Cosmology intertwined: A review of the particle physics, astrophysics, and cosmology associated with the cosmological tensions and anomalies

E Abdalla, GF Abellán, A Aboubrahim, A Agnello… - Journal of High Energy …, 2022 - Elsevier
Abstract The standard Λ Cold Dark Matter (ΛCDM) cosmological model provides a good
description of a wide range of astrophysical and cosmological data. However, there are a …

The SDSS-IV extended baryon oscillation spectroscopic survey: overview and early data

KS Dawson, JP Kneib, WJ Percival… - The Astronomical …, 2016 - iopscience.iop.org
In a six-year program started in 2014 July, the Extended Baryon Oscillation Spectroscopic
Survey (eBOSS) will conduct novel cosmological observations using the BOSS …

Target selection and validation of DESI luminous red galaxies

R Zhou, B Dey, JA Newman, DJ Eisenstein… - The Astronomical …, 2023 - iopscience.iop.org
Abstract The Dark Energy Spectroscopic Instrument (DESI) is carrying out a five-year survey
that aims to measure the redshifts of tens of millions of galaxies and quasars, including 8 …

The clustering of the SDSS DR7 main Galaxy sample – I. A 4 per cent distance measure at z = 0.15

AJ Ross, L Samushia, C Howlett… - Monthly Notices of …, 2015 - academic.oup.com
We create a sample of spectroscopically identified galaxies with z< 0.2 from the Sloan
Digital Sky Survey (SDSS) Data Release 7 (DR7), covering 6813 deg2. Galaxies are chosen …

The DESI experiment part I: science, targeting, and survey design

A Aghamousa, J Aguilar, S Ahlen, S Alam… - arXiv preprint arXiv …, 2016 - arxiv.org
DESI (Dark Energy Spectroscopic Instrument) is a Stage IV ground-based dark energy
experiment that will study baryon acoustic oscillations (BAO) and the growth of structure …

Measurement of parity-odd modes in the large-scale 4-point correlation function of Sloan Digital Sky Survey Baryon Oscillation Spectroscopic Survey twelfth data …

J Hou, Z Slepian, RN Cahn - Monthly Notices of the Royal …, 2023 - academic.oup.com
ABSTRACT A tetrahedron is the simplest shape that cannot be rotated into its mirror image
in three-dimension (3D). The 4-point correlation function (4PCF), which quantifies excess …

Cosmological implications of baryon acoustic oscillation measurements

É Aubourg, S Bailey, JE Bautista, F Beutler, V Bhardwaj… - Physical Review D, 2015 - APS
We derive constraints on cosmological parameters and tests of dark energy models from the
combination of baryon acoustic oscillation (BAO) measurements with cosmic microwave …

SDSS-III Baryon Oscillation Spectroscopic Survey Data Release 12: galaxy target selection and large-scale structure catalogues

B Reid, S Ho, N Padmanabhan… - Monthly Notices of …, 2016 - academic.oup.com
Abstract The Baryon Oscillation Spectroscopic Survey (BOSS), part of the Sloan Digital Sky
Survey (SDSS) III project, has provided the largest survey of galaxy redshifts available to …

The baryon oscillation spectroscopic survey of SDSS-III

KS Dawson, DJ Schlegel, CP Ahn… - The Astronomical …, 2012 - iopscience.iop.org
ABSTRACT The Baryon Oscillation Spectroscopic Survey (BOSS) is designed to measure
the scale of baryon acoustic oscillations (BAO) in the clustering of matter over a larger …

The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: baryon acoustic oscillations in the Data Releases 10 and 11 Galaxy samples

L Anderson, E Aubourg, S Bailey… - Monthly Notices of …, 2014 - academic.oup.com
We present a one per cent measurement of the cosmic distance scale from the detections of
the baryon acoustic oscillations (BAO) in the clustering of galaxies from the Baryon …