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Aims. We aim to find more eclipsing multiple systems and obtain theirparameters, thus increasing our understanding of multiple systems.  Methods. The extraneous eclipses on the \textit{kepler} binary light curvesindicating extraneous bodies were searched. The binary light curves wereanalyzed using the binary model, and the extraneous eclipses were studied ontheir periodicity and shape changes.  Results. Three binaries with extraneous eclipses on the binary light curveswere found and studied based on the \textit{Kepler} observations. The objectKIC 5255552 is an eclipsing triple system with a fast changing inner binary andan outer companion uncovered by three groups of extraneous eclipses of$862.1(\pm0.1)$ d period. The KIC 10091110 is suggested to be a doubleeclipsing binary system with several possible extraordinary coincidences: thetwo binaries share similar extremely small mass ratios ($0.060(13)$ and$0.0564(18)$), similar mean primary densities ($0.3264(42)\;\rho_\odot$ and$0.3019(28)\;\rho_\odot$), and, most notably, the ratio of the two binaries'periods is very close to integer 2 (8.5303353/4.2185174 = 2.022). The KIC11495766 is a probable triple system with a $\sim120.73$ d period binary and(at least) one non-eclipse companion. Furthermore, very close to it in thecelestial sphere, there is a blended background stellar binary of 8.3404432 dperiod. A first list of 25 eclipsing multiple candidates is presented, with thehope that it will be beneficial for study of eclipsing multiples.

The extraneous eclipses on binary light curves: KIC 5255552, KIC 10091110, and KIC 11495766