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

FLARE (First Light And Reionization Explorer) is a space mission that will besubmitted to ESA (M5 call). Its primary goal (about 80% of lifetime) is toidentify and study galaxies that dwell in the universe before the end of thereionization up to about z = 15, a redshift that might not be statisticallyreachable for JWST, Euclid and WFIRST. A secondary objective (about 20% oflifetime) is to survey star formation in the Milky Way.  The strategy selected for FLARE optimizes the science return: imaging andspectroscopic integral-field observations will be carried out simultaneously ontwo parallel focal planes and over very wide instantaneous fields of view.FLARE will feature an instantaneous field of view of about 0.2 deg$^2$ with0.2-arcsec pixels and an instantaneous integral-field spectroscopic field ofview of about 1 arcmin$^2$ with R = 500 - 1000 and an angular resolution ofabout 0.4 arcsec. To detect first-light galaxies, the imaging and spectroscopicsurvey (parallel observations over about 6 years) will reach m$_{AB}$ = 28 andf$_{\lambda}$ = 10$^{-18}$ erg/cm$^2$/S.  FLARE will help addressing two of ESA's Cosmic Vision themes: a) "How did theuniverse originate and what is it made of?" and b) "What are the conditions forplanet formation and the emergence of life?" and more specifically, "From gasand dust to stars and planets".  FLARE will provide to the ESA community a leading position to statisticallystudy the early universe after JWST's deep but pin-hole surveys. Moreover, theinstrumental development of wide-field imaging and wide-field integral-fieldspectroscopy in space will be a major breakthrough after making them availableon ground-based telescopes.

The FLARE mission: Deep and Wide-field 1-5$\mu$m Imaging and Spectroscopy for the Early Universe: a proposal for M5 Cosmic Vision call