Published July 15, 2010
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Type 2 Quasars at the heart of dust-obscured galaxies (DOGs) at high z
Abstract
Dust‐obscured galaxies (DOGs) represent a recently‐discovered, intriguing class of mid‐IR luminous sources at high redshifts. Evidence is mounting that DOGs (selected on the basis of extreme optical/mid‐IR color cut and high mid‐IR flux level) may represent systems caught in the process of host galaxy formation and intense SMBH growth. Here we report the results of an X‐ray spectroscopic survey aimed at studying the X‐ray properties of these sources and establishing the fraction of Type 2 quasars among them.
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© 2010 American Institute of Physics. Published online 15 July 2010.Attached Files
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Additional details
- Eprint ID
- 66329
- Resolver ID
- CaltechAUTHORS:20160420-140504600
- Created
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2016-04-20Created from EPrint's datestamp field
- Updated
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2021-11-10Created from EPrint's last_modified field
- Series Name
- AIP Conference Proceedings
- Series Volume or Issue Number
- 1248