Pixel-level, spatially resolved physical properties of the target system: stellar mass (log M_*; panel a), SFR (panel b), mass-weighted stellar age (${⟨a⟩}_{\ast }^{\mathrm{m}}$; panel c), ionization parameter (log U; panel d), V-band attenuation (A_V; panel e), slope (S; panel f) and UV bump (B; panel g) of the dust attenuation curve, sSFR (panel h), and Lyα flux (f_Lyα; panel i). The quantities log M_*, SFR, and f_Lyα are corrected for lensing magnification. The three adjacent NIRSpec slits are overlaid as cyan rectangles. The NIRCam RGB map is shown as white contours at the 5σ and 10σ levels, while the Lyα emission is traced by magenta contours at 1−2σ.