  We report on Chandra observations of 18 hard X-ray (>20 keV) sources
discovered with the INTEGRAL satellite near the Galactic plane. For 14 of the
INTEGRAL sources, we have uncovered one or two potential Chandra counterparts
per source. These provide soft X-ray (0.3-10 keV) spectra and sub-arcsecond
localizations, which we use to identify counterparts at other wavelengths,
providing information about the nature of each source. Despite the fact that
all of the sources are within 5 degrees of the plane, four of the IGR sources
are AGN (IGR J01545+6437, IGR J15391-5307, IGR J15415-5029, and IGR
J21565+5948) and four others are likely AGN (IGR J03103+5706, IGR J09189-4418,
IGR J16413-4046, and IGR J16560-4958) based on each of them having a strong IR
excess and/or extended optical or near-IR emission. We compare the X-ray and
near-IR fluxes of this group of sources to those of AGN selected by their 2-10
keV emission in previous studies and find that these IGR AGN are in the range
of typical values. There is evidence in favor of four of the sources being
Galactic (IGR J12489-6243, IGR J15293-5609, IGR J16173-5023, and IGR
J16206-5253), but only IGR J15293-5609 is confirmed as a Galactic source as it
has a unique Chandra counterpart and a parallax measurement from previous
optical observations that puts its distance at 1.56+/-0.12 kpc. The 0.3-10 keV
luminosity for this source is 1.4e32 erg/s, and its optical/IR spectral energy
distribution is well described by a blackbody with a temperature of 4200-7000 K
and a radius of 12.0-16.4 Rsun. These values suggest that IGR J15293-5609 is a
symbiotic binary with an early K-type giant and a white dwarf accretor. We also
obtained likely Chandra identifications for IGR J13402-6428 and IGR
J15368-5102, but follow-up observations are required to constrain their source
types.
