Table 2.
Photometric results and fesc upper limits of the stacks.
| Group | Number | LyC | F606W | fesc |
|---|---|---|---|---|
| [AB mag] | [AB mag] | |||
| F275W stack | 26 | > 29.92 | 26.57 ± 0.004 | < 0.06 |
| F336W stack | 65 | > 31.39 | 27.56 ± 0.01 | < 0.04 |
| LAE stack | 13 | > 30.46 | 28.13 ± 0.02 | < 0.16 |
| O32 stack | 14 | > 29.96 | 26.52 ± 0.01 | < 0.06 |
Notes. The second column represents the number of galaxies we stacked in the process. The 2σ upper limit magnitudes for the stack of different subgroups are constrained by an aperture with 
to avoid the omission of flux due to the potential offsets. The fesc of the stacks are under the assumption of an average IGM transmission TIGM = 0.33, dust attenuation E(B − V) = 0.2, and L1500, intr/L900, intr = 3.
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