Cosmological parameter estimation using Very Small Array data out to ℓ = 1500

@article{Rebolo2004CosmologicalPE,
  title={Cosmological parameter estimation using Very Small Array data out to ℓ = 1500},
  author={Rafael Rebolo and Richard A. Battye and Pedro Carreira and Kieran A. Cleary and Rodney D. Davies and Richard J. Davis and Clive Dickinson and Ricardo G{\'e}nova-Santos and K. J. B. Grainge and Carlos M. Gutirrez and Yaser A. Hafez and Michael P. Hobson and Michael E. Jones and R{\"u}diger Kneissl and Katy Lancaster and Anthony N. Lasenby and J. Patrick Leahy and Klaus Maisinger and Guy G. Pooley and Nutan Rajguru and Jos{\'e} Alberto Rubi{\~n}o-Mart{\'i}n and Richard D. E. Saunders and Richard S. Savage and A. M. M. Scaife and Paul F. Scott and An{\vz}e Slosar and Pedro J. Sosa Molina and Angela C. Taylor and David J. Titterington and Elizabeth M. Waldram and Robert A. Watson and Althea Wilkinson},
  journal={Monthly Notices of the Royal Astronomical Society},
  year={2004},
  volume={353},
  pages={747-759}
}
We estimate cosmological parameters using data obtained by the Very Small Array (VSA) in its extended configuration, in conjunction with a variety of other cosmic microwave background (CMB) data and external priors. Within the flat A cold dark matter (ACDM) model, we find that the inclusion of high-resolution data from the VSA modifies the limits on the cosmological parameters as compared to those suggested by the Wilkinson Microwave Anisotropy Probe (WMAP) alone, while still remaining… Expand
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