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Table 2.

Results from our two-dimensional exponential fitting procedure (Sect. 3.3).

ID rsMg II rscont@Mg II rs[O II] rsCont@[O II] ΔMg II−[O II] Δ[Mg II]−cont Δ[O II]−cont
[kpc] [kpc] [kpc] [kpc] [kpc] [kpc] [kpc]
J0047+0154 2.47 ± 0.06h < 0.8 1.99 ± 0.01h < 0.6 2.5 ± 0.1o 2.8 ± 0.1o 0.30 ± 0.05o
J0130-0014 < 0.4 < 0.5 1.09 ± 0.14o
J0141-0304 0.56 ± 0.02 0.61 ± 0.06 < 0.6 0.60 ± 0.03 0.01 ± 0.03 0.14 ± 0.07 0.21 ± 0.03o
J0804+4726* < 1.2 < 1.2 2.16 ± 0.49o
J0811+4141 1.40 ± 0.25 3.60 ± 0.26 1.22 ± 0.02h < 1.0 1.36 ± 0.27o 0.92 ± 0.53 0.69 ± 0.07o
J0834+4805 2.27 ± 0.29 2.84 ± 0.11 1.79 ± 0.01h < 0.8 1.27 ± 0.25o 1.59 ± 0.39o 0.12 ± 0.02o
J0844+5312 1.05 ± 0.05h 0.59 ± 0.13 1.05 ± 0.01h 0.96 ± 0.06 0.29 ± 0.13o 0.22 ± 0.07o
J0912+5050 1.28 ± 0.22 2.68 ± 0.15 1.67 ± 0.01h < 0.8 1.76 ± 0.19o 1.68 ± 0.34o 0.43 ± 0.02o
J0919+4906 < 1.3 1.76 ± 1.55 < 0.8 < 1.6 2.25 ± 0.19o 3.5 ± 1.5 1.73 ± 0.67
J0940+5932 < 1.5 < 1.3 1.97 ± 0.02h < 0.9 2.18 ± 0.79 2.0 ± 0.84 0.4 ± 0.03o
J1014+5501 2.90 ± 0.21h 2.35 ± 0.17 1.47 ± 0.01 2.21 ± 0.13 0.96 ± 0.28o 1.08 ± 0.45 0.33 ± 0.13
J1033+6353* 2.03 ± 0.08h 1.72 ± 0.07 1.83 ± 0.01h < 1.2 0.47 ± 0.09o 0.75 ± 0.14o 0.09 ± 0.02o
J1046+5827 1.21 ± 0.05h 0.85 ± 0.05 0.74 ± 0.01h 0.68 ± 0.04 0.53 ± 0.05o 0.36 ± 0.09o 0.31 ± 0.04o
J1137+3605 < 0.4 0.94 ± 0.07 < 0.4 0.88 ± 0.03 0.39 ± 0.08o 0.84 ± 0.12o 0.31 ± 0.03o
J1154+2443* < 0.4 < 0.5 < 0.5 < 0.4 0.07 ± 0.02o 0.08 ± 0.02o 0.01 ± 0.01
J1157+5801 0.43 ± 0.25 < 1.2 0.56 ± 0.01 0.77 ± 0.07 1.02 ± 0.37 1.71 ± 0.58 0.85 ± 0.09o
J1243+4646* < 0.3 < 0.3 < 0.5 0.4 ± 0.1 0.08 ± 0.01o 0.13 ± 0.04 0.48 ± 0.01o
J1256+4509* < 0.4 < 0.5 < 0.5 < 0.3 0.11 ± 0.02o 0.03 ± 0.02 0.19 ± 0.06o
J1352+5617 1.27 ± 0.04 1.4 ± 0.1 0.93 ± 0.01 1.10 ± 0.06 0.28 ± 0.05o 0.38 ± 0.14 0.07 ± 0.06
J1503+3644 1.06 ± 0.03h 0.92 ± 0.05 0.20 ± 0.07
J1517+3705 2.06 ± 0.11h 1.35 ± 0.14 1.46 ± 0.01h < 1.0 0.39 ± 0.11o 0.54 ± 0.25 0.26 ± 0.04o
J1648+4957 2.26 ± 0.25 3.13 ± 0.32 2.01 ± 0.02h < 1.3 0.77 ± 0.28 2.1 ± 0.8 0.79 ± 0.08o

Notes. ID: source identifier. Objects identified with * are considered as strong LyC leakers following the criteria of Flury et al. (2022b): > 5σ detection and f esc LyC > 5 % $ f_{\mathrm{esc}}^{\mathrm{LyC}} > 5\% $. rsMg II([O II]): exponential scale length of the Mg II ([O II]) emission in physical kpc. The nebular emission scale lengths that are significantly more extended than the continuum are marked with h for “halo” (see Sect. 3.4). rscont@Mg II([O II]): exponential scale length of the continuum at Mg II ([O II]) wavelenghts in kpc. ΔMg II−[O II]: spatial offset between the Mg II and [O II] emission best-fit centroids in kpc. ΔMg II([O II])−cont: spatial offset between the Mg II ([O II]) emission and the continuum best-fit centroids in kpc. The significant offsets are marked with o (see Sect. 3.5).

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