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

Einstein@Home aggregates the computer power of hundreds of thousands ofvolunteers from 193 countries, to search for new neutron stars using data fromelectromagnetic and gravitational-wave detectors. This paper presents adetailed description of the search for new radio pulsars using Pulsar ALFAsurvey data from the Arecibo Observatory. The enormous computing power allowsthis search to cover a new region of parameter space; it can detect pulsars inbinary systems with orbital periods as short as 11 minutes. We also describethe first Einstein@Home discovery, the 40.8 Hz isolated pulsar PSR J2007+2722,and provide a full timing model. PSR J2007+2722's pulse profile is remarkablywide with emission over almost the entire spin period. This neutron star ismost likely a disrupted recycled pulsar, about as old as its characteristicspin-down age of 404 Myr. However there is a small chance that it was bornrecently, with a low magnetic field. If so, upper limits on the X-ray fluxsuggest but can not prove that PSR J2007+2722 is at least ~ 100 kyr old. In thefuture, we expect that the massive computing power provided by volunteersshould enable many additional radio pulsar discoveries.

The Einstein@Home search for radio pulsars and PSR J2007+2722 discovery