0000000001115871

AUTHOR

Marc Lachièze-rey

showing 2 related works from this author

Wavelet analysis of baryon acoustic structures in the galaxy distribution

2011

Baryon Acoustic Oscillations (BAO) are a feature imprinted in the density field by acoustic waves travelling in the plasma of the early universe. Their fixed scale can be used as a standard ruler to study the geometry of the universe. BAO have been previously detected using correlation functions and power spectra of the galaxy distribution. In this work, we present a new method for the detection of the real-space structures associated with this feature. These baryon acoustic structures are spherical shells with a relatively small density contrast, surrounding high density central regions. We design a specific wavelet adapted to the search for shells, and exploit the physics of the process b…

Cosmology and Nongalactic Astrophysics (astro-ph.CO)Cold dark mattermedia_common.quotation_subjectFOS: Physical sciencesContext (language use)AstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciences0103 physical sciencesDensity contrast010303 astronomy & astrophysicsmedia_commonPhysicsmethods: statistical[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph]010308 nuclear & particles physicsgalaxies: cluster: generalAstronomy and AstrophysicsAcoustic wavecosmology: distance scalecosmology: large-scale structure of Universemethods: data analysisUniverseGalaxyBaryonSpace and Planetary ScienceBaryon acoustic oscillationsAstrophysics - Cosmology and Nongalactic Astrophysics
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Uncertainty in 2-point correlation function estimators and baryon acoustic oscillation detection in galaxy surveys

2012

Abstract We study the uncertainty in different two-point correlation function (2PCF) estimators in currently available galaxy surveys. This is motivated by the active subject of using the baryon acoustic oscillations (BAOs) feature in the correlation function as a tool to constrain cosmological parameters, which requires a fine analysis of the statistical significance. We discuss how estimators are affected by both the uncertainty in the mean density n and the integral constraint 1 V 2 ∫ V 2 ξ ˆ ( r ) d 3 r = 0 which necessarily causes a bias. We quantify both effects for currently available galaxy samples using simulated mock catalogues of the Sloan Digital Sky Survey (SDSS) following a lo…

Statistics and ProbabilityNumber density010308 nuclear & particles physicsmedia_common.quotation_subjectDark matterEstimatorAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesRedshiftGalaxyBaryonSky0103 physical sciencesBaryon acoustic oscillationsStatistical physics010303 astronomy & astrophysicsmedia_commonMathematicsStatistical Methodology
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