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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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Journal:
Astronomy and Astrophysics More from this journal
Volume:
518
Issue:
4
Publication date:
2010-01-01
EISSN:
1432-0746
ISSN:
0004-6361
Language:
English
Keywords:
Pubs id:
pubs:161722
UUID:
uuid:f209d9f7-e3e6-4c43-8293-fba942184b9d
Local pid:
pubs:161722
Source identifiers:
161722
Deposit date:
2012-12-19

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