Context :

Aims : We aim to find more eclipsing multiple systems and obtain their parameters , thus increasing our understanding of multiple systems .

Methods : The extraneous eclipses on the kepler binary light curves indicating extraneous bodies were searched .
The binary light curves were analyzed using the binary model , and the extraneous eclipses were studied on their periodicity and shape changes .

Results : Three binaries with extraneous eclipses on the binary light curves were found and studied based on the Kepler observations .
The object KIC 5255552 is an eclipsing triple system with a fast changing inner binary and an outer companion uncovered by three groups of extraneous eclipses of 862.1 ( \pm 0.1 ) d period .
The KIC 10091110 is suggested to be a double eclipsing binary system with several possible extraordinary coincidences : the two 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 KIC 11495766 is a probable triple system with a \sim 120.73 d period binary and ( at least ) one non-eclipse companion .
Furthermore , very close to it in the celestial sphere , there is a blended background stellar binary of 8.3404432 d period .
A first list of 25 eclipsing multiple candidates is presented , with the hope that it will be beneficial for study of eclipsing multiples .

Conclusions :