Up until very recently, the Epoch of Reionization has been largely 
observationally unexplored .  However, with advancements of modern 
telescopes, we are now able to observe this period of the Universe in 
multiple ways. While observations are still very challenging due to a 
host of foreground contaminants, combining observations at multiple 
wavelengths can lead to a greater understanding of the populations of 
stars and galaxies at these redshifts.  I will describe two of these 
observables: the Cosmic Infrared Background, which is partially the 
integrated light from all stars and galaxies at high redshifts, and 
the 21cm Background, which results from emission from neutral gas. 
These observables, when paired with theory and simulations, can tell 
us about some of the first stars and galaxies that formed within our Universe.