Carrie R. Bridge, Andrew Blain, Colin J. K. Borys, Sara Petty, Dominic Benford, Peter Eisenhardt, Duncan Farrah, Roger L. Griffith, Tom Jarrett, S. Adam Stanford, Daniel Stern, Chao-Wei Tsai, Edward L. Wright, Jingwen Wu
We report a new technique to select 1.610^{13-14}L_sun) and warm colors, typically larger than submillimeter-selected galaxies (SMGs) and dust-obscured galaxies (DOGs). These traits are commonly associated with the dust being energized by intense AGN activity. We hypothesize that the combination of spatially extended Lyman-alpha, large amounts of warm IR-luminous dust, and rarity (implying a short-lived phase) can be explained if the galaxies are undergoing strong `feedback' transforming them from an extreme dusty starburst to a QSO.
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http://arxiv.org/abs/1205.4030
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