The Carnegie Chicago Hubble Program X: Tip of the Red Giant Branch Distances to NGC 5643 and NGC 1404

The primary goal of the Carnegie Chicago Hubble Program (CCHP) is to calibrate zero-point Type Ia supernova (SN Ia) Diagram through use Population II standard candles. So far, CCHP has measured direct distances 11 SNe Ia, and here we increase that number 15 with two new TRGB NGC 5643 1404, for a total 20 SN calibrators. We present resolved, point-source photometry from Space Telescope (HST) imaging these galaxies in F814W F606W bandpasses. From each galaxy's stellar halo, construct an F814W-band luminosity function which detect unambiguous edge feature identified as Tip Red Giant Branch (TRGB). For 5643, find $\mu_0 = 30.48\pm0.03(stat)\pm0.07(sys) $ mag, 1404 \mu_0=31.36\pm 0.04(stat)\pm 0.05(sys)$ mag. preliminary consideration galaxies, increased confidence results presented Paper VIII (Freedman et al. 2019). high precision our enables significant measurement 3D displacement between Fornax Cluster 1316 (Fornax A) equal $1.50^{+0.25}_{-0.39}$ Mpc, show agreement independent literature constraints.