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

A new grid of detailed atmosphere model spectra for hot and moderately coolsubdwarf stars is presented. High-resolution spectra and synthetic photometryare calculated in the range from 1000{\AA} to 10,000{\AA} using Non-LTE fullyline-blanketed atmosphere structures. Our grid covers eight temperatures within10,000<Teff [K]<65,000, three surface gravities in the range 4.5<logg[cgs]<6.5, two helium abundances matching two extreme helium-rich andhelium-poor scenarios, and two limiting metallicity boundaries regarding bothsolar ([Fe/H] = 0) and Galactic halo ([Fe/H] = -1.5 and [{\alpha}/Fe] = +0.4).Besides its application in the determination of fundamental parameters ofsubdwarfs in isolation and in binaries, the resulting database is also ofinterest for population synthesis procedures in a wide variety of stellarsystems.

A Grid of Synthetic Spectra for Subdwarfs: Non-LTE line-blanketed atmosphere models