THE BARYONIC ACOUSTIC FEATURE AND LARGE-SCALE CLUSTERING IN THE SLOAN DIGITAL SKY SURVEY LUMINOUS RED GALAXY SAMPLE

By E. Kazin, M. Blanton, R. Scoccimarro, Cameron McBride, A. Berlind, N. Bahcall, J. Brinkmann, P. Czarapata, Joshua A. Frieman, S. Kent and 2 more. 2010

197 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Statistical and Nonlinear Physics

View Paper: https://www.semanticscholar.org/paper/90a991901a3df00afb446cddd0e68e3d1c8beca6

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Citations in the corpus

The WiggleZ Dark Energy Survey: mapping the distance-redshift relation with baryon acoustic oscillations (2011, methodology): “The sky coverage and redshift distributions of the LRG samples are presented in Figures 1 and 2 of Kazin et al. (2010a).”
GALAXY CLUSTERING IN THE COMPLETED SDSS REDSHIFT SURVEY: THE DEPENDENCE ON COLOR AND LUMINOSITY (2010, methodology): “…correlation function measurements and HODmodels of the SDSS Luminous Red Galaxy (LRG) sample (Eisenstein et al. 2001, 2005b; Zehavi et al. 2005a; Zheng et al. 2009; Kazin et al. 2010; Watson et al. 2010), which probes the most luminous galaxies out to redshift z ≈ 0.45 (Eisenstein et al. 2001).”
NINE-YEAR WILKINSON MICROWAVE ANISOTROPY PROBE (WMAP) OBSERVATIONS: COSMOLOGICAL PARAMETER RESULTS (2012, methodology): “(These data were used in the WMAP seven-year analysis, see also Kazin et al. 2010).”
Measuring DA and H at z = 0.35 from the SDSS DR7 LRGs using baryon acoustic oscillations (2012, background): “…on the spherically averaged (monopole) statistics (Cole et al. 2005; Eisenstein et al. 2005; Hütsi 2006; Tegmark et al. 2006; Percival et al. 2007; Kazin et al. 2010a; Percival et al. 2010; Beutler et al. 2011; Blake et al. 2011a; Mehta et al. 2012; Padmanabhan et al. 2012; Xu et al. 2012),…”
The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: measuring DA and H at z = 0.57 from the baryon acoustic peak in the data release 9 spectroscopic galaxy sample (2013, background): “…redshift surveys, including the Sloan Digital Sky Survey (SDSS Eisenstein et al. 2005; Hütsi 2006; Tegmark et al. 2006; Percival et al. 2007, 2010; Kazin et al. 2010; Chuang et al. 2012; Chuang & Wang 2012; Padmanabhan et al. 2012; Xu et al. 2012), 2dF Galaxy Redshift Survey (Cole et al. 2005),…”
The DESI Experiment Part I: Science,Targeting, and Survey Design (2016, background): “They exhibit strong clustering and a relatively high large-scale-structure bias, which enhances the amplitude of their power spectrum, and hence the BAO signal ([193], [194], [195]).”
The WiggleZ Dark Energy Survey: testing the cosmological model with baryon acoustic oscillations at z= 0.6 (2011, methodology): “Other studies of the SDSS LRG sample, producing broadly similar conclusions, have been performed by Huetsi (2006), Percival et al. (2007), Sanchez et al. (2009) and Kazin et al. (2010a).”
The clustering of galaxies in the sdss-iii baryon oscillation spectroscopic survey: Baryon acoustic oscillations in the data release 9 spectroscopic galaxy sample (2012, methodology): “…2005; Hütsi 2006; Blake et al. 2007, 2011a; Padmanabhan et al. 2007, 2012a; Okumura et al. 2008; Gaztanaga, Cabre & Hui 2009; Sanchez et al. 2009; Kazin et al. 2010; Reid et al. 2010; Beutler et al. 2011; Cabré & Gaztañaga 2011; Seo et al. 2012), and it is already producing stringent…”
The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: measurements of the growth of structure and expansion rate at z = 0.57 from anisotropic clustering (2012, background): “…et al. 2005; Hütsi 2006; Blake et al. 2007; Padmanabhan et al. 2007; Percival et al. 2007, 2010; Okumura et al. 2008; Gaztanaga, Cabre & Hui 2009; Kazin et al. 2010; Reid et al. 2010b; Beutler et al. 2011; Blake et al. 2011a) have revealed that the expansion of the Universe is accelerating;…”
The clustering of galaxies in the SDSS‐III Baryon Oscillation Spectroscopic Survey: cosmological implications of the large‐scale two‐point correlation function (2012, background): “…al. (2005) and has been subsequently observed using a variety of datasets and techniques (Hütsi 2006; Padmanabhan et al. 2007; Percival et al. 2007, 2010; Cabré & Gaztañaga 2009; Gaztañaga et al. 2009; Kazin et al. 2010; Beutler et al. 2011; Blake et al. 2011; Ho et al. 2012; Seo et al. 2012).”
A 2 per cent distance to $z$=0.35 by reconstructing baryon acoustic oscillations - I. Methods and application to the Sloan Digital Sky Survey (2012, methodology): “These results are also consistent with those of Kazin et al. (2010) who obtain 7.17 ± 0.25.”
The 6dF Galaxy Survey: baryon acoustic oscillations and the local Hubble constant (2011, methodology): “Another motivation for our study is that the SDSS data after data release 3 (DR3) show more correlation on large scales than expected by ΛCDM and have no sign of a crossover to negative ξ up to 200h−1 Mpc (the ΛCDM prediction is 140h−1 Mpc) (Kazin et al. 2010).”
THE BARYON OSCILLATION SPECTROSCOPIC SURVEY OF SDSS-III (2012, methodology): “Kazin et al. (2010) used the full LRG sample from DR7 to measure the galaxy correlation function and obtain a 3.5% measurement of the BAO distance scale at z = 0.35.”
SEVEN-YEAR WILKINSON MICROWAVE ANISOTROPY PROBE (WMAP) OBSERVATIONS: COSMOLOGICAL INTERPRETATION (2010, methodology): “Kazin et al. (2010) used the two-point correlation function of SDSS-DR7 LRGs to measure rs/DV (z) at z = 0.278.”
The Intrinsic Alignment of Galaxies and its Impact on Weak Gravitational Lensing in an Era of Precision Cosmology (2014, methodology): “Applying this methodology to a lens sample of SDSS LRGs from DR7 selected by Kazin et al. (2010) and a source sample with shape measurements from the SDSS DR8 photometric data selected by Reyes et al. (2011), they find an intrinsic alignment signal consistent with zero.”
The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: single-probe measurements from CMASS anisotropic galaxy clustering (2013, methodology): “…function method (see, e.g. Eisenstein et al. 2005; Okumura et al. 2008; Cabre & Gaztanaga 2009; Martinez et al. 2009; Sanchez et al. 2009; Kazin et al. 2010; Samushia, Percival & Raccanelli 2011; Chuang, Wang & Hemantha 2012; Padmanabhan et al. 2012; Xu et al. 2013; Hemantha, Wang &…”
The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: single-probe measurements and the strong power of f(z)σ8(z) on constraining dark energy (2013, methodology): “…Montesano et al. 2011), and the correlation function method (see, e.g., Eisenstein et al. 2005; Okumura et al. 2008; Cabre & Gaztanaga 2009; Martinez et al. 2009; Sanchez et al. 2009; Kazin et al. 2010a; Chuang, Wang, & Hemantha 2012; Samushia et al. 2011; Padmanabhan et al. 2012; Xu et al. 2012).”
Measurements of H(z) and DA(z) from the two-dimensional two-point correlation function of Sloan Digital Sky Survey luminous red galaxies (2011, methodology): “The same selection criteria were used in previous papers (Zehavi et al. 2005; Eisenstein et al. 2005; Okumura et al. 2008; Kazin et al. 2010a).”