The 1-point PDF of the Initial Conditions of our Local Universe from the IRAS PSC redshift catalogue
arXiv:astro-ph/0006066 · doi:10.1046/j.1365-8711.2000.03739.x
Abstract
The algorithm ZTRACE of Monaco & Efstathiou (1999) is applied to the IRAS PSCz catalogue to reconstruct the initial conditions of our local Universe with a resolution down to ~5 Mpc/h. The 1-point PDF of the reconstructed initial conditions is consistent with the assumptions that (i) IRAS galaxies trace mass on scales of ~5 Mpc/h, and (ii) the statistics of primordial density fluctuations is Gaussian. We use simulated PSCz catalogues, constructed from N-body simulations with Gaussian initial conditions, to show that local non-linear bias can cause the recovered initial PDF (assuming no bias) to be non-Gaussian. However, for plausible bias models, the distortions of the recovered PDF would be difficult to detect using the volume finely sampled by the PSCz catalogue. So, for Gaussian initial conditions, a range of bias models remain compatible with our PSCz reconstruction results.
arXiv comment13 pages, figures included (needs mn.sty), in press on MNRAS
References in corpus (34)
- The PSCz Catalogue
- The Nature of Galaxy Bias and Clustering
- Large-scale structure, the cosmic microwave background, and primordial non-gaussianity
- The IRAS 1.2 Jy Survey: Redshift Data
- Hydra: An Adaptive--Mesh Implementation of PPPM--SPH
- The time-evolution of bias
- The bias field of dark matter haloes
- The Microwave Background Bispectrum, Paper I: Basic Formalism
- A simulation of galaxy formation and clustering
- A Non Parametric Model for the Cosmic Velocity Field
- Spherical Harmonic Analysis of the PSCz Galaxy Catalogue: Redshift distortions and the real-space power spectrum
- The Optical Redshift Survey: Sample Selection and the Galaxy Distribution
- On the Non-Gaussianity Observed in the COBE-DMR Sky Maps
- The Nearby Optical Galaxy Sample: The Local Galaxy Luminosity Function
- The IRAS PSCz Dipole
- The Topology of the IRAS Point Source Catalogue Redshift Survey
- Is the cosmic microwave background really non-Gaussian?
- On the least action principle in cosmology
- Reconstruction of cosmological density and velocity fields in the Lagrangian Zel'dovich Approximation
- Simulating Our Cosmological Neighborhood: Mock Catalogs for Velocity Analysis
- Reconstruction of cosmological initial conditions from galaxy redshift catalogues
- On density and velocity fields and beta from the IRAS PSCz survey
- Measuring the Nonlinear Biasing Function from a Galaxy Redshift Survey
- Likelihood Analysis of the Local Group Acceleration
- The Power Spectrum of the PSC Redshift Survey
- The Velocity Field Predicted by the Optical Redshift Survey
- A Bayesian estimate of the skewness of the Cosmic Microwave Background
- A Comparison of The PSCz and Stromlo-APM Redshift Surveys
- Recovering the Primordial Density Fluctuations: A comparison of methods
- Reconstruction Analysis of Galaxy Redshift Surveys: A Hybrid Reconstruction Method
- Genus Statistics of the Virgo N-body simulations and the 1.2-Jy Redshift Survey
- Topological Defects and Cosmology
- Reconstruction Analysis I.: Redshift--space deprojection in the quasi--nonlinear regime
- Galaxy and Cluster Biasing from Local Group Dynamics