  The energy levels of the first few low-lying states of carbon in intense
magnetic fields upwards of $\approx 10^7$ T are calculated in this study. We
extend our previously employed pseudospectral approach for calculating the
eigenstates of the carbon atom. We report data for the ground state and a
low-lying state that are in good agreement with findings elsewhere, as well as
new data for ten other states of the carbon atom that have not been
investigated until now. It is seen that these hitherto uninvestigated states
also become strongly bound with increasing magnetic field strengths. The data
presented in this study are relevant for astrophysical applications, such as
magnetized white dwarf and neutron star spectral analysis as well as opacity
calculations and absorption features, including in the context of material
accreting onto the surfaces of these compact objects.
