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 . 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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