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Table 2.
List of the galaxies, the kernel sizes used to smooth their maps, and the Lyα SB used for determining the faintest encompassing isophote in our morphological studies.
| ID | Kernel size | Lyα SB |
|---|---|---|
| (Physical scale) | (1039 erg s−1 kpc−2) | |
| LARS01-10 | 0.3 kpc | 1.5 |
| LARS11-14 | 0.8 kpc | 1.5 |
| ELARS01-28 | 0.3 kpc | 1.5 |
| Tol1214 | 0.3 kpc | 1.5 |
| Tol1247 | 0.3 kpc | 1.5 |
| J1156 | 0.8 kpc | 5.0 |
Notes. The kernel sizes are chosen differently based on the redshift of the galaxies.
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