ANGULAR SIZE TEST ON THE EXPANSION OF THE UNIVERSE

@article{LpezCorredoira2010ANGULARST,
  title={ANGULAR SIZE TEST ON THE EXPANSION OF THE UNIVERSE},
  author={M. L{\'o}pez-Corredoira},
  journal={International Journal of Modern Physics D},
  year={2010},
  volume={19},
  pages={245-291}
}
Assuming the standard cosmological model to be correct, the average linear size of the galaxies with the same luminosity is six times smaller at z = 3.2 than at z = 0; and their average angular size for a given luminosity is approximately proportional to z-1. Neither the hypothesis that galaxies which formed earlier have much higher densities nor their luminosity evolution, merger ratio, and massive outflows due to a quasar feedback mechanism are enough to justify such a strong size evolution… 

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