  The results of Chandra snapshot observations of 11 LINERs (Low-Ionization
Nuclear Emission-line Regions), three low-luminosity Seyfert galaxies, and one
HII-LINER transition object are presented. Our sample consists of all the
objects with a flat or inverted spectrum compact radio core in the VLA survey
of 48 low-luminosity AGN (LLAGN) by Nagar et al. (2000). An X-ray nucleus is
detected in all galaxies except one and their X-ray luminosities are in the
range 5x10^38 to 8x10^41 ergs s^-1. The X-ray to Halpha luminosity ratios for
11 out of 14 objects are in good agreement with the value characteristic of
LLAGNs and more luminous AGNs, and indicate that their optical emission lines
are predominantly powered by a LLAGN. For three objects, this ratio is less
than expected. Comparing with multi-wavelength results, we find that these
three galaxies are most likely to be heavily obscured AGN. We compare the radio
to X-ray luminosity ratio of LLAGNs with those of more-luminous AGNs, and
confirm the suggestion that a large fraction of LLAGNs are radio loud.
