Evolution of the Non-Linear Galaxy Bias up to Redshift z=1.5

Details Evolution of the Non-Linear Galaxy Bias up to Redshift z=1.5 Evolution of the Non-Linear Galaxy Bias up to Redshift z=1.5

2006-12-05

arxiv.org/abs/astro-ph/0612123v2

Astronomy and Astrophysics

Astrophysics

8 pages, 3 figures. To appear in the proceedings of the XLIst Rencontres de Moriond, XXVIth Astrophysics Moriond Meeting: "Fro

Scientific paper

Deep redshift surveys of the universe provide the basic ingredients to compute the probability distribution function (PDF) of galaxy fluctuations and to constrain its evolution with cosmic time. When this statistic is combined with analytical CDM predictions for the PDF of mass, useful insights into the biasing function relating mass and galaxy distributions can be obtained. In this paper, we focus on two issues: the shape of the biasing function and its evolution with redshift. We constrain these quantities by using a preliminary sample of galaxies spectroscopically surveyed by the Vimos-VLT Deep Survey in a deep cone 0.4 0.8.

Affiliated with

Also associated with

No associations

Rating

Evolution of the Non-Linear Galaxy Bias up to Redshift z=1.5 does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Evolution of the Non-Linear Galaxy Bias up to Redshift z=1.5, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Evolution of the Non-Linear Galaxy Bias up to Redshift z=1.5 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-717369