  In this paper, we present some relativistic mean-field inner crust equations
of state that have recently been uploaded in the CompOSE online repository.
These equations of state fulfill experimental and microscopic constraints, and
are also able to reproduce two solar-mass stars. We integrate the TOV equations
to obtain the mass-radius relation, and we also calculate the tidal
deformability, compactness, and effective tidal deformability to compare with
the latest astrophysical data from NICER and LIGO and Virgo.
