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Chung Chung, a graduate student at Columbia University, presents their recent paper on ultra-short period massive black hole binary candidates in LSST as LISA verification binaries. LSST is expected to discover a large number of quasars, possibly in the millions, triggered by galaxy mergers. A fraction of these quasars may be powered by massive black hole mergers, with a small fraction evolving into LISA frequency band in their late inspiring stage. These verification binaries, similar to galactic white dwarf binaries in LISA, can be computed analytically using assumptions about quasar luminosity functions. They reference the work of George Kokarni et al. 2019.