  We report the results of analyzing Swift, RossiXTE, and INTEGRAL data of
Swift J1922.7-1716, a likely transient X-ray source discovered by Swift/BAT.
Both the fast variability measured by the RXTE/PCA and the combined Swift/XRT,
RXTE/PCA, and INTEGRAL/ISGRI (0.5-100 keV) energy spectrum suggest that the
system is a neutron-star low-mass X-ray binary or a black-hole candidate at low
accretion levels. The non-simultaneous spectra are consistent with the same
spectral shape and flux, suggesting little variability over the period July to
October 2005, but the analysis of archival INTEGRAL data shows that the source
was not detected in 2003-2004, suggesting a transient or strongly variable
behavior.
