The progress achieved over the last few years in variational Multiconf
iguration Hartree-Fock and Configuration Interaction calculations is r
eviewed. The high level of accuracy which can be reached in the ab ini
tio calculation of atomic properties of light systems is illustrated t
hrough the results of calculations of isotope shifts, hyperfine struct
ures and transition probabilities. The active space method and associa
ted restricted active space methods allowing systematic calculations f
rom which the accuracy of the studied property can be estimated will b
e discussed. We exemplify quality checks through results in small syst
ems for which spectroscopic accuracy is often required For transition
probabilities, recent progress derived from new algorithm developments
allowing independent optimization of the states is emphasized.