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

An international consortium is presently constructing a beamformer for theAtacama Large Millimeter/submillimeter Array (ALMA) in Chile that will beavailable as a facility instrument. The beamformer will aggregate the entirecollecting area of the array into a single, very large aperture. Theextraordinary sensitivity of phased ALMA, combined with the extremely fineangular resolution available on baselines to the Northern Hemisphere, willenable transformational new very long baseline interferometry (VLBI)observations in Bands 6 and 7 (1.3 and 0.8 mm) and provide substantialimprovements to existing VLBI arrays in Bands 1 and 3 (7 and 3 mm). The ALMAbeamformer will have impact on a variety of scientific topics, includingaccretion and outflow processes around black holes in active galactic nuclei(AGN), tests of general relativity near black holes, jet launch and collimationfrom AGN and microquasars, pulsar and magnetar emission processes, the chemicalhistory of the universe and the evolution of fundamental constants acrosscosmic time, maser science, and astrometry.

High-Angular-Resolution and High-Sensitivity Science Enabled by Beamformed ALMA