Project Vera Rubin: Six High-Probability Gravitational Lens Candidates from ZTF Light Curves

An independent pipeline utilizing Z-transformed Discrete Correlation Functions (ZDCF) for time-delay measurements, local Gaia DR3 astrometric masking, and DESI spectroscopic cross-matching to identify galaxy-scale strong gravitational lenses in Zwicky Transient Facility (ZTF) data. This dataset includes the discovery portfolios and coordinate data for six high-probability candidates, notably including WISEA J003903.93+242208.4 with an estimated Singular Isothermal Sphere (SIS) mass of 1.57 x 10^11 solar masses.