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From: jxw@ustc.edu.cn
Subject: XMM reveals difference in narrow FeK line emission between type 1 and type 2 AGNs
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Date: Tue, 26 Oct 2010 07:35:22 GMT
From: jxw@ustc.edu.cn
To: xmmhelp@sciops.esa.int
Cc: jxw@ustc.edu.cn
Subject: XMM reveals difference in narrow FeK line emission between type 1 and type 2 AGNs
Full_Name: Junxian Wang
Submission from: (NULL) (218.22.21.22)



I am writing in response to the Call for XMM-Newton results with potential for
ESA press releases.

I would like to inform you our new significant XMM science results. The work was
finished by one of my student and myself. The paper was accepted by ApJ and is
scheduled for the December 10, 2010, v725 -1 issue. The preprint of the paper is
available at http://arxiv.org/abs/1010.4811

In this work we provide the first observational evidence showing the narrow Fe
Kalpha line emission in AGN X-ray spectra is anisotropic, and its important
applications. 

All the best
Junxian Wang


Reply 1

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From: Ignacio de la Calle <xmmhelp@sciops.esa.int>
To: jxw@ustc.edu.cn
Subject: Re: XMM reveals difference in narrow FeK line emission between type 1 and type 2 AGNs (PR#46154)
Date: Wed Oct 27 08:19:27 2010
Dear Junxian,

Many thanks for making us aware of this. The Project Scientist
has been notified and will look into it and let you know of
any possible outcome.

Best regards,

Ignacio de la Calle
XMM-Newton SOc

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