[en] We present the discovery of eight quasars at $z\sim <!--\; ???\; -->6$ identified in the Sloan Digital Sky Survey (SDSS) overlap regions. Individual SDSS imaging runs have some overlap with each other, leading to repeat observations over an area spanning >4000 deg² (more than one-fourth of the total footprint). These overlap regions provide a unique data set that allows us to select high-redshift quasars more than 0.5 mag fainter in the z band than those found with the SDSS single-epoch data. Our quasar candidates were first selected as i-band dropout objects in the SDSS imaging database. We then carried out a series of follow-up observations in the optical and near-IR to improve photometry, remove contaminants, and identify quasars. The eight quasars reported here were discovered in a pilot study utilizing the overlap regions at high galactic latitude ($|b|><!--\; >\; -->30{}^{\circ <!--\; ???\; -->}$). These quasars span a redshift range of $5.86<<!--\; <\; -->z<<!--\; <\; -->6.06$ and a flux range of $19.3<<!--\; <\; -->z_{\mathrm{A}\mathrm{B}}<<!--\; <\; -->20.6$ mag. Five of them are fainter than $z_{\mathrm{A}\mathrm{B}}=20$ mag, the typical magnitude limit of $z\sim <!--\; ???\; -->6$ quasars used for the SDSS single-epoch images. In addition, we recover eight previously known quasars at $z\sim <!--\; ???\; -->6$ that are located in the overlap regions. These results validate our procedure for selecting quasar candidates from the overlap regions and confirming them with follow-up observations, and they provide guidance to a future systematic survey over all SDSS imaging regions with repeat observations.