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  5. Probing AGN Accretion History Through X-Ray Variability
 

Probing AGN Accretion History Through X-Ray Variability

Date Issued
2016
Author(s)
Paolillo, Maurizio  
•
Papadakis, I.
•
Brandt, W. N.
•
Xue, Y. Q.
•
Luo, B.
•
TOZZI, Paolo  
•
Shemmer, O.
•
Allevato, V.  
•
Bauer, F.
•
Koekemoer, A.
•
Vignali, C.
•
Vito, F.  
•
Yang, G.
•
Wang, J. X.
•
Zheng, X.
DOI
10.5281/zenodo.163795
Abstract
I will present recent results on AGN variability in the CDFS survey. Using over 10 years of X-ray monitoring and comparison with local AGNs we are able to constrain the variability dependence on BH mass and accreton rate, and use it to trace the accretion hisory of the AGN population up to z=3.
Coverage
Active Galactic Nuclei 12: A Multi-Messenger Perspective (AGN12)
Start page
39
Conferenece
Active Galactic Nuclei 12: A Multi-Messenger Perspective (AGN12)
Conferenece place
Napoli, Italy
Conferenece date
26-29 September, 2016
Uri
http://hdl.handle.net/20.500.12386/26425
Url
https://ui.adsabs.harvard.edu/abs/2016agnt.confE..39P/abstract
Ads BibCode
2016agnt.confE..39P
Rights
open.access
File(s)
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Thumbnail Image
Name

agn12_paolillo_talk.pdf

Description
Talk
Size

8.64 MB

Format

Adobe PDF

Checksum (MD5)

4823e4a5a3520afc3f223e11a7de0766

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