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

The mechanisms of the formation and evolution of the Milky Way are encoded inthe orbits, chemistry and ages of its stars. With the 4MOST MIlky way Disk AndBuLgE Low-Resolution Survey (4MIDABLE-LR) we aim to study kinematic andchemical substructures in the Milky Way disc and bulge region with samples ofunprecedented size out to larger distances and greater precision thanconceivable with Gaia alone or any other ongoing or planned survey. Gaia givesus the unique opportunity for target selection based almost entirely onparallax and magnitude range, hence increasing the efficiency in samplinglarger Milky Way volumes with well-defined and effective selection functions.Our main goal is to provide a detailed chrono-chemo-kinematical extended map ofour Galaxy and the largest Gaia follow-up down to $G = 19$ magnitudes (Vega).The complex nature of the disc components (for example, large target densitiesand highly structured extinction distribution in the Milky Way bulge and discarea), prompted us to develop a survey strategy with five main sub-surveys thatare tailored to answer the still open questions about the assembly andevolution of our Galaxy, while taking full advantage of the Gaia data.

4MOST Consortium Survey 3: Milky Way Disc and Bulge Low-Resolution Survey (4MIDABLE-LR)