  Gaia DR3 provides >181, 000 radial velocity solutions for single-lined
spectroscopic binaries (SB1s) which can be used to search for non-interacting
compact object+star binary candidates by selecting systems with large mass
functions. We selected 234 such systems and identified 114 systems with good RV
solutions in DR3. We used light curves from ASAS-SN and TESS to identify and
remove 31 eclipsing binaries to produce a catalog of 80 compact object+star
candidates, including 38 ellipsoidal variables. The positions of these
candidates on Gaia and 2MASS CMDs suggest that many of these systems are
binaries with luminous companions. We compared the periods and eccentricities
of detached eclipsing binaries in Gaia DR3 and ASAS-SN, and found that ~11% and
~60% of the binaries had different periods and eccentricities. We also compared
RV solutions for 311 binaries in both Gaia DR3 and the Ninth Catalog of
Spectroscopic Binary Orbits (SB9), and found similar results. We do not
identify any strong candidates for non-interacting compact object+star
binaries.
