact on core evolution and magnetic field generation on Ganymede (2005, methodology): “Ganymede is the most centrally concentrated, largely solid body known in the solar system as indicated by the nondimensional polar moment of inertia (C/MR2) of 0.3115 [Schubert et al., 2004].”
Europa’s Surface Composition (2009, background): “Jupiter’s satellites formed from either a warm and dense protojovian nebula or a thin and cold disk (Schubert et al., 2004; chapter by Canup and Ward).”
Geophysical controls of chemical disequilibria in Europa (2016, background): “The thick line for H2 flux corresponds to a rocky seafloor 100 km below Europa’s surface; the shaded region surrounding it portrays uncertainties based on interpretation of Galileo gravity data (80-170 km) [Schubert et al., 2004]).”
Enceladus: Present internal structure and differentiation by early and long-term radiogenic heating (2007, methodology): “For the two-layer model, the basic parameter is the ratio βc of the radius of the rock-metal core to the total radius according to Schubert et al. (2004), (2)ρ = ρs + (ρc − ρs)β3c .”