pith. sign in

arxiv: 0709.3268 · v2 · submitted 2007-09-20 · 🌌 astro-ph

FERO (Finding Extreme Relativistic Objects): statistics of relativistic broad Fe K alpha lines in AGN

A. L. Longinotti (1) , I. de La Calle (1) , S. Bianchi (2) , M. Guainazzi (1) , M. Dovciak (3) (1 ESAC Madrid - 2 Universita' degli studi Roma Tre - 3 Astronomical Institute , Academy of Science , Prague) This is my paper
classification 🌌 astro-ph
keywords alphabroadlinerelativisticactiveanalysisarchivalbroadened
0
0 comments X
read the original abstract

The properties of the relativistically broadened Fe K alpha line emitted in Active Galactic Nuclei (AGN) are still debated among the AGN community. Recent works seem to exclude that the broad Fe line is a common feature of AGN. The analysis of a large sample composed by 157 XMM-Newton archival observations of radio quiet AGN is presented here. This ongoing project is a development of the work reported in Guainazzi et al. 2006.

This paper has not been read by Pith yet.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.