# The evolution of galaxy clustering since z=1

@article{Phleps2001TheEO,
title={The evolution of galaxy clustering since z=1},
author={Stefanie Phleps and Klaus Meisenheimer},
journal={arXiv: Astrophysics},
year={2001}
}
• Published 13 September 2001
• Physics
• arXiv: Astrophysics
We present results of an investigation of clustering evolution of field galaxies between a redshift of z~1 and the present epoch. The current analysis relies on a sample of ~3600 galaxies from the Calar Alto Deep Imaging Survey (CADIS). The multicolor classification and redshift determination is reliable up to I=23. The redshift distribution extends to z~1.1, the resolution is Delta cz=12000 km s^-1. Thus the amplitude of the three-dimensional correlation function has to be estimated by means…

## Figures and Tables from this paper

The VIMOS-VLT Deep Survey - The evolution of galaxy clustering per spectral type to z~1.5
We measure the evolution of clustering for galaxies with different spectral types from 6495 galaxies with 17.5 1.2, due to the growth in clustering of the star-forming population. We find similar
Galaxy clustering from COMBO-17: the halo occupation distribution at = 0.6
• Physics
• 2005
We present measurements of galaxy clustering at redshift $\langle z \rangle=0.6$ using $10\,360$ galaxies with photometric redshifts over an area of 0.78 deg 2 from the COMBO-17 survey. To obtain a
Tracing the filamentary structure of the galaxy distribution at z∼0.8
• Physics
• 2010
We study filamentary structure in the galaxy distribution at z ∼ 0.8 using data from the Deep Extragalactic Evolutionary Probe 2 (DEEP2) Redshift Survey and its evolution to z ∼ 0.1 using data from
COMBO-17 measurements of the effect of environment on the type-dependent galaxy luminosity function
• Physics
• 2007
We have developed a method to calculate overdensities in multicolour surveys, facilitating a direct comparison of the local density contrast measured using galaxy samples that have different redshift
Spatial clustering in the ESO-Sculptor survey: two-point correlation functions by galaxy type at redshifts 0.1-0.5
• Physics
• 2007
Context: Galaxy clustering shows segregation effects with galaxy type, color and luminosity, which bring clues on the relationship with the underlying density field. Aims: We explore these effects
Evolution of the dark matter distribution with three-dimensional weak lensing
We present a direct detection of the growth of large-scale structure, using weak gravitational lensing and photometric redshift data from the {COMBO-17} survey. We use deep R-band imaging of two 0.5
Relative clustering and the joint halo occupation distribution of red sequence and blue-cloud galaxies in COMBO-17
This paper studies the relative spatial distribution of red-sequence and blue-cloud galaxies, and their relation to the dark matter distribution in the COMBO-17 survey as function of scale down to z
GEMS: Galaxy Evolution from Morphologies and SEDs
GEMS (Galaxy Evolution from Morphologies and SEDs) is a large-area (800 arcmin2) two-color (F606W and F850LP) imaging survey with the Advanced Camera for Surveys on the Hubble Space Telescope.
Scaling laws in the distribution of galaxies
• Physics
• 2005
Past surveys have revealed that the large-scale distribution of galaxies in the universe is far from random: it is highly structured over a vast range of scales. Surveys being currently undertaken
The Importance of Spheroidal and Mixed Mergers for Early-Type Galaxy Formation
We use semianalytical modeling techniques to investigate the progenitor morphologies of present-day elliptical galaxies. We find that, independent of the environment, the fraction of mergers of

## References

SHOWING 1-10 OF 55 REFERENCES
The Canada France Redshift Survey VIII: Evolution of the clustering of galaxies from z~1
• Physics
• 1995
We have used the projected two-point correlation function, $w(r_p)$, to investigate the spatial distribution of the 591 galaxies with secure redshifts between $0 \leq z \leq 1.3$ in the five CFRS
Southern Sky Redshift Survey: Clustering of Local Galaxies
• Physics
• 1998
We use the two-point correlation function to calculate the clustering properties of the recently completed SSRS2 survey, which probes two well-separated regions of the sky, allowing one to evaluate
The Clustering of Faint Galaxies and the Evolution of XI (r)
• Physics
• 1996
The two-point angular correlation function, $\w$, is constructed from a catalog of 13,000 objects in 24 fields distributed over an area of 4 deg$^2$ and complete to a limit of $R = 23.5$. The
Galaxy Clustering Evolution in the CNOC2 High-Luminosity Sample
The redshift evolution of the galaxy two-point correlation function is a fundamental cosmological statistic. To identify similar galaxy populations at different redshifts, we select a strict
Galaxy Clustering in Early SDSS Redshift Data
We present the first measurements of clustering in the Sloan Digital Sky Survey (SDSS) galaxy redshift survey. Our sample consists of 29,300 galaxies with redshifts 5,700 km/s < cz < 39,000 km/s,
Clustering of galaxies in a hierarchical universe - I. Methods and results at z=0
• Physics
• 1999
We introduce a new technique for following the formation and evolution of galaxies in cosmological N-body simulations. Dissipationless simulations are used to track the formation and merging of dark
The Canada-France Redshift Survey. I. Introduction to the Survey, Photometric Catalogs, and Surface Brightness Selection Effects
• Physics
• 1995
The Canada-France Redshift Survey has been undertaken to provide a large well-defined sample of faint galaxies at high redshift in which the selection criteria match as closely as possible those of
A survey of galaxy redshifts. V. The two-point position and velocity correlations.
• Physics
• 1983
We describe the results of a study of the two-point correlations in the 14.5 m/sub B/ CfA redshift survey. We use the distance information provided by the redshifts to estimate the two-point spatial
Galaxy clustering in early sloan digital sky survey redshift data
We present the first measurements of clustering in the Sloan Digital Sky Survey (SDSS) galaxy redshift survey. Our sample consists of 29,300 galaxies with redshifts 5700 km s-1 ≤ cz ≤ 39,000 km s-1,
The two-point correlation function and morphological segregation in the Optical Redshift Survey
We study the clustering of galaxies in real and redshift space using the Optical Redshift Survey (ORS). We estimate the two-point correlation function in redshift space, xi(s), for several subsamples