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 optical through radio observations of the host galaxies of twodust obscured, luminous quasars selected in the mid-infrared, at z=2.62 andz=2.99, including a search for CO emission. Our limits on the CO luminositiesare consistent with these objects having masses of molecular gas <~10^10 solarmasses, several times less than those of luminous submillimeter-detectedgalaxies (SMGs) at comparable redshifts. Their near-infrared spectral energydistributions, however, imply that these galaxies have high stellar masses(~10^11-12 solar masses). The relatively small reservoirs of molecular gas andlow dust masses are consistent with them being relatively mature systems athigh-z.

The stellar, molecular gas and dust content of the host galaxies of two z~2.8 dust obscured quasars