Claudia G. Scóccola

The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: baryon acoustic oscillations in the Data Release 9 spectroscopic galaxy sample

We present a one per cent measurement of the cosmic distance scale from the detections of the baryon acoustic oscillations in the clustering of galaxies from the Baryon Oscillation Spectroscopic Survey (BOSS), which is part of the Sloan Digital Sky Survey III (SDSS-III). Our results come from the Data Release 11 (DR11) sample, containing nearly one million galaxies and covering approximately

The clustering of galaxies in the SDSS‐III Baryon Oscillation Spectroscopic Survey: cosmological implications of the large‐scale two‐point correlation function

8\,500

The formation and evolution of hydrogen-deficient post-AGB white dwarfs: The emerging chemical profile and the expectations for the PG 1159-DB-DQ evolutionary connection

square degrees and the redshift range

The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: mock galaxy catalogues for the BOSS Final Data Release

0.2<z<0.7

nIFTy cosmology: Galaxy/halo mock catalogue comparison project on clustering statistics

. We also compare these results with those from the publicly released DR9 and DR10 samples. Assuming a concordance

Constraining the halo bispectrum in real and redshift space from perturbation theory and non-linear stochastic bias

\Lambda

Early universe constraints on time variation of fundamental constants

CDM cosmological model, the DR11 sample covers a volume of 13\,Gpc

B polarization of the CMB from Faraday rotation

{}^3

The SDSS-III Baryonic Oscillation Spectroscopic Survey: constraints on the integrated Sachs-Wolfe effect

and is the largest region of the Universe ever surveyed at this density. We measure the correlation function and power spectrum, including density-field reconstruction of the baryon acoustic oscillation (BAO) feature. The acoustic features are detected at a significance of over

Hunting down systematics in baryon acoustic oscillations after cosmic high noon

7\,\sigma