| Issue |
A&A
Volume 570, October 2014
|
|
|---|---|---|
| Article Number | A96 | |
| Number of page(s) | 24 | |
| Section | Extragalactic astronomy | |
| DOI | https://doi.org/10.1051/0004-6361/201423975 | |
| Published online | 29 October 2014 | |
Online material
 |
Fig. 4
Results of the line-fit analysis on theLyα (left panel) Civλ1549 (middle) and 1900 Å emission features for population A sources. The lines are shown after continuum subtraction. The magenta dashed line shows the full model of the emission features and intervening narrow absorptions, if present. The thick black lines show the broad components of the prominent emission lines. The thick blue line traces the BLUE component. The Nvλ1240 line on the red side of theLyα profile is traced by a gray line that includes BC and BLUE. Orange lines are narrow-line components. The lower panel of each frame shows the residuals between the line model and the observations as a function of radial velocity from rest frame (for Ciii]λ1909 in the case of the 1900 blend). |
| Open with DEXTER | |
 |
Fig. 4
continued. |
| Open with DEXTER | |
 |
Fig. 4
continued. |
| Open with DEXTER | |
 |
Fig. 5
Results of the line-fit analysis on theLyα (left panel) Civλ1549 (middle) and 1900 Å emission features for population B sources. The meanings of symbols and colors is as in the previous figure. The VBC assumed to be present in the population B emission line profiles is traced by a thick red line. |
| Open with DEXTER | |
 |
Fig. 5
continued. |
| Open with DEXTER | |
© ESO, 2014
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