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We analyze the anomalies appearing in the light curves of the threemicrolensing events MOA-2022-BLG-563, KMT-2023-BLG-0469, and KMT-2023-BLG-0735.The anomalies exhibit common short-term dip features that appear near the peak.From the detailed analyses of the light curves, we find that the anomalies wereproduced by planets accompanied by the lenses of the events. For all threeevents, the estimated mass ratios between the planet and host are on the orderof $10^{-4}$: $q\sim 8 \times 10^{-4}$ for MOA-2022-BLG-563L, $q\sim 2.5\times10^{-4}$ for KMT-2023-BLG-0469L, and $q\sim 1.9\times 10^{-4}$ forKMT-2023-BLG-0735L. The interpretations of the anomalies are subject to acommon inner-outer degeneracy, which causes ambiguity when estimating theprojected planet-host separation. We estimated the planet mass, $M_{\rm p}$,host mass, $M_{\rm h}$, and distance, $D_{\rm L}$, to the planetary system byconducting Bayesian analyses using the observables of the events. The estimatedphysical parameters of the planetary systems are $(M_{\rm h}/M_\odot, M_{\rmp}/M_{\rm J}, D_{\rm L}/{\rm kpc}) = (0.48^{+0.36}_{-0.30},0.40^{+0.31}_{-0.25}, 6.53^{+1.12}_{-1.57})$ for MOA-2022-BLG-563L,$(0.47^{+0.35}_{-0.26}, 0.124^{+0.092}_{-0.067}, 7.07^{+1.03}_{-1.19})$ forKMT-2023-BLG-0469L, and $(0.62^{+0.34}_{-0.35}, 0.125^{+0.068}_{-0.070},6.26^{+1.27}_{-1.67})$ for KMT-2023-BLG-0735L. According to the estimatedparameters, all planets are cold planets with projected separations that aregreater than the snow lines of the planetary systems, they have masses that liebetween the masses of Uranus and Jupiter of the Solar System, and the hosts ofthe planets are main-sequence stars that are less massive than the Sun.

MOA-2022-BLG-563Lb, KMT-2023-BLG-0469Lb, and KMT-2023-BLG-0735Lb: Three sub-Jovian-mass microlensing planets