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 introduce a technique for gravitational-wave analysis, where Gaussianprocess regression is used to emulate the strain spectrum of a stochasticbackground using population-synthesis simulations. This leads to directBayesian inference on astrophysical parameters. For PTAs specifically, weinterpolate over the parameter space of supermassive black-hole binaryenvironments, including 3-body stellar scattering, and evolving orbitaleccentricity. We illustrate our approach on mock data, and assess the prospectsfor inference with data similar to the NANOGrav 9-yr data release.

Constraints On The Dynamical Environments Of Supermassive Black-hole Binaries Using Pulsar-timing Arrays