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 a new 3D map of interstellar dust reddening, covering threequarters of the sky (declinations greater than -30 degrees) out to a distanceof several kiloparsecs. The map is based on high-quality stellar photometry of800 million stars from Pan-STARRS 1 and 2MASS. We divide the sky intosightlines containing a few hundred stars each, and then infer stellardistances and types, along with the line-of-sight dust distribution. Our newmap incorporates a more accurate average extinction law and an additional 1.5years of Pan-STARRS 1 data, tracing dust to greater extinctions and at higherangular resolutions than our previous map. Out of the plane of the Galaxy, ourmap agrees well with 2D reddening maps derived from far-infrared dust emission.After accounting for a 15% difference in scale, we find a mean scatter of 10%between our map and the Planck far-infrared emission-based dust map, out to adepth of 0.8 mag in E(r-z), with the level of agreement varying over the sky.Our map can be downloaded at http://argonaut.skymaps.info, or by its DOI:10.7910/DVN/LCYHJG.

Galactic Reddening in 3D from Stellar Photometry - An Improved Map