The goal of this conference is to share a diverse range of scientific perspectives, both on the discoveries that VLASS can make in its own right, and on the advances that can come from the synergy of VLASS with other datasets. Opportunities for multiwavelength VLASS synergy include radio/mm observatories (e.g. ALMA) and surveys (e.g. EMU, Apertif), widefield imaging and spectroscopy (e.g. Roman, Euclid, DESI, PFS), multi-epoch surveys (e.g. ZTF, PanSTARRS, and LSST), and the high-energy domain (e.g. eROSITA).