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Presentation . 2016
License: CC BY
Data sources: Datacite
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Other literature type . 2016
License: CC BY
Data sources: ZENODO
https://dx.doi.org/10.5281/zen...
Other literature type
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https://dx.doi.org/10.5281/zen...
Other literature type
Data sources: Microsoft Academic Graph
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Agn Diagnostic Plot In The Wise And 3Xmm Era: The Role Of Variability

descriptionPublicationkeyboard_double_arrow_right Presentation , Other literature type 29 Oct 2016Publisher:Zenodo
Authors: Zaino, Alessandra; Severgnini, P.; Vignali, C.; Della Ceca, R.; Ballo, L.;

doi: 10.5281/zenodo.163800

Agn Diagnostic Plot In The Wise And 3Xmm Era: The Role Of Variability

Abstract

An efficient diagnostic method to find local (z<0.1) Compton-thick AGN consists in selecting sources characterized by hard X- ray colors and low hard X-ray over mid-IR flux ratio. This has been done efficiently in the past using 2XMM and IRAS data (Severgnini et al. 2012). In this talk I will present my thesis work in which I tested this technique using the latest 3XMM and WISE data for the sample presented by Severgnini et al. I will also briefly discuss the X-ray spectral properties of all of those sources showing flux and/or spectral variability in the XMM-Newton observations.

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Keywords

active galactic nuclei, AGN

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This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
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