DUST-OBSCURED RADIO AGNS FROM THE WISE SURVEY

DUST-OBSCURED RADIO AGNS FROM THE WISE SURVEY

Feedback from accreting BH (AGN) is thought to be responsible for the co-evolution of BHs and galaxies. It is likely to be prominent in the most luminous dust-obscured quasars, particularly those containing radio sources too luminous to be powered by starbursts. In order to investigate the feedback...

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Veröffentlicht in:Publications of The Korean Astronomical Society 2012-09, Vol.27 (4), p.289-290
Hauptverfasser: Kim, Minjin, Lonsdale, Carol J., Lacy, Mark, Kimball, Amy, Condon, Jim
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container_issue 4
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container_title Publications of The Korean Astronomical Society
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creator Kim, Minjin
Lonsdale, Carol J.
Lacy, Mark
Kimball, Amy
Condon, Jim
description Feedback from accreting BH (AGN) is thought to be responsible for the co-evolution of BHs and galaxies. It is likely to be prominent in the most luminous dust-obscured quasars, particularly those containing radio sources too luminous to be powered by starbursts. In order to investigate the feedback mechanism in detail, we select a unique sample containing ~ 200 of the most luminous obscured QSOs by cross-matching the WISE catalog with the FIRST and NVSS radio surveys. We present overall statistics for the observed range of colors and radio/mid-IR flux density ratio. We also present our efforts to understand the physical and evolutionary nature of these extreme feedback candidates using various telescopes such as Magellan, SOAR, Herschel, and ALMA.
doi_str_mv 10.5303/PKAS.2012.27.4.289
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