1986
DOI: 10.1086/184673
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N-point correlations for biased galaxy formation

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Cited by 61 publications
(64 citation statements)
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“…This result was interpreted as a support for gravitational instability from Gaussian initial conditions and in disagreement with models of threshold bias [21,344], which predicted Q 3 ∼ 1. The results in Fig.…”
Section: Three-point Statisticsmentioning
confidence: 55%
“…This result was interpreted as a support for gravitational instability from Gaussian initial conditions and in disagreement with models of threshold bias [21,344], which predicted Q 3 ∼ 1. The results in Fig.…”
Section: Three-point Statisticsmentioning
confidence: 55%
“…For Gaussian initial conditions, one obtains (Kaiser 1984;Politzer & Wise 1984;Jensen & Szalay 1986) 2 2 n n y (r) p exp…”
Section: Halos As Peaks Of the Density Fieldmentioning
confidence: 99%
“…In the case of the first stars, such populations are likely to be biased, i.e., the luminous sources form at the high peaks of the underlying density field. The relation between the underlying P ΛCDM and P 3 (k) is likely to be nonlinear even on linear scales depending on the height of the peaks (Jensen & Szalay 1986;Kashlinsky 1998), but as a toy model we approximate here that P 3 (k) ∝ P ΛCDM . We further assume that dF/dt does not vary significantly over the corresponding epochs, which can happen if the emitters span a narrow range of cosmic times.…”
Section: Source-subtracted Cib Fluctuations From Spitzermentioning
confidence: 99%