Astronomy & Astrophysics

All Figures

$\begin{figure} \par\includegraphics[width=8cm,clip]{1072fig1.ps} \end{figure}$ Figure 1: Objects observed with VIMOS-VLT around the Chandra Deep Field South. Black circles are objects in the HST-ACS GOODS area.
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In the text

$\begin{figure} \par\includegraphics[width=8cm,clip]{1072fig2.ps} \end{figure}$ Figure 2: Redshift difference between objects observed twice or more in independent VIMOS observations. The distribution has a velocity dispersion $\sigma _z=0.0012$ or 360 km s^-1, hence the accuracy in redshift measurement is $360/\!\sqrt(2)\sim255$ km s^-1.
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In the text

$\begin{figure} \par\includegraphics[width=8cm,clip]{1072fig3.ps} \end{figure}$ Figure 3: Completeness of the $I_{AB} \leq 24$ sample. ( Top panel) the fraction of secure redshift measurements and all measurements . The overall redshift measurement completeness is 84% with redshifts measurements for 95% of the sample. ( Middle panel) The magnitude distribution of galaxies with secure redshift measurements (open histogram), and failed measurements (filled histogram). See text for the statistical computation of the failed measurements. ( Lower panels) magnitude distribution of the galaxies for each of the quality flags.
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In the text

$\begin{figure} \par\includegraphics[width=8cm,clip]{1072fig4.ps} \end{figure}$ Figure 4: ( Top panel) I_AB magnitude distribution of objects observed with VIMOS in the Chandra Deep Field South (filled histogram), compared to the distribution of all objects in the area in the EIS photometric catalog (open histogram). ( Bottom panel) The ratio of observed vs. all objects is 0.3.
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In the text

$\begin{figure} \par\includegraphics[width=8cm,clip]{1072fig5.eps} \end{figure}$ Figure 5: Redshift distribution of galaxies with $I_{AB} \leq 24$ observed with VIMOS in the Chandra Deep Field South. The redshift bin is dz=0.005. There are 42 objects identified with $z\geq 2$ not included in this figure.
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In the text

$\begin{figure} \par\includegraphics[width=8cm,clip]{1072fig6.ps} \end{figure}$ Figure 6: Absolute M_{B_AB} magnitude - redshift distribution for the full VVDS-CDFS sample
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In the text

$\begin{figure} \par\includegraphics[width=8cm,clip]{1072fig7.ps} \end{figure}$ Figure 7: B_AB-I_AB vs. redshift distribution for the full VVDS-CDFS sample
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In the text

$\begin{figure} \par\includegraphics[width=15.8cm,clip]{1072fig8.ps} \end{figure}$ Figure 8: Output from the VVDS-CDFS CENCOS database output panel for one single object. All information is presented, including the EIS and HST-GOODS identifiers, the ground based and HST-ACS magnitudes, the VVDS redshift and quality flag, and the HST-GOODS images and VVDS spectrum are displayed.
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In the text

$\begin{figure} \par\includegraphics[width=8cm,clip]{1072fig1.ps} \end{figure}$	Figure 1: Objects observed with VIMOS-VLT around the Chandra Deep Field South. Black circles are objects in the HST-ACS GOODS area.
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$\begin{figure} \par\includegraphics[width=8cm,clip]{1072fig2.ps} \end{figure}$	Figure 2: Redshift difference between objects observed twice or more in independent VIMOS observations. The distribution has a velocity dispersion $\sigma _z=0.0012$ or 360 km s^-1, hence the accuracy in redshift measurement is $360/\!\sqrt(2)\sim255$ km s^-1.
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$\begin{figure} \par\includegraphics[width=8cm,clip]{1072fig4.ps} \end{figure}$	Figure 4: ( Top panel) I_AB magnitude distribution of objects observed with VIMOS in the Chandra Deep Field South (filled histogram), compared to the distribution of all objects in the area in the EIS photometric catalog (open histogram). ( Bottom panel) The ratio of observed vs. all objects is 0.3.
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$\begin{figure} \par\includegraphics[width=8cm,clip]{1072fig5.eps} \end{figure}$	Figure 5: Redshift distribution of galaxies with $I_{AB} \leq 24$ observed with VIMOS in the Chandra Deep Field South. The redshift bin is dz=0.005. There are 42 objects identified with $z\geq 2$ not included in this figure.
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$\begin{figure} \par\includegraphics[width=8cm,clip]{1072fig6.ps} \end{figure}$	Figure 6: Absolute M_{B_AB} magnitude - redshift distribution for the full VVDS-CDFS sample
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$\begin{figure} \par\includegraphics[width=8cm,clip]{1072fig7.ps} \end{figure}$	Figure 7: B_AB-I_AB vs. redshift distribution for the full VVDS-CDFS sample
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$\begin{figure} \par\includegraphics[width=15.8cm,clip]{1072fig8.ps} \end{figure}$	Figure 8: Output from the VVDS-CDFS CENCOS database output panel for one single object. All information is presented, including the EIS and HST-GOODS identifiers, the ground based and HST-ACS magnitudes, the VVDS redshift and quality flag, and the HST-GOODS images and VVDS spectrum are displayed.
Open with DEXTER