![\begin{figure}
\par\includegraphics[width=17.55cm,clip]{H4512f3.eps}\par\vspace*{3mm}
\includegraphics[width=17.55cm,clip]{H4512f4.eps}\end{figure}](/articles/aa/full/2004/07/aah4512/Timg34.gif) |
Figure 2:
Portions of the UVES spectrum of SDSS J0011+0055 illustrating the
absorption line systems A and B defined in Table 1.
System B is best seen in C IV and system A in Si IV (C IV at
2.29 is outside the observed UVES spectral range). The
following transitions are indicated: N V
1238.82,
1242.80, C IV
1548.20, 1550.78, Si IV
1393.75, 1402.77, Mg II
2796.35,
2803.53, Si II
1260.42, 1264.74, 1265.00, C II
1334.53, 1335.66, 1335.71, and Ly
1215.67. For clarity, the two reddest and very close transitions of
Si II and C II are represented by single marks at the
mean wavelengths; all four of those transitions are excited-state
transitions. Absorption from the high-velocity system B is not
detected in Si II or C II, and therefore is not plotted although it
lies well within the observed UVES spectral range (Si II 1260.42 could be present in system B1 but the detection is not
convincing). Narrow intervening Mg II
2796.35, 2803.53 absorption contaminates the Si II absorption of
system A2. Narrow intervening C IV 1548.20 lines are seen
slightly longward of the Si IV absorption from system B, along with a
broader instrumental artifact. All spectra are plotted on a velocity
scale of
v/c = (R2-1)/(R2+1) where
,
being
the observed wavelength,
the laboratory vacuum rest
wavelength of the red transition of the multiplets, and
the
systemic redshift of the quasar. |