  In this study, we use archival data from HST, Chandra, XMM-Newton, and
Swift-XRT, to probe the nature of 9 (X1-X9) candidate ULXs in NGC 1672. Our
study focuses on using the precise source positions obtained via improved
astrometry based on {\it Chandra} and HST observations to search for and
identify optical counterparts for these ULXs.Unique optical counterparts are
identified for X2 an{d X6; two potential counterparts were determined for X1,
X5 and X7 within the respective error radii while no optical counterparts were
found for the remaining four sources. Based on spectral energy distributions
(SEDs), X-ray and optical temporal analyses, some evidences about the nature of
X1 and X2 were obtained.
