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 Tools annual

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 monthly

Global: Zendy Plus monthly

Presents the access of premium content as premium feature

Premium Content

Global: Zendy Plus annual

Global: Zendy Free Plan

NASA's K2 mission began observing fields along the ecliptic plane in 2014.Each observing campaign lasts approximately 80 days, during whichhigh-precision optical photometry of select astrophysical targets is collectedby the Kepler spacecraft. Due to the 4 arcsec pixel scale of the Keplerphotometer, significant blending between the observed targets can occur(especially in dense fields close to the Galactic plane). We undertook aprogram to use the Wide Field Camera (WFCAM) on the 3.8 m United KingdomInfraRed Telescope (UKIRT) to collect high-spatial-resolution near-infraredimages of targets in select K2 campaign fields, which we report here. These 0.4arcsec resolution K-band images offer the opportunity to perform a variety ofscience, including vetting exoplanet candidates by identifying nearby starsblended with the target star and estimating the size, color, and type ofgalaxies observed by K2.

High-Spatial-Resolution K-Band Imaging of Select K2 Campaign Fields