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We present a list of galaxy-scale lens candidates including a highly probableinteracting galaxy-scale lens in the Hyper Suprime-Cam (HSC) imaging survey. Wecombine HSC imaging with the blended-spectra catalog from the Galaxy And MassAssembly (GAMA) survey to identify lens candidates, and use lens mass modelingto confirm the candidates. We find 46 matches between the HSC S14A_0b imagingdata release and the GAMA catalog. Ten of them are probable lens systemsaccording to their morphology and redshifts. There is one system with aninteracting galaxy pair, HSC J084928+000949, that has a valid mass model. Wepredict the total mass enclosed by the Einstein radius of $\sim0.72$"($\sim1.65$kpc) for this new expected lens system to be$\sim10^{10.59}M_{\odot}$. Using the photometry in the {\it grizy} bands of theHSC survey and stellar population synthesis modeling with a Salpeter stellarinitial mass function, we estimate the stellar mass within the Einstein radiusto be $\sim10^{10.46}\,M_{\odot}$. We thus find a dark matter mass fractionwithin the Einstein radius of $\sim25\%$. Further spectroscopy orhigh-resolution imaging would allow confirmation of the nature of these lenscandidates. The particular system with the interacting galaxy pair, ifconfirmed, would provide an opportunity to study the interplay between darkmatter and stars as galaxies build up through hierarchical mergers.

Galaxy-scale gravitational lens candidates from the Hyper Suprime-Cam imaging survey and the Galaxy And Mass Assembly spectroscopic survey