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Measuring Large-Scale Structure at z ∼ 1 with the VIPERS galaxy survey

Published online by Cambridge University Press:  12 October 2016

Luigi Guzzo
Luigi Guzzo*
Affiliation:
INAF - Osservatorio Astronomico di Brera, 20122 Milano, Italy email: luigi.guzzo@brera.inaf.it
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Abstract

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The VIMOS Public Extragalactic Redshift Survey (VIPERS) is the largest redshift survey ever conducted with the ESO telescopes. It has used the Very Large Telescope to collect nearly 100,000 redshifts from the general galaxy population at 0.5 < z < 1.2. With a combination of volume and high sampling density that is unique for these redshifts, it allows statistical measurements of galaxy clustering and related cosmological quantities to be obtained on an equal footing with classic results from local redshift surveys. At the same time, the simple magnitude-limited selection and the wealth of ancillary photometric data provide a general view of the galaxy population, its physical properties and the relation of the latter to large-scale structure. This paper presents an overview of the galaxy clustering results obtained so far, together with their cosmological implications. Most of these are based on the ∼ 55,000 galaxies forming the first public data release (PDR-1). As of January 2015, observations and data reduction are complete and the final data set of more than 90,000 redshifts is being validated and made ready for the final investigations.

Keywords

catalogssurveysgalaxiesdistances and redshiftstechniques: spectroscopicmethods: data analysis(cosmology:) large scale structure of universecosmology: observations
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 11 , Symposium S308: The Zeldovich Universe: Genesis and Growth of the Cosmic Web , June 2014 , pp. 149 - 160
Copyright
Copyright © International Astronomical Union 2016 

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