  We consider Einstein gravity with positive cosmological constant coupled with
higher spin interactions and calculate Euclidean path integral perturbatively.
We confine ourselves to the static patch of the 3 dimensional de Sitter space.
This geometry, when Euclideanlized is equivalent to 3-sphere. However, infinite
number of topological quotients of this space by discrete subgroups of the
isometry group are valid Euclidean saddles as well. Pure Einstein gravity is
known to diverge, when all saddles are included as contribution to the thermal
partition functions (also interpreted as the Hartle Hawking state in the
cosmological scenario). We show how higher spins, described by metric-Fronsdal
fields help making the partition function finite. Counter-intuitively, this
convergence is not achieved by mere inclusion of spin-3, but requires spin-4
interactions.
