The First Hyper-Luminous Infrared Galaxy Discovered by WISE
Abstract
We report the discovery by the Wide-field Infrared Survey Explorer of the z = 2.452 source WISE J181417.29+341224.9, the first hyperluminous source found in the WISE survey. WISE 1814+3412 is also the prototype for an all-sky sample of ~1000 extremely luminous "W1W2-dropouts" (sources faint or undetected by WISE at 3.4 and 4.6 microns and well detected at 12 or 22 microns). The WISE data and a 350 micron detection give a minimum bolometric luminosity of 3.7 x 10^13 Lsun, with ~10^14 Lsun plausible. Followup images reveal four nearby sources: a QSO and two Lyman Break Galaxies (LBGs) at z = 2.45, and an M dwarf star. The brighter LBG dominates the bolometric emission. Gravitational lensing is unlikely given the source locations and their different spectra and colors. The dominant LBG spectrum indicates a star formation rate ~300 Msun/yr, accounting for < 10% of the bolometric luminosity. Strong 22 micron emission relative to 350 microns implies that warm dust contributes significantly to the luminosity, while cooler dust normally associated with starbursts is constrained by an upper limit at 1.1 mm. Radio emission is ~10x above the far-infrared/radio correlation, indicating an active galactic nucleus is present. An obscured AGN combined with starburst and evolved stellar components can account for the observations. If the black hole mass follows the local M_BH-bulge mass relation, the implied Eddington ratio is >~4. WISE 1814+3412 may be a heavily obscured object where the peak AGN activity occurred prior to the peak era of star formation.
Cite
@article{arxiv.1208.5517,
title = {The First Hyper-Luminous Infrared Galaxy Discovered by WISE},
author = {Peter R. M. Eisenhardt and Jingwen Wu and Chao-Wei Tsai and Roberto Assef and Dominic Benford and Andrew Blain and Carrie Bridge and J. J. Condon and Michael C. Cushing and Roc Cutri and Neal J. Evans and Chris Gelino and Roger L. Griffith and Carl J. Grillmair and Tom Jarrett and Carol J. Lonsdale and Frank J. Masci and Brian S. Mason and Sara Petty and Jack Sayers and S. Adam Stanford and Daniel Stern and Edward L. Wright and Lin Yan},
journal= {arXiv preprint arXiv:1208.5517},
year = {2012}
}
Comments
Published in 2012 August 20 Astrophysical Journal