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 an overview of and status report on the WEAVE next-generationspectroscopy facility for the William Herschel Telescope (WHT). WEAVEprincipally targets optical ground-based follow up of upcoming ground-based(LOFAR) and space-based (Gaia) surveys. WEAVE is a multi-object and multi-IFUfacility utilizing a new 2-degree prime focus field of view at the WHT, with abuffered pick-and-place positioner system hosting 1000 multi-object (MOS)fibres, 20 integral field units, or a single large IFU for each observation.The fibres are fed to a single spectrograph, with a pair of 8k(spectral) x 6k(spatial) pixel cameras, located within the WHT GHRIL enclosure on thetelescope Nasmyth platform, supporting observations at R~5000 over the full370-1000nm wavelength range in a single exposure, or a high resolution modewith limited coverage in each arm at R~20000. The project is now in the finaldesign and early procurement phase, with commissioning at the telescopeexpected in 2017.

Project overview and update on WEAVE: the next generation wide-field spectroscopy facility for the William Herschel Telescope