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 Tools annual

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 monthly

Global: Zendy Plus monthly

Presents the access of premium content as premium feature

Premium Content

Global: Zendy Plus annual

Global: Zendy Free Plan

The PULSE@Parkes project has been designed to monitor the rotation of radiopulsars over time spans of days to years. The observations are obtained usingthe Parkes 64-m and 12-m radio telescopes by Australian and international highschool students. These students learn the basis of radio astronomy andundertake small projects with their observations. The data are fully calibratedand obtained with the state-of-the-art pulsar hardware available at Parkes. Thefinal data sets are archived and are currently being used to carry out studiesof 1) pulsar glitches, 2) timing noise, 3) pulse profile stability over longtime scales and 4) the extreme nulling phenomenon. The data are also includedin other projects such as gamma-ray observatory support and for the ParkesPulsar Timing Array project. In this paper we describe the current status ofthe project and present the first scientific results from the Parkes 12-m radiotelescope. We emphasise that this project offers a straightforward means toenthuse high school students and the general public about radio astronomy whileobtaining scientifically valuable data sets.

The PULSE@Parkes project: A new observing technique for long-term pulsar monitoring