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

The Gaia satellite will be launched at the end of 2011. It will observe atleast 1 billion stars, and among them several million emission line stars andhot stars. Gaia will provide parallaxes for each star and spectra for starstill V magnitude equal to 17. After a general description of Gaia, we presentthe codes and methods, which are currently developed by our team. They willprovide automatically the astrophysical parameters and spectral classificationfor the hot and emission line stars in the Milky Way and other close LocalGroup galaxies such as the Magellanic Clouds.

The Gaia satellite: a tool for Emission Line Stars and Hot Stars