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 characterize the SWIRE galaxy populations in the SWIRE validation fieldwithin the Lockman Hole, based on the 3.6-24$\mu$ Spitzer data and deepU,g',r',r' optical imaging within an area ~1/3 sq. deg for ~16,000Spitzer-SWIRE sources. The entire SWIRE survey will discover over 2.3 milliongalaxies at 3.6$\mu$m and almost 350,000 at 24$\mu$m; ~70,000 of these will be5-band 3.6-24$\mu$ detections. The colors cover a broad range, generally wellrepresented by redshifted spectral energy distributions of known galaxypopulations, however significant samples of unusually blue objects in the[3.6-4.5]$\mu$m color are found, as well as many objects very red in the3.6-24$\mu$m mid-IR. Nine of these are investigated and are interpreted asstar-forming systems, starbursts and AGN from z=0.37 to 2.8, with luminositiesfrom L$_{IR}$=10$^{10.3}$ to 10$^{13.7}$ L$_{\odot}$Comment: Accepted for publication in the ApJ Supplements Spitzer Special Issue  17 pages, 4 figure

First Insights into the Spitzer Wide‐Area Infrared Extragalactic Legacy Survey (SWIRE) Galaxy Populations