X-ray properties of extreme UV-Fe II emitters

Details X-ray properties of extreme UV-Fe II emitters X-ray properties of extreme UV-Fe II emitters

Oct 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006xmm..prop..211g&link_type=abstract

XMM-Newton Proposal ID #05058803

Physics

Active Galactic Nuclei, Quasars, Bl-Lac Objects, X-Ray Background, Sdss J1020+1219, Sdss J1032+5022, Sdss J1119+1532, Xmm-Newton Proposal 05058803

Scientific paper

We propose to examine the X-ray spectral and simultaneous Optical Monitor characteristics of a sample of very strong UV-Fe II emitters selected from the Sloan Digital Sky Survey (SDSS). Strong optical Fe II emitters are known to the X-ray community as narrow-line Seyfert 1 galaxies (NLS1) and they exhibit very extreme X-ray properties. Our sample of strong UV-Fe II has not been significantly detected in the RASS leading to the possibility that their X-ray spectra are not typical of NLS1. We propose to observe 8 objects for 10 ks each for a total requested time of 80 ks.

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