All Figures

$\begin{figure} \par\includegraphics[width=5.4cm,clip]{8545fig1.ps}\hspace*{5mm} ... ...g5.ps}\hspace*{5mm} \includegraphics[width=5.4cm,clip]{8545fig6.ps} \end{figure}$ Figure 1: Optical/NIR data coverage for DEEP1a ( top) and DEEP1b ( bottom). From left to right coverage in the K-band (shallow and deep strategies) and J-band (deep strategy only).
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In the text

$\begin{figure} \par\includegraphics[width=6.6cm,clip]{8545fig7.ps}\par\vspace{8mm} \includegraphics[width=6.6cm,clip]{8545fig8.ps}\end{figure}$ Figure 2: U-B vs. B-V colour diagram for stars in field DEEP1b. No correction applied ( top), correction $U_{\rm corr}=-0.15$ applied ( bottom). Green points refer to DPS stars, black dots to modelled stars.
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In the text

$\begin{figure} \par\includegraphics[width=6.6cm,clip]{8545fig9.ps}\par\vspace{8mm} \includegraphics[width=6.6cm,clip]{8545fg10.ps}\end{figure}$ Figure 3: Optical vs. infrared colour-colour diagram for stars in DEEP1b: V-R vs. R-J ( top) and V-R vs. $R-K_{\rm s}$ ( bottom). Green points refer to DPS stars, black dots to modelled stars.
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In the text

$\begin{figure} \par\includegraphics[width=7.1cm,clip]{8545fg11.ps}\end{figure}$ Figure 4: $z_{\rm phot}$ vs. $z_{\rm spec}$ for the 88 galaxies in DEEP1a, b, c fields with spectra available. U-band magnitudes of DEEP1b objects are corrected and NIR information is used, when available. The solid line indicates $z_{\rm phot}=z_{\rm spec}$ and the dotted lines indicate the range that contains 95% of the objects. The error bars represent the limits of the confidence intervals at 68%.
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In the text

$\begin{figure} \par\includegraphics[width=7.7cm,clip]{8545fg12.ps}\end{figure}$ Figure 5: Galaxy photometric redshift distribution for field DEEP1b.
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In the text

$\begin{figure} \par\includegraphics[width=7.1cm,clip]{8545fg13.ps}\end{figure}$ Figure 6: LR values vs. radio-optical offsets for the 85 radio sources located in DEEP1a, b and c. The horizontal solid line indicate the LR value $L_{\rm th}=0.3$ , above which counterparts are considered as good identifications (see text for details).
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In the text

$\begin{figure} \par\includegraphics[height=5.5cm,width=5.5cm,clip]{8545fg14.ps}\... ...{2.5mm} \includegraphics[height=5.5cm,width=5.5cm,clip]{8545fg16.ps}\end{figure}$ Figure 7: The three extended radio sources included a posteriori in the identification sample: two with double radio morphology, ATESP5 J225034-401936 ( left panel) and ATESP5 J225426-402442 ( middle panel); and one wide angle tail source, ATESP5 J225505-401301 ( right panel). Grayscale: optical image in the reference band (R for DEEP1a and I for DEEP1b). Contours: 5 GHz flux density.
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In the text

$\begin{figure} \par\includegraphics[height=5.5cm,width=5.5cm,clip]{8545fg17.ps}\... ...{2.5mm} \includegraphics[height=5.5cm,width=5.5cm,clip]{8545fg19.ps}\end{figure}$ Figure 8: The three sources identified in bands other than the reference one: ATESP5 J224827-402515 ( left panel), identified in I-band; ATESP5 J225443-401147 ( middle panel), identified in $K_{\rm s}$ -band; and ATESP5 J225511-401513 ( right panel), identified in J-band. Grey scale: optical or NIR image. Contours: 5 GHz flux density.
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In the text

$\begin{figure} \par\includegraphics[width=6.9cm,clip]{8545fg20.ps}\end{figure}$ Figure 9: Redshift distribution for the 56 radio sources in the ATESP-DEEP1 sample with photometric redshift determination. The sample is divided into four different classes. From top to bottom: AGNs, ETS, LTS, and star-burst galaxies.
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In the text

$\begin{figure} \par\includegraphics[width=6.9cm,clip]{8545fg21.ps}\end{figure}$ Figure 10: 1.4 GHz radio power distribution for the 56 ATESP-DEEP1 radio sources with photometric redshift determination. The sample is divided into four different classes. From top to bottom: AGNs, ETS, LTS and star-burst galaxies. Light shading indicates two upper limits.
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In the text

$\begin{figure} \par\includegraphics[width=6.9cm,clip]{8545fg22.ps}\end{figure}$ Figure 11: Absolute B-band magnitude distribution. The sample is divided into four different classes. From top to bottom: AGNs, ETS, LTS and star-burst galaxies.
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In the text

$\begin{figure} \par\includegraphics[width=6.9cm,clip]{8545fg23.ps}\end{figure}$ Figure 12: Absolute R-band magnitude distribution. The sample is divided into four different classes. From top to bottom: AGNs, ETS, LTS and star-burst galaxies.
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In the text

$\begin{figure} \par\includegraphics[width=11.2cm,clip]{8545fg24.ps}\end{figure}$ Figure 13: Radio-to-optical ratio (R, top panel), linear radio source size (d in kpc, middle panel) and 1.4 GHz radio power (in W/Hz, bottom panel) against 1.4-5 GHz spectral index for the radio sources from the ATESP-DEEP1 sample: red filled circles (ETS); blue stars (LTS/SB); green filled triangles (AGNs). Circled symbols indicate sources with extended and/or two-component radio morphology, typical of classical radio galaxies. Black open circles are for identified sources that do not have a redshift/type determination. Arrows indicate upper/lower limits. Vertical dashed lines indicate the $\alpha =-0.5$ and the $\alpha =0$ values, above which source spectra are defined respectively as flat and inverted. Horizontal dashed lines in the three panels indicate, from top to bottom, values of R=1000, d=30 kpc and $P_{\rm 1.4~GHz}=10^{24}$ W/Hz, respectively.
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In the text

$\begin{figure} \par\includegraphics[width=5.4cm,clip]{8545fig1.ps}\hspace{5mm} ... ...g5.ps}\hspace{5mm} \includegraphics[width=5.4cm,clip]{8545fig6.ps} \end{figure}$	Figure 1: Optical/NIR data coverage for DEEP1a ( top) and DEEP1b ( bottom). From left to right coverage in the K-band (shallow and deep strategies) and J-band (deep strategy only).
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$\begin{figure} \par\includegraphics[width=6.6cm,clip]{8545fig7.ps}\par\vspace{8mm} \includegraphics[width=6.6cm,clip]{8545fig8.ps}\end{figure}$	Figure 2: U-B vs. B-V colour diagram for stars in field DEEP1b. No correction applied ( top), correction $U_{\rm corr}=-0.15$ applied ( bottom). Green points refer to DPS stars, black dots to modelled stars.
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$\begin{figure} \par\includegraphics[width=6.6cm,clip]{8545fig9.ps}\par\vspace{8mm} \includegraphics[width=6.6cm,clip]{8545fg10.ps}\end{figure}$	Figure 3: Optical vs. infrared colour-colour diagram for stars in DEEP1b: V-R vs. R-J ( top) and V-R vs. $R-K_{\rm s}$ ( bottom). Green points refer to DPS stars, black dots to modelled stars.
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$\begin{figure} \par\includegraphics[width=7.7cm,clip]{8545fg12.ps}\end{figure}$	Figure 5: Galaxy photometric redshift distribution for field DEEP1b.
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$\begin{figure} \par\includegraphics[width=7.1cm,clip]{8545fg13.ps}\end{figure}$	Figure 6: LR values vs. radio-optical offsets for the 85 radio sources located in DEEP1a, b and c. The horizontal solid line indicate the LR value $L_{\rm th}=0.3$ , above which counterparts are considered as good identifications (see text for details).
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$\begin{figure} \par\includegraphics[height=5.5cm,width=5.5cm,clip]{8545fg14.ps}\... ...{2.5mm} \includegraphics[height=5.5cm,width=5.5cm,clip]{8545fg16.ps}\end{figure}$	Figure 7: The three extended radio sources included a posteriori in the identification sample: two with double radio morphology, ATESP5 J225034-401936 ( left panel) and ATESP5 J225426-402442 ( middle panel); and one wide angle tail source, ATESP5 J225505-401301 ( right panel). Grayscale: optical image in the reference band (R for DEEP1a and I for DEEP1b). Contours: 5 GHz flux density.
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$\begin{figure} \par\includegraphics[height=5.5cm,width=5.5cm,clip]{8545fg17.ps}\... ...{2.5mm} \includegraphics[height=5.5cm,width=5.5cm,clip]{8545fg19.ps}\end{figure}$	Figure 8: The three sources identified in bands other than the reference one: ATESP5 J224827-402515 ( left panel), identified in I-band; ATESP5 J225443-401147 ( middle panel), identified in $K_{\rm s}$ -band; and ATESP5 J225511-401513 ( right panel), identified in J-band. Grey scale: optical or NIR image. Contours: 5 GHz flux density.
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$\begin{figure} \par\includegraphics[width=6.9cm,clip]{8545fg20.ps}\end{figure}$	Figure 9: Redshift distribution for the 56 radio sources in the ATESP-DEEP1 sample with photometric redshift determination. The sample is divided into four different classes. From top to bottom: AGNs, ETS, LTS, and star-burst galaxies.
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$\begin{figure} \par\includegraphics[width=6.9cm,clip]{8545fg21.ps}\end{figure}$	Figure 10: 1.4 GHz radio power distribution for the 56 ATESP-DEEP1 radio sources with photometric redshift determination. The sample is divided into four different classes. From top to bottom: AGNs, ETS, LTS and star-burst galaxies. Light shading indicates two upper limits.
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$\begin{figure} \par\includegraphics[width=6.9cm,clip]{8545fg22.ps}\end{figure}$	Figure 11: Absolute B-band magnitude distribution. The sample is divided into four different classes. From top to bottom: AGNs, ETS, LTS and star-burst galaxies.
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$\begin{figure} \par\includegraphics[width=6.9cm,clip]{8545fg23.ps}\end{figure}$	Figure 12: Absolute R-band magnitude distribution. The sample is divided into four different classes. From top to bottom: AGNs, ETS, LTS and star-burst galaxies.
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