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Imposing extendibility on Kasner-Fronsdal black hole local isometric embedding is equivalent to removing conic singularities in Kruskal representation. Allowing for globally non-trivial (living in $M_{5}\times S_{1}k$, extendibility can be achieved for apparently forbidden frequencies . The Hawking-Gibbons limit, say for Schwarzschild geometry, is respected. The corresponding Kruskal sheets are viewed as slices in some Kaluza-Klein background. Euclidean discreteness, dictated by imaginary time periodicity, is correlated with twistor flux quantization.

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