Iron Line In Integrated Spectra Of CDFS Sources

Details Iron Line In Integrated Spectra Of CDFS Sources Iron Line In Integrated Spectra Of CDFS Sources

Feb 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010head...11.0832b&link_type=abstract

American Astronomical Society, HEAD meeting #11, #8.32; Bulletin of the American Astronomical Society, Vol. 41, p.667

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We will exploit the deepest (so far) Chandra and XMM data ever obtained in the CDFS to perform source stacking study of iron K lines in integrated X-ray spectra as a function of luminosity, redshift, and absorption column density.
The 2Ms Chandra datasets substantially improves the statistics for the low-redshift AGN population (z < 1) and provides new sources detected mostly at z>1. The average properties of AGN will be studied in their rest-frame space, allowing a full characterization of the line intensity and line profile.
The available multi-wavelength data allow us to study Iron-line properties also as a function of the optical properties of the AGN host galaxies (stellar masses, star formation rates), therefore putting the formation of iron in the more general AGN-host galaxies co-evolution framework.

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