Astronomy & Astrophysics

All Figures

$\begin{figure} \par\includegraphics[width=7.8cm,clip]{hist.ps} \end{figure}$ Figure 1: The redshift distributions. The shaded histograms indicate the photometric redshifts.
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In the text

$\begin{figure} \par\includegraphics[width=7.8cm,clip]{n2.ps} \end{figure}$ Figure 2: The Sersic index n vs. the spectral (top) and visual morphological class (bottom). Filled symbols: reliable fit of n; open symbols: uncertain fit of n. Spectral classes: -1 = unidentified or unobserved, 1 = passive early-type, 1.5 = early-type + weak [OII] $\lambda$ 3727 emission, 2 = star-forming. Visual morphological classes: 1 = E/S0, 2 = spiral-like, 3 = irregular.
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In the text

$\begin{figure} \par\includegraphics[width=8.7cm,clip]{newfig2.eps} \end{figure}$ Figure 3: Examples of EROs VLT spectra and HST morphologies (ACS filter F850LP, box size = $4\times 4$ arcsec). From top: E/S0 (z=1.096), spiral-like (z=1.222), irregular (z=1.221).
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In the text

$\begin{figure} \par\includegraphics[width=7.8cm,clip]{rkz_tau03.ps} \end{figure}$ Figure 4: $R-K_{\rm s}$ vs. z for the EROs with E/S0 morphology. Continuous lines indicate the predicted colors for different formation redshifts (indicated by the numbers) and $\tau =0.3$ Gyr.
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In the text

$\begin{figure} \par\includegraphics[width=7.8cm,clip]{rkjk_morfo.ps} \end{figure}$ Figure 5: The segregation color-color diagram. The E(B-V) vector is relative to z=1.1 and the Calzetti extinction curve.
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In the text

$\begin{figure} \par\includegraphics[width=7.8cm,clip]{hist.ps} \end{figure}$	Figure 1: The redshift distributions. The shaded histograms indicate the photometric redshifts.
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$\begin{figure} \par\includegraphics[width=7.8cm,clip]{n2.ps} \end{figure}$	Figure 2: The Sersic index n vs. the spectral (top) and visual morphological class (bottom). Filled symbols: reliable fit of n; open symbols: uncertain fit of n. Spectral classes: -1 = unidentified or unobserved, 1 = passive early-type, 1.5 = early-type + weak [OII] $\lambda$ 3727 emission, 2 = star-forming. Visual morphological classes: 1 = E/S0, 2 = spiral-like, 3 = irregular.
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$\begin{figure} \par\includegraphics[width=8.7cm,clip]{newfig2.eps} \end{figure}$	Figure 3: Examples of EROs VLT spectra and HST morphologies (ACS filter F850LP, box size = $4\times 4$ arcsec). From top: E/S0 (z=1.096), spiral-like (z=1.222), irregular (z=1.221).
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$\begin{figure} \par\includegraphics[width=7.8cm,clip]{rkz_tau03.ps} \end{figure}$	Figure 4: $R-K_{\rm s}$ vs. z for the EROs with E/S0 morphology. Continuous lines indicate the predicted colors for different formation redshifts (indicated by the numbers) and $\tau =0.3$ Gyr.
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$\begin{figure} \par\includegraphics[width=7.8cm,clip]{rkjk_morfo.ps} \end{figure}$	Figure 5: The segregation color-color diagram. The E(B-V) vector is relative to z=1.1 and the Calzetti extinction curve.
Open with DEXTER