Folded Gaia G, G_BP, and G_RP photometry and RV data of HD 23692, together with TESS binned data. Top panel: Gaia RV data, while the second panel presents the Gaia G data. Third panel: Gaia G_BP and G_RP data, with medians shifted to the Gaia G median for clarity, and the bottom panel presents the TESS data binned to 200 phase bins. All plots were folded using the Gaia EB-model period and deeper-eclipse epoch as the folding period and phase zero, respectively. We note that the primary eclipse is at phase 0.5, while the secondary eclipse is at phase zero. Observed TESS-eclipse phase drift is due to the more than 1300 day delay from the last Gaia point to the first TESS point. For clarity, the three bottom panels use the same y-axis scale.