Understanding the extreme soft X-ray excess in RE 1034+396

Details Understanding the extreme soft X-ray excess in RE 1034+396 Understanding the extreme soft X-ray excess in RE 1034+396

Oct 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006xmm..prop..236w&link_type=abstract

XMM-Newton Proposal ID #05064401

Physics

Active Galactic Nuclei, Quasars, Bl-Lac Objects, X-Ray Background, Re 1034+396, Xmm-Newton Proposal 05064401

Scientific paper

We propose a 90ks XMM--Newton observation of the Narrow Line Seyfert 1 galaxy RE 1034+396. This has the strongest soft X-ray excess ever seen in an active galaxy (AGN). It also has extremely low absorption in the line-of-sight, so has excellent FUSE/EUVE/HST data to delineate the lower energy extent of the soft X-ray excess and especially how this connects onto the accretion disc emission. RE1034+396 thus represents the extreme of the NLS1 population, and the best hope for constraining the nature of the soft excess.

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