Summary
We have combined three different samples, totalling 371 quasars, to study the evolution of their clustering properties with cosmic time. Clustering is detected at low redshifts (z<1.5) on scales less than 10 h-1 Mpc at the 4.7σ level, but not at high redshifts (z>1.5). The difference between these two results is significant at the 2.2σ level.
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References
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© 1988 Kluwer Academic Publishers
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Iovino, A., Shaver, P. (1988). Evolution of Quasar Clustering. In: Kaiser, N., Lasenby, A.N. (eds) The Post-Recombination Universe. NATO ASI Series, vol 240. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-3035-3_32
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DOI: https://doi.org/10.1007/978-94-009-3035-3_32
Publisher Name: Springer, Dordrecht
Print ISBN: 978-94-010-7864-1
Online ISBN: 978-94-009-3035-3
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