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 point out the existence of a second feature in the matter two-pointfunction, besides the acoustic peak, due to the baryon-baryon correlation inthe early universe and positioned at twice the distance of the peak. We discusshow the existence of this feature is implied by the well-known heuristicargument that explains the baryon bump in the correlation function. A standard$\chi^2$ analysis to estimate the detection significance of the second featureis mimicked. We conclude that for realistic values of the baryon density, anSKA-like galaxy survey will not be able to detect this feature with standardcorrelation function analysis.

On the $2^\text{nd}$ feature of the matter two-point function