  The spotted detached eclipsing binary (DEB) offers insights into starspots on
the binary. Three spotted DEBs, KIC 8097825, KIC 6859813, and KIC 5527172,
which were observed by the Kepler photometry and LAMOST spectroscopy, are
studied in this work. The physical parameters of binaries are determined by
binary modeling. The sizes, lifetimes, and single/double-dip ratio (SDR) of
starspots are derived by starspot analysis. KIC 8097825 has large starspots.
KIC 6859813 has a spot rotation period shorter than its orbital period but the
system should be synchronized inferred from timescale estimation. The
difference may be the result of the surface differential rotation. The KIC
5527172 has a long spot lifetime and an M dwarf component with an inflation
radius. The primaries of these binaries and the secondary of KIC 8097825 have
spots. Adding spotted DEBs of literature, we compare the starspots on binaries
with those on the single stars. The spot sizes of starspots on 65% binaries are
smaller than the median of those on single stars. The lifetimes of starspots on
binaries are consistent with those on single stars when the rotation periods
are larger than 3 days. SDRs for half of the binaries are consistent with those
of single star systems, while another half are smaller. The relative lifetime
positively correlates with the RMS and SDR but negatively correlates with the
rotation period. These relations are similar to those of spots on the single
star systems. Binaries with luminosity ratios close to the unit tend to have
more double dips.
