  (abridged) We analysed data from observations of 17 INTEGRAL sources made
with the Swift satellite. We refine the position of the hard X-ray sources to
an accuracy of a few arcsec. We then browsed the online catalogs (e.g., NED,
SIMBAD, 2MASS, 2MASX, USNO) to search for counterparts at other wavelengths. We
also made use of the X-ray spectral parameters to try to identify the nature of
those sources. We provide the X-ray position with arcsec accuracy, identify
possible infrared and optical counterparts (when found), give the magnitudes in
those bands and in the optical and UV as seen with the Swift/UVOT telescope
when observations are available. We confirm the previously suggested
associations and source types for IGR J03532-6829, J05346-5759, J10101-5654,
J13000+2529, J13020-6359, J15479-4529, J18214-1318, and J23206+6431. We
identify
  IGR J09025-6814 as an AGN for the first time, and we suggest that it may be a
Seyfert 2. We suggest that IGR J05319-6601, J16287-5021, J17353-3539 and
J17476-2253 are X-ray binaries, with J05319-6601 being located in the LMC and
the other three possibly being HMXBs in our Galaxy. For IGR J15161-3827 and
J20286+2544, we find several possible X-ray counterparts in the IBIS error
region, and we discuss which, if any, are the likely counterparts. Both are
likely AGNs, although the latter could be a blend of two AGNs. For IGR
J03184-0014 and J19267+1325, we find X-ray sources slightly outside the IBIS
error circle. In the former, we do not favour an association of the Swift and
INTEGRAL source, while it is very likely that IGR J19267+1325 and the Swift
source are the same.
