English (United Kingdom)

https://curated-unify.zendy.io/wp-json/zendy-region/v1/featured_content/oa?rat=en

https://curated-unify.zendy.io/wp-json/zendy-region/v1/highlighted_journal/

Global: Zendy Plus annual

Presents the access of premium content as premium feature

Premium Content

Presents the keyphrase highlighting as premium feature

Keyphrase Highlighting

Presents the summarisation as premium feature

Summarisation

Insights

Presents the pdf analysis as premium feature

PDF Analysis

Presents the zaia usage as premium feature

ZAIA

Global: Zendy Tools annual

Global: Zendy Free Plan

Global: Zendy Tools monthly

Global: Zendy Plus monthly

We analyze the anisotropic clustering of the Sloan Digital Sky Survey-IVExtended Baryon Oscillation Spectroscopic Survey (eBOSS) Luminous Red GalaxyData Release 14 (DR14) sample combined with Baryon Oscillation SpectroscopicSurvey (BOSS) CMASS sample of galaxies in the redshift range 0.6$<z<$1.0, whichconsists of 80,118 galaxies from eBOSS and 46,439 galaxies from the BOSS-CMASSsample. The eBOSS-CMASS Luminous Red Galaxy sample has a sky coverage of 1,844deg$^2$, with an effective volume of 0.9 Gpc$^3$. The analysis was made inconfiguration space using a Legendre multipole expansion. The Redshift SpaceDistortion signal is modeled as a combination of the Convolution LagrangianPerturbation Model and the Gaussian Streaming Model.  We constrain the logarithmic growth of structure times the amplitude of darkmatter density fluctuations, $f (z_{\rm eff})\sigma_8(z_{\rm eff})=0.454\pm0.139 $, and the Alcock-Paczynski dilation scales which constraints theangular diameter distance $D_A(z_{eff})=1466.5 \pm 136.6 (r_s/r_s^{\rm fid})$and $H(z_{\rm eff})=105.8 \pm 16 (r_s^{\rm fid}/r_s)\mathrm{km\,s^{-1}\,Mpc^{-1}}$, where $r_s$ is the sound horizon at the end ofthe baryon drag epoch and $r_s^{\rm fid}$ is its value in the fiducialcosmology at an effective redshift $z_{\rm eff}=0.72$. These results are infull agreement with the current $\Lambda$-Cold Dark Matter ($\Lambda$-CDM)cosmological model inferred from Planck measurements. This study is the firsteBOSS LRG full-shape analysis i.e. including Redshift-Space Distortions (RSD)simultaneously with the Alcock-Paczynski (AP) effect and the Baryon AcousticOscillation (BAO) scale.

monthly notices of the royal astronomical society

The clustering of the SDSS-IV extended Baryon Oscillation Spectroscopic  Survey DR14 LRG sample: structure growth rate measurement from the  anisotropic LRG correlation function in the redshift range 0.6 < z < 1.0