Abstract
Future deep galaxy surveys will cover a range in redshift over which the galaxy-bias and density field evolve significantly. In this brief conference proceedings contribution, we describe how models for these effects can be factored into a clustering analysis and can then be constrained by the data. Even for recent low-redshift surveys such as the 2dF galaxy redshift survey (2dFGRS), luminosity-dependent galaxy-bias can change the recovered clustering signal from that of the underlying density field [5].
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Percival, W.J., Verde, L., Peacock, J.A. Analysing Galaxy Clustering in Future Surveys. In: Renzini, A., Bender, R. (eds) Multiwavelength Mapping of Galaxy Formation and Evolution. ESO Astrophysics Symposia. Springer, Berlin, Heidelberg. https://doi.org/10.1007/10995020_99
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DOI: https://doi.org/10.1007/10995020_99
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Publisher Name: Springer, Berlin, Heidelberg
Print ISBN: 978-3-540-25665-6
Online ISBN: 978-3-540-31641-1
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