  Line intensity mapping is rapidly gaining prominence as a tool to understand
galaxy evolution and cosmology at high redshift. However, the standard power
spectrum analysis for these surveys suffers from a tight degeneracy between the
overall mean line intensity and the bias of the emitting galaxies. We outline a
new formalism for the Voxel Intensity Distribution (VID), a one-point statistic
which is known to contain information beyond the power spectrum. We use this
new calculation to show for the first time that the VID can be used to break
this key degeneracy in intensity mapping data.
