Volume 569, September 2014
|Number of page(s)||10|
|Published online||29 September 2014|
TNG spectra of the RL (first 16 panels) and RQ (second 18 panels) BAL QSOs from our optically bright sample. Units are 10-16 erg/s/cm2/Å vs. μm. Regions where atmospheric transmittance becomes critical have been blanked (1.35–1.44 μm and 1.81–1.94 μm). Dashed lines indicate the position of the Mg ii (left side) and Hβ (right side) emission lines at rest-frame.
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© ESO, 2014
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