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

We introduce IGM-Vis, a novel astrophysics visualization and data analysisapplication for investigating galaxies and the gas that surrounds them incontext with their larger scale environment, the Cosmic Web. Environment is animportant factor in the evolution of galaxies from actively forming stars toquiescent states with little, if any, discernible star formation activity. Thegaseous halos of galaxies (the circumgalactic medium, or CGM) play a criticalrole in their evolution, because the gas necessary to fuel star formation andany gas expelled from widely observed galactic winds must encounter thisinterface region between galaxies and the intergalactic medium (IGM). Wepresent a taxonomy of tasks typically employed in IGM/CGM studies informed by asurvey of astrophysicists at various career levels, and demonstrate how thesetasks are facilitated via the use of our visualization software. Finally, weevaluate the effectiveness of IGM-Vis through two in-depth use cases thatdepict real-world analysis sessions that use IGM/CGM data.

IGM-Vis: Analyzing Intergalactic and Circumgalactic Medium Absorption Using Quasar Sightlines in a Cosmic Web Context