Multiwavelength long-term light curve of YZ Ret covering the period 2017-2026, starting in quiescence until the most recent observations. The panel shows the optical evolution from ASAS-SN. Vertical colored regions indicate the epochs of high-cadence TESS observations analyzed by Schaefer (2022) and in this work (TESS Sectors 3, 4, 29, 30, 31, 69, 96, and 97), X-ray observations from Swift, Chandra, and XMM-Newton, and high-speed ground-based photometry from GS/Zorro and SAAO. The light curve illustrates the transition from the post-outburst decline to the current VY Scl-type high state, providing the temporal context for the detected white dwarf spin.