Deep IRAC Imaging of the z=2.45 Hyper-Luminous IR Galaxy WISE 1814+34

Details Deep IRAC Imaging of the z=2.45 Hyper-Luminous IR Galaxy WISE 1814+34 Deep IRAC Imaging of the z=2.45 Hyper-Luminous IR Galaxy WISE 1814+34

Jun 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010sptz.prop..549e&link_type=abstract

Spitzer Proposal ID #549

Physics

Scientific paper

We have recently measured a redshift of 2.45 for an unusual WISE source (WISE 1814+34) which rises steeply from 12 to 22 microns and is undetected at 3.4 and 4.6 microns. The source is also detected at 20 cm, and appears to be a Hyper Luminous IR galaxy with well above 1E14 solar luminosities. We propose to observe WISE 1814+34 with IRAC on warm Spitzer at 3.4 and 4.6 microns to a depth 40 times better than WISE, to help assess whether the source is powered by AGN or star formation, whether it is gravitationally lensed, and whether it shows evidence for merging.

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