UV to Mid-IR SEDs of Low-redshift Quasars

Details UV to Mid-IR SEDs of Low-redshift Quasars UV to Mid-IR SEDs of Low-redshift Quasars

Oct 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aspc..373..604s&link_type=abstract

The Central Engine of Active Galactic Nuclei, ASP Conference Series, Vol. 373, proceedings of the conference held 16-21 October,

Physics

Scientific paper

We present a mean spectral energy distribution (SED) constructed from 15 low-redshift, broad-line quasars using spectroscopic data from the ultraviolet (UV) to the mid-infrared (IR). The mean SED shows more detailed features than previous work. We find a correlation between the UV-optical continuum slope and mid-IR luminosity that we interpret as indicating the existence of line-of-sight dust and reddening even in very blue quasars. We also show that the equivalent width of the 10 micron silicates feature is an important parameter of the optical Eigenvector 1 relationships.

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