Fig. 8.
Continuum emitter found in the J2228$+$0152 field (${13{^{\prime \prime}_{.}}7}$ away from the phase reference position). The contours are $-$3 $\sigma$, $-$2 $\sigma$, 2 $\sigma$, 3 $\sigma$, 4 $\sigma$, 5 $\sigma$, 10 $\sigma$, 15 $\sigma$, and 20 $\sigma$, with 1 $\sigma$ = 11.2 μJy beam$^{-1}$. The emission is spatially resolved with a peak flux of 0.25 mJy beam$^{-1}$, and the area-integrated flux is $0.38 \pm 0.05$ mJy, respectively. The photometric redshift predicted for this object is $z_{\rm photo} = 2.26 \pm 0.56$

Continuum emitter found in the J2228|$+$|0152 field (⁠|${13{^{\prime \prime}_{.}}7}$| away from the phase reference position). The contours are |$-$|3 |$\sigma$|⁠, |$-$|2 |$\sigma$|⁠, 2 |$\sigma$|⁠, 3 |$\sigma$|⁠, 4 |$\sigma$|⁠, 5 |$\sigma$|⁠, 10 |$\sigma$|⁠, 15 |$\sigma$|⁠, and 20 |$\sigma$|⁠, with 1 |$\sigma$| = 11.2 μJy beam|$^{-1}$|⁠. The emission is spatially resolved with a peak flux of 0.25 mJy beam|$^{-1}$|⁠, and the area-integrated flux is |$0.38 \pm 0.05$| mJy, respectively. The photometric redshift predicted for this object is |$z_{\rm photo} = 2.26 \pm 0.56$|

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