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A TOPOLOGICAL ANALYSIS OF LARGE-SCALE STRUCTURE, STUDIED USING THE CMASS SAMPLE OF SDSS-III
Journal article   Open access

A TOPOLOGICAL ANALYSIS OF LARGE-SCALE STRUCTURE, STUDIED USING THE CMASS SAMPLE OF SDSS-III

Prachi Parihar, Michael Vogeley, J Gott, Yun-Young Choi, Juhan Kim, Sungsoo Kim, Robert Speare, Joel Brownstein and J Brinkmann
The Astrophysical journal, v 796(2), pp 1-14
01 Feb 2014
url
https://doi.org/10.1088/0004-637x/796/2/86View
Published, Version of Record (VoR)Maybe Open Access (Publisher Bronze) Open
url
https://doi.org/10.1088/0004-637X/796/2/86View
Published, Version of Record (VoR) Open

Abstract

Dark matter Dynamical systems Galaxy formation Gaussian Initial conditions Sky surveys (astronomy) Stellar mass Three dimensional Topology
We study the three-dimensional genus topology of large-scale structure using the northern region of the CMASS Data Release 10 (DR10) sample of the SDSS-III Baryon Oscillation Spectroscopic Survey. We select galaxies with redshift 0.452 < z < 0.625 and with a stellar mass M super(stellar) > 10 super(11.56) M sub([middot in circle]). We study the topology at two smoothing lengths: R sub(G) = 21 h super(-1) Mpc and R = 34 h super(-1) Mpc. The genus topology studied at the R sub(G) = 21 h super(-1) Mpc scale results in the highest genus amplitude observed to date. The CMASS sample yields a genus curve that is characteristic of one produced by Gaussian random phase initial conditions. The data thus support the standard model of inflation where random quantum fluctuations in the early universe produced Gaussian random phase initial conditions. We construct 54 mock SDSS CMASS surveys along the past light cone from the Horizon Run 3 (HR3) N-body simulations, where gravitationally bound dark matter subhalos are identified as the sites of galaxy formation.

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Astronomy & Astrophysics
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