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

Presently only 30% of short gamma ray bursts (SGRBs) have accurate redshifts,and this sample is highly biased by the limited sensitivity of {\it Swift} todetect SGRBs. We account for the dominant biases to calculate a realistic SGRBrate density out to $z = 0.5$ using the {\it Swift} sample of peak fluxes,redshifts, and those SGRBs with a beaming angle constraint from X-ray/opticalobservations. Assuming a significant fraction of binary neutron star mergersproduce SGRBs, we calculate lower and upper detection rate limits of (1-180)per Yr by an advanced LIGO and Virgo coincidence search. Our detection rate iscompatible with extrapolations using Galactic pulsar observations andpopulation synthesis.

The Swift short gamma-ray burst rate density: prospects for detecting binary neutron star mergers by aLIGO