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...
| Main Authors: | , , , , , , , , , |
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| Format: | Journal Article |
| Published: |
Institute of Physics Publishing
2011
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| Online Access: | http://hdl.handle.net/20.500.11937/52773 |