Astronomy & Astrophysics

All Figures

$\begin{figure} \par\includegraphics[angle=-90,width=8.8cm,clip]{0109fig3.ps}\end{figure}$ Figure 3: Median redshift as a function of $I_{{\rm AB}}$ .
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In the text

$\begin{figure} \par\includegraphics[angle=-90,width=8.8cm,clip]{0109fig4.ps}\end{figure}$ Figure 4: Redshift distribution for all objects with confirmed spectroscopic redshifts.
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In the text

$\begin{figure} \par\includegraphics[angle=-90,width=8.8cm,clip]{0109fig5.ps}\end{figure}$ Figure 5: [OII] luminosity function based on the $V_{{\rm max}}$ method with no extinction-corrections applied.
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In the text

$\begin{figure} \par\includegraphics[angle=-90,width=8.8cm,clip]{0109fig6.ps}\end{figure}$ Figure 6: [OII] luminosity density as a function of median redshift.
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In the text

$\begin{figure} \par\includegraphics[angle=-90,width=8.8cm,clip]{0109fig7.ps}\end{figure}$ Figure 7: SFR densities based on the present data, supplemented with literature values. Both the observed and extinction-corrected values are shown for the present sample and are represented as open and filled squares. Filled diamonds correspond to Gallego et al. (2002); filled triangles are for Hammer et al. (1997), filled pentagons for Vanzella et al. (2002) and filled stars are for Steidel et al. (1997).
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In the text

$\begin{figure} \par\subfigure[]{\includegraphics[height=17.6cm,width=15cm,clip]{0109fig1a.ps} } \end{figure}$ Figure 1: Spectra of galaxies observed in the HDFS. The ordinate gives the flux (in erg cm^-2 s^-1 Å^-1). The wavelength coverage extends between 4200 Å and 8200 Å. The numbers on the top left corner of the spectra correspond to objects from Table 2 while the second number denotes the redshift. Note that for objects 1-39 the resolution is $\Delta \lambda / \lambda \sim$ 440 while for objects 40 to 94 resolution is $\Delta \lambda / \lambda \sim$ 260 (due to different grism filter combination). Since the wavelength coverage is common we present both spectra together.
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In the text

$\begin{figure}\par\subfigure[]{\includegraphics[height=19.1cm,width=15cm,clip]{0109fig1b.ps} } \end{figure}$ Figure 1: continued.
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In the text

$\begin{figure}\par\subfigure[]{\includegraphics[height=19.1cm,width=15cm,clip]{0109fig1c.ps} } \end{figure}$ Figure 1: continued.
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In the text

$\begin{figure}\par\subfigure[]{\includegraphics[height=19.1cm,width=15cm,clip]{0109fig1d.ps} } \end{figure}$ Figure 1: continued.
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In the text

$\begin{figure}\par\subfigure[]{\includegraphics[height=19.1cm,width=15cm,clip]{0109fig1e.ps} } \end{figure}$ Figure 1: continued.
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In the text

$\begin{figure}\par\subfigure[]{\includegraphics[height=19.1cm,width=15cm,clip]{0109fig1f.ps} } \end{figure}$ Figure 1: continued.
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In the text

$\begin{figure}\par\subfigure[]{\includegraphics[height=9.7cm,width=15cm,clip]{0109fig1g.ps} } \end{figure}$ Figure 1: continued.
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In the text

$\begin{figure} \par\subfigure[]{\includegraphics[height=23cm,width=16cm,clip]{0109fig2a.ps} } \end{figure}$ Figure 2: Same as Fig. 1. The wavelength coverage extends between 6000-9200 Å.
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In the text

$\begin{figure} \par\subfigure[]{\includegraphics[height=9.5cm,width=16cm,clip]{0109fig2b.ps} } \end{figure}$ Figure 2: continued.
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In the text

$\begin{figure} \par\includegraphics[angle=-90,width=8.8cm,clip]{0109fig3.ps}\end{figure}$	Figure 3: Median redshift as a function of $I_{{\rm AB}}$ .
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$\begin{figure} \par\includegraphics[angle=-90,width=8.8cm,clip]{0109fig4.ps}\end{figure}$	Figure 4: Redshift distribution for all objects with confirmed spectroscopic redshifts.
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$\begin{figure} \par\includegraphics[angle=-90,width=8.8cm,clip]{0109fig5.ps}\end{figure}$	Figure 5: [OII] luminosity function based on the $V_{{\rm max}}$ method with no extinction-corrections applied.
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$\begin{figure} \par\includegraphics[angle=-90,width=8.8cm,clip]{0109fig6.ps}\end{figure}$	Figure 6: [OII] luminosity density as a function of median redshift.
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$\begin{figure}\par\subfigure[]{\includegraphics[height=19.1cm,width=15cm,clip]{0109fig1b.ps} } \end{figure}$	Figure 1: continued.
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$\begin{figure} \par\subfigure[]{\includegraphics[height=23cm,width=16cm,clip]{0109fig2a.ps} } \end{figure}$	Figure 2: Same as Fig. 1. The wavelength coverage extends between 6000-9200 Å.
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$\begin{figure} \par\subfigure[]{\includegraphics[height=9.5cm,width=16cm,clip]{0109fig2b.ps} } \end{figure}$	Figure 2: continued.
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