  Next-to-Minimal Supersymmetric Standard Model neutralino dark matter
candidates in the (1-15) GeV range are found with a Markov Chain Monte Carlo
scanning code. A very light, singlet-like Higgs and/or CP-odd Higgs is needed
in order to achieve such light masses. Light scalar Higgses can yield large
direct detection cross sections, suitable for an account of the recent claims
for signals. Neutralino annihilations via resonant light pseudoscalar Higgs
exchanges can overproduce the indirect yield of gamma-rays from dwarf
spheroidal galaxies. Hence, direct and indirect detection experiments probe
different configurations of the NMSSM with a light neutralino DM candidate.
