Evolution in the bias of faint radio sources to z ∼ 2 . 2

@inproceedings{Lindsay2014EvolutionIT,
  title={Evolution in the bias of faint radio sources to z ∼ 2 . 2},
  author={Sam N. Lindsay and Matt J. Jarvis and K. W. McAlpine},
  year={2014}
}
Quantifying how the baryonic matter traces the underlying d ark matter distribution is key to both understanding galaxy formation and our ability to cons train the cosmological model. Using the cross-correlation function of radio and near-inf ared galaxies, we present a largescale clustering analysis of radio galaxies to z ∼ 2.2. We measure the angular auto-correlation function ofKs < 23.5 galaxies in the VIDEO-XMM3 field with photometric redshifts out to z = 4 using VIDEO and CFHTLS photometry… CONTINUE READING