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 present seven new transiting hot Jupiters from the WASP‐South survey. The planets are all typical hot Jupiters orbiting stars from F4 to K0 with magnitudes of  V  = 10.3–12.5. The orbital periods are all in the range of 3.9–4.6 d, the planetary masses range from 0.4 to 2.3  M  Jup  and the radii from 1.1 to 1.4  R  Jup . In line with known hot Jupiters, the planetary densities range from Jupiter‐like to inflated (ρ = 0.13–1.07ρ Jup ). We use the increasing numbers of known hot Jupiters to investigate the distribution of their orbital periods and the 3–4 d ‘pile‐up’.

Seven transiting hot Jupiters from WASP‐South, Euler and TRAPPIST: WASP‐47b, WASP‐55b, WASP‐61b, WASP‐62b, WASP‐63b, WASP‐66b and WASP‐67b