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Tracing black hole accretion with SED decomposition and IR lines: from local galaxies to the high-z Universe

Abstract:

We present new estimates of AGN accretion and star formation (SF) luminosity in galaxies obtained for the local 12 μm sample of Seyfert galaxies (12MGS), by performing a detailed broad-band spectral energy distribution (SED) decomposition including the emission of stars, dust heated by SF and a possible AGN dusty torus. Thanks to the availability of data from the X-rays to the sub-millimetre, we constrain and test the contribution of the stellar, AGN and SF components to the SEDs. The availab...

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Publication status:
Published
Peer review status:
Peer reviewed

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Publisher copy:
10.1093/mnras/stw577

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Institution:
University of Oxford
Division:
MPLS Division
Department:
Physics
Sub department:
Astrophysics
Role:
Author
Publisher:
Oxford University Press
Journal:
Monthly Notices of the Royal Astronomical Society More from this journal
Volume:
477
Issue:
2
Pages:
2815-2816
Publication date:
2018-03-23
Acceptance date:
2018-03-21
DOI:
EISSN:
1365-2966
ISSN:
0035-8711
Keywords:
Pubs id:
pubs:883888
UUID:
uuid:657f4bfc-234b-4ba5-8d1f-7c1fa138b7a1
Local pid:
pubs:883888
Source identifiers:
883888
Deposit date:
2018-09-28

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