The ultraviolet-to-mid-infrared spectral energy distribution of weak emission line quasars

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The ultraviolet-to-mid-infrared spectral energy distribution of weak emission line quasars

We present Spitzer Space Telescope photometry of 18 Sloan Digital Sky Survey (SDSS) quasars at 2.7 = z = 5.9 which have weak or undetectable high-ionization emission lines in their rest-frame ultraviolet (UV) spectra (hereafter weak-lined quasars, or WLQs). The Spitzer data are combined with SDSS sp...

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Bibliographic Details
Main Authors:	Lane, R., Shemmer, O., Diamond-Stanic, A., Fan, X., Anderson, S., Brandt, W., Plotkin, Richard, Richards, G., Schneider, D., Strauss, M.
Format:	Journal Article
Published:	Institute of Physics Publishing 2011
Online Access:	http://hdl.handle.net/20.500.11937/52773

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