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 derive the galaxy luminosity functions in V, R, I, and K bands of thecluster EIS 0048 at z~0.64 from data taken at the ESO Very Large Telescope. Thedata span the restframe wavelength range from UV, which is sensitive to evenlow rates of star formation, to the NIR, which maps the bulk of the stellarmass. By comparing our data and previous results with pure luminosity evolutionmodels, we conclude that bright (M<= M^*+1) cluster galaxies are alreadyassembled at z~1 and that star formation is almost completed at z~1.5.Comment: 11 pages, 5 figures. A&A accepte

UV–NIR restframe luminosity functions of the galaxy cluster EIS 0048 atz$\mathsf{\,\sim 0.64}$