All Figures

$\begin{figure} \par\includegraphics[width=7.3cm,clip]{4578f1.ps}\par\vspace*{5mm... ...2.ps}\par\vspace*{5mm} \includegraphics[width=7.4cm,clip]{4578f3.ps}\end{figure}$ Figure 1: One-dimensional spectra of the quasars extracted from the data cubes, by co-adding spectra from 20-30 spaxels. Emission lines have been indicated.
Open with DEXTER

In the text

$\begin{figure} \par\includegraphics[width=5.6cm,clip]{4578f4.ps}\end{figure}$ Figure 2: A narrow-band image of the [O II] emission at z=0.871 (6954-6990 Å) from 3C 196 interpolated to a grid scale of 0 $.\!\!^{\prime\prime}$ 3. The axes are given in arcseconds, and the gray scaling is relative. Residuals from the QSO subtraction are present at the central region, which corresponds to three spaxels. Contours of an image at 7000-7050 Å are overlaid, and the QSO centre is located at (0,-1). The innermost contour corresponds to the FWHM of the QSO PSF. The "+'' signs denote the positions of the radio hot spots. (See the online edition for a colour version of this figure.)
Open with DEXTER

In the text

$\begin{figure} \par\includegraphics[width=7.6cm,clip]{4578f5.ps}\end{figure}$ Figure 3: One-dimensional spectrum of the brightest region to the south of 3C 196 where both [O II] and [Ne III] emission appear extended. These lines are indicated by the vertical lines. The lower panel shows a one-dimensional spectrum of the northern region where no [Ne III] emission is detected.
Open with DEXTER

In the text

$\begin{figure} \par\resizebox{7cm}{5.7cm}{\includegraphics[bb=50 350 475 710,cli... ...7cm}{5.7cm}{\includegraphics[bb=50 350 475 710,clip]{4578f7.ps}}\par\end{figure}$ Figure 4: Upper panel: velocity structures of the extended [O II] emission around 3C 196 determined after the QSO emission was subtracted. The zero-point of the velocity is the QSO redshift. Outlined circles indicate the spectra where no [O II] emission lines could be fit due to their low signal-to-noise levels. One spaxel close to the QSO centre has not been fitted, because the emission line is affected by QSO subtraction residuals. (See the online edition for a colour version of this figure.) Lower panel: image of the [O II] line emission intensity around 3C 196 with velocity contours overlaid. Contour levels are separated by 100 km s^-1 and negative velocities are shown by the dashed lines. The "+'' signs indicate the positions of the two radio hot-spots which are roughly spatially coincident with the brightest emission line regions.
Open with DEXTER

In the text

$\begin{figure} \par\includegraphics[width=5.6cm,clip]{4578f8.ps}\end{figure}$ Figure 5: Narrow-band image of OI 363 created from the INTEGRAL data at $6070<\lambda <6090$ Å which includes [O II] at z=0.63. The scaling has been chosen to show features brighter than 2 $\sigma$ above the background noise, and no EELR features surrounding the quasar are detected. The small features visible in this image are not significant, i.e. they have no associated emission line in an extracted one-dimensional spectrum at this wavelength. The contours show an off-band narrow-band image of the QSO centered at (0, 0) where the innermost contour represents the seeing FWHM. Because of cross talk between spectra positioned next to each other on the CCD, the QSO PSF appears non circular.
Open with DEXTER

In the text

$\begin{figure} \par\includegraphics[width=5.6cm,clip]{4578f9.eps}\end{figure}$ Figure 6: Narrow-band image of the [O II] line emission region from 3C 336 in the region 7167-7193 Å. The image is interpolated to a pixel scale of 0 $.\!\!^{\prime\prime}$ 2 to make visible the faint emission. The field of view is $8\hbox {$^{\prime \prime }$ }\times 8\hbox {$^{\prime \prime }$ }$ , north is up and east to the left. The location of the object denoted "2'' in Steidel et al. (1997) is marked by the "+'' sign. A narrow-band image at slightly redder wavelengths (7190-7206 Å) shows emission at larger distances than in this image, which is consistent with the 2 $.\!\!^{\prime\prime}$ 58 offset reported in Steidel et al. (1997). Contours show an off-band narrow-band image (6950-7000 Å) where the innermost contour represent the seeing FWHM. The dashed line represents the orientation of the radio jet which extends beyond the field of view of the IFS data.
Open with DEXTER

In the text

$\begin{figure} \par\includegraphics[width=7.3cm,clip]{4578f1.ps}\par\vspace{5mm... ...2.ps}\par\vspace{5mm} \includegraphics[width=7.4cm,clip]{4578f3.ps}\end{figure}$	Figure 1: One-dimensional spectra of the quasars extracted from the data cubes, by co-adding spectra from 20-30 spaxels. Emission lines have been indicated.
Open with DEXTER

$\begin{figure} \par\includegraphics[width=7.6cm,clip]{4578f5.ps}\end{figure}$	Figure 3: One-dimensional spectrum of the brightest region to the south of 3C 196 where both [O II] and [Ne III] emission appear extended. These lines are indicated by the vertical lines. The lower panel shows a one-dimensional spectrum of the northern region where no [Ne III] emission is detected.
Open with DEXTER