• DOI:10.1111/j.1365-2966.2005.09318.x
Corpus ID: 6906627

The 2dF Galaxy Redshift Survey: power-spectrum analysis of the final data set and cosmological implications

@article{Cole2005The2G,
  title={The 2dF Galaxy Redshift Survey: power-spectrum analysis of the final data set and cosmological implications},
  author={S. Cole and W. J. Percival and J. Peacock and P. Norberg and C. Baugh and C. Frenk and I. Baldry and J. Bland-hawthorn and T. Bridges and R. Cannon and M. Colless and C. Collins and W. Couch and N. Cross and G. Dalton and V. Eke and R. D. Propris and S. Driver and G. Efstathiou and R. Ellis and K. Glazebrook and C. Jackson and A. Jenkins and O. Lahav and I. Lewis and S. Lumsden and S. Maddox and D. Madgwick and B. Peterson and W. Sutherland and K. Taylor},
  journal={Monthly Notices of the Royal Astronomical Society},
  year={2005},
  volume={362},
  pages={505-534}
}

S. Cole, W. J. Percival, +28 authors K. Taylor

Published 2005

Physics

Monthly Notices of the Royal Astronomical Society

We present a power-spectrum analysis of the final 2dF Galaxy Redshift Survey (2dFGRS), employing a direct Fourier method. The sample used comprises 221 414 galaxies with measured redshifts. We investigate in detail the modelling of the sample selection, improving on previous treatments in a number of respects. A new angular mask is derived, based on revisions to the photometric calibration. The redshift selection function is determined by dividing the survey according to rest-frame colour, and… CONTINUE READING

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