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 report the results of the first search for gravitational waves fromcompact binary coalescence using data from the LIGO and Virgo detectors. Fivemonths of data were collected during the concurrent S5 (LIGO) and VSR1 (Virgo)science runs. The search focused on signals from binary mergers with a totalmass between 2 and 35 Msun. No gravitational waves are identified. Thecumulative 90%-confidence upper limits on the rate of compact binarycoalescence are calculated for non-spinning binary neutron stars, blackhole-neutron star systems, and binary black holes to be 8.7x10^-3, 2.2x10^-3and 4.4x10^-4 yr^-1 L_10^-1 respectively, where L_10 is 10^10 times the bluesolar luminosity. These upper limits are compared with astrophysicalexpectations.

Search for Gravitational Waves from Compact Binary Coalescence in LIGO and Virgo Data from S5 and VSR1