  In this work we construct metrics corresponding to radiating black holes
whose near horizon regions cannot be approximated by Rindler spacetime. We
first construct infinite parameter coordinate transformations from Minkowski
coordinates, such that an observer using these coordinates to describe
spacetime events measures the Minkowski vacuum to be Planckian. Utilizing these
results, we construct family of black holes that radiate at spatial infinity.
As an illustration we study a subset of the black hole solutions that satisfy
the null energy condition.
