Angular Diameter Distances in Clumpy Friedmann Universes
Clustering tomography: measuring cosmological distances through angular clustering in thin redshift shells
Angular-diameter distance estimates from the Sunyaev–Zeldovich effect in hydrodynamical cluster simulations
A distance estimate based on angular expansion for the planetary nebula NGC 6881
The angular-diameter distance maximum and its redshift as constraints on Λ≠ 0 Friedmann–Lemaître–Robertson–Walker models
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1 The sum of all the angular changes that occur during the rotation of a body.
2 The distance between two bodies measured in terms of the angle subtended by them at the point of observation.
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