We study fluctuations about axisymmetric warped brane solutions in 6D minimal
gauged supergravity. Much of our analysis is general and could be applied to
other scenarios. We focus on bulk sectors that could give rise to Standard
Model gauge fields and charged matter. We reduce the dynamics to Schroedinger
type equations plus physical boundary conditions, and obtain exact solutions
for the Kaluza-Klein wave functions and discrete mass spectra. The power-law
warping, as opposed to exponential in 5D, means that zero mode wave functions
can be peaked on negative tension branes, but only at the price of localizing
the whole Kaluza-Klein tower there. However, remarkably, the codimension two
defects allow the Kaluza-Klein mass gap to remain finite even in the infinite
volume limit. In principle, not only gravity, but Standard Model fields could
`feel' the extent of large extra dimensions, and still be described by an
effective 4D theory.Comment: 33 pages, 2 figures; typesetting problem fixed ({\o}replaced by
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