All Figures

$\begin{figure} \par\includegraphics[clip,width=8.8cm]{0954fig1.eps} \end{figure}$ Figure 1: Comparison of new COMBO-17 and GaBoDS photometry. Now, the SED shapes of COMBO-17 and GaBoDS agree. An overall offset remains of $I_{\rm C17}-I_{\rm Gab}=0\hbox{$.\!\!^{\rm m}$ }077$ or $I_{\rm C17}-I_{\rm Mus}\approx 0\hbox{$.\!\!^{\rm m}$ }10$ .
Open with DEXTER

In the text

$\begin{figure} \par\includegraphics[clip,angle=270,width=17cm]{0954fig2.ps} \end{figure}$ Figure 2: Comparison of photometric and spectroscopic redshifts of galaxies: precision is <0.01 rms at R<21 but changes with brightness.
Open with DEXTER

In the text

$\begin{figure} \par\hbox{ \includegraphics[clip,angle=270,width=12cm]{0954fi3a.ps}\includegraphics[clip,angle=270,width=5.1cm]{0954fi3b.ps} } \end{figure}$ Figure 3: Left and centre: comparison of old and new photometric redshifts. Right: change in restframe U-V resulting from the new calibration.
Open with DEXTER

In the text

$\begin{figure} \par\includegraphics[clip,angle=270,width=8.8cm]{0954fig4.ps} \end{figure}$ Figure 4: Left: photometric vs. spectroscopic QSO redshifts: excluding outliers the rms is 0.007 and the bias is consistent with zero. Crosses are objects with two ambiguous photo-z solutions and are responsible for most outliers Right: type-1 AGN, encircled are those classed as QSO by COMBO-17: all but three QSOs with M_B<-22 and z>0.5 are found, while fainter AGN are dominated by the host galaxy SED.
Open with DEXTER

In the text

$\begin{figure} \par\includegraphics[clip,width=8.8cm]{0954fig1.eps} \end{figure}$	Figure 1: Comparison of new COMBO-17 and GaBoDS photometry. Now, the SED shapes of COMBO-17 and GaBoDS agree. An overall offset remains of $I_{\rm C17}-I_{\rm Gab}=0\hbox{$.\!\!^{\rm m}$ }077$ or $I_{\rm C17}-I_{\rm Mus}\approx 0\hbox{$.\!\!^{\rm m}$ }10$ .
Open with DEXTER

$\begin{figure} \par\includegraphics[clip,angle=270,width=17cm]{0954fig2.ps} \end{figure}$	Figure 2: Comparison of photometric and spectroscopic redshifts of galaxies: precision is <0.01 rms at R<21 but changes with brightness.
Open with DEXTER

$\begin{figure} \par\hbox{ \includegraphics[clip,angle=270,width=12cm]{0954fi3a.ps}\includegraphics[clip,angle=270,width=5.1cm]{0954fi3b.ps} } \end{figure}$	Figure 3: Left and centre: comparison of old and new photometric redshifts. Right: change in restframe U-V resulting from the new calibration.
Open with DEXTER