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 Plus monthly

Global: Zendy Tools annual

Global: Zendy Tools monthly

Global: Zendy Free Plan

Goodness-of-fit statistics are used to quantitatively establish thecompatibility of CMB anisotropy predictions in a wide range of DMR-normalized,open and spatially-flat $\Lambda$, CDM cosmogonies with the set of allpresently available small-scale CMB anisotropy detection data. Conclusionsregarding model viability depend sensitively on the prescription used toaccount for the 1$\sigma$ uncertainty in the assumed value of the DMRnormalization, except for low-density, $\Omega_0 \sim 0.3$ -- 0.4, open modelswhich are compatible with the data for all prescriptions used. While largebaryon-density ($\Omega_B \gap 0.0175 h^{-2}$), old ($t_0 \gap 15$ -- 16 Gyr),low-density ($\Omega_0 \sim 0.2$ -- 0.4), flat-$\Lambda$ models might beincompatible, no model is incompatible with the data for all prescriptions. Infact, some open models seem to fit the data better than should be expected, andthis might be an indication that some error bars are mildly overconservative.Comment: 15 page PostScript file, including 6 included figures. Also available  via anonymous ftp from ftp://astro.caltech.edu/users/kmg/chi.p

astrophysical journal/the astrophysical journal

Tentative Appraisal of Compatibility of Small-Scale Cosmic Microwave Background Anisotropy Detections in the Context of [ITAL]COBE[/ITAL]-DMR–normalized Open and Flat-Λ Cold Dark Matter Cosmogonies