Table 1: Log of the observations. $\sigma _{{\rm star}}$ denotes the standard deviation of flux in images of the guide star during each integration. Column 6 lists the signal to noise ratio of a one-dimensional spectrum within a 1 $^{\prime \prime }$ radius of the QSO.
Date (UT) Exposure time (s) Airmass Seeing $\sigma _{{\rm star}}$ (%) S/N

Sep. 5 2002 02:48 1800 1.19 1 $^{\prime \prime }$ 0.5 5.9

Sep. 5 2002 03:20 1800 1.19 1 $^{\prime \prime }$ 0.5 5.7

Sep. 8 2002 00:03 1800 1.57 1 $.\!\!^{\prime\prime}$ 3-1 $.\!\!^{\prime\prime}$ 5 10 3.9

Sep. 8 2002 00:36 1800 1.14 1 $.\!\!^{\prime\prime}$ 3-1 $.\!\!^{\prime\prime}$ 5 9 4.2

**Table 1:** Log of the observations. $\sigma _{{\rm star}}$ denotes the standard deviation of flux in images of the guide star during each integration. Column 6 lists the signal to noise ratio of a one-dimensional spectrum within a 1 $^{\prime \prime }$ radius of the QSO.
Date (UT)	Exposure time (s)	Airmass	Seeing	$\sigma _{{\rm star}}$ (%)	S/N
Sep. 5 2002 02:48	1800	1.19	1 $^{\prime \prime }$	0.5	5.9
Sep. 5 2002 03:20	1800	1.19	1 $^{\prime \prime }$	0.5	5.7
Sep. 8 2002 00:03	1800	1.57	1 $.\!\!^{\prime\prime}$ 3-1 $.\!\!^{\prime\prime}$ 5	10	3.9
Sep. 8 2002 00:36	1800	1.14	1 $.\!\!^{\prime\prime}$ 3-1 $.\!\!^{\prime\prime}$ 5	9	4.2

Source LaTeX | All tables | In the text

	1 Introduction
	2 Observations and data reduction
	3 Galaxy and QSO spectra
	4 Derived properties
	5 Kinematics
	6 Discussion
	7 Conclusions
	References