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 population of the Galactic X-ray binaries has been mostly probed withmoderately sensitive hard X-ray surveys so far. The eRosita mission willprovide, for the first time a sensitive all-sky X-ray survey in the 2-10 keVenergy range, where the X-ray binaries emit most of the flux and discover thestill unobserved low-luminosity population of these objects. In this paper, webriefly review the current constraints for the X-ray luminosity functions ofhigh- and low-mass X-ray binaries and present our own analysis based theINTEGRAL 9-year Galactic survey, which yields improved constraints. Based onthese results, we estimate the number of new XRBs to be detected in the eRositaall-sky survey

Population of the Galactic X-ray binaries and eRosita