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Star formation in AGN hosts in GOODS-N

Abstract:

Sensitive Herschel far-infrared observations can break degeneracies that were inherent to previous studies of star formation in high-z AGN hosts. Combining PACS 100 and 160 μm observations of the GOODS-N field with 2 Ms Chandra data, we detect ∼20% of X-ray AGN individually at >3σ. The host far-infrared luminosity of AGN with L2-10 keV ≈ 10 43 erg s-1 increases with redshift by an order of magnitude from z = 0 to z ∼ 1. In contrast, there is little dependence of far-infrared luminosity on ...

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Publication status:
Published

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Publisher copy:
10.1051/0004-6361/201014606

Authors


Maiolino, R More by this author
Alexander, DM More by this author
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Journal:
ASTRONOMY and ASTROPHYSICS
Volume:
518
Issue:
1
Pages:
L26-L26
Publication date:
2010
DOI:
EISSN:
1432-0746
ISSN:
0004-6361
URN:
uuid:dbbb0cd5-cadf-4225-a816-f3b55d9b7739
Source identifiers:
158937
Local pid:
pubs:158937
Language:
English
Keywords:

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