  We predict the arrival direction distribution of cosmic rays including their
deflection in the Galactic magnetic field, for several combinations of source
and composition hypotheses: the sources are hard X-ray AGNs or uniformly sample
the matter distribution of galaxies, and the composition at the source is pure
proton or is the Galactic cosmic ray composition measured by CREAM. We use the
regular component of the Jansson-Farrar 2012 model for the GMF and allow for
rigidities as low as 2 EeV. We report the correlations of published UHECRs,
rescaling event energies so as to reconcile the spectra of the different
experiments and taking the overall energy uncertainty into account; different
composition hypotheses are considered. This work demonstrates the feasibility
of calculating GMF deflections to low enough rigidities to allow for heavy
composition in correlation studies, and that non-trivial arrival direction
structure should be expected even for mixed or heavy composition, as long as
UHECRs come from the local universe.
