  We present a rest-frame composite spectrum for Seyfert 1 galaxies using
spectra obtained from the DR12 release of the Sloan Digital Sky Survey (SDSS).
The spectrum is constructed by combining data from a total of 10,112 galaxies,
spanning a redshift range of 0 to 0.793. We produce an electronic table of the
median and geometric mean composite Seyfert 1 spectrum. We measure the spectral
index of the composite spectrum, and compare it with that of the composite
quasar spectrum. We also measure the flux and width of the strong emission
lines present in the composite spectrum. We compare the entire spectrum with
the quasar spectrum in the context of the AGN unification model. The two
composite spectra match extremely well in the blue part of the spectrum, while
there is an offset in flux in the red portion of the spectrum.
