  We report on the results from our search for the Wide-field Infrared Survey
Explorer detection of the Galactic low-mass X-ray binaries. Among 187 binaries
catalogued in Liu et al. (2007), we find 13 counterparts and two candidate
counterparts. For the 13 counterparts, two (4U~0614+091 and GX~339$-$4) have
already been confirmed by previous studies to have a jet and one (GRS~1915+105)
to have a candidate circumbinary disk, from which the detected infrared
emission arose. Having collected the broad-band optical and near-infrared data
in literature and constructed flux density spectra for the other 10 binaries,
we identify that three (A0620$-$00, XTE J1118+480, and GX 1+4) are candidate
circumbinary disk systems, four (Cen X-4, 4U 1700+24, 3A 1954+319, and Cyg X-2)
had thermal emission from their companion stars, and three (Sco X-1, Her X-1,
and Swift J1753.5$-$0127) are peculiar systems with the origin of their
infrared emission rather uncertain. We discuss the results and WISE
counterparts' brightness distribution among the known LMXBs, and suggest that
more than half of the LMXBs would have a jet, a circumbinary disk, or the both.
