  We present an updated model for the extragalactic background light (EBL) from
stars and dust, over wavelengths approximately 0.1 to 1000 $\mu$m. This model
uses accurate theoretical stellar spectra, and tracks the evolution of star
formation, stellar mass density, metallicity, and interstellar dust extinction
and emission in the universe with redshift. Dust emission components are
treated self-consistently, with stellar light absorbed by dust reradiated in
the infrared as three blackbody components. We fit our model, with free
parameters associated with star formation rate and dust extinction and
emission, to a wide variety of data: luminosity density, stellar mass density,
and dust extinction data from galaxy surveys; and $\gamma$-ray absorption
optical depth data from $\gamma$-ray telescopes. Our results strongly
constraint the star formation rate density and dust photon escape fraction of
the universe out to redshift $z=10$, about 90% of the history of the universe.
We find our model result is, in some cases, below lower limits on the $z=0$ EBL
intensity, and below some low-$z$ $\gamma$-ray absorption measurements.
