The three-point function in large-scale structure: redshift distortions and galaxy bias
Open Access
- 11 August 2005
- journal article
- Published by Oxford University Press (OUP) in Monthly Notices of the Royal Astronomical Society
- Vol. 361 (3) , 824-836
- https://doi.org/10.1111/j.1365-2966.2005.09234.x
Abstract
No abstract availableKeywords
All Related Versions
This publication has 52 references indexed in Scilit:
- The 2dF Galaxy Redshift Survey: hierarchical galaxy clusteringMonthly Notices of the Royal Astronomical Society, 2004
- The Halo Occupation Distribution and the Physics of Galaxy FormationThe Astrophysical Journal, 2003
- Halo models of large scale structurePhysics Reports, 2002
- Large-scale structure of the Universe and cosmological perturbation theoryPhysics Reports, 2002
- The three-point function in large-scale structure – I. The weakly non-linear regime in N-body simulationsMonthly Notices of the Royal Astronomical Society, 2002
- The 2dF Galaxy Redshift Survey: spectra and redshiftsMonthly Notices of the Royal Astronomical Society, 2001
- Effects of sampling on statistics of large-scale structureMonthly Notices of the Royal Astronomical Society, 1998
- Testing Ansatze for quasi-non-linear clustering: the linear APM power spectrumMonthly Notices of the Royal Astronomical Society, 1996
- Moments of the Counts Distribution in the 1.2 Jansky IRAS Galaxy Redshift SurveyThe Astrophysical Journal, 1993
- Fourier spectra of three-dimensional dataThe Astrophysical Journal, 1991