Table 1.
Properties of the simulated galaxy at three different times.
| Output | z | Rvir | Mh | Mgas | M* | Zgas | Z* | SFR | LyC fesc | M1500 | A1500 |
|---|---|---|---|---|---|---|---|---|---|---|---|
| [kpc] | [M⊙] | [M⊙] | [M⊙] | [Z⊙] | [Z⊙] | [M⊙ yr−1] | [%] | [mag] | [mag] | ||
| A | 3.2 | 27 | 5.09 × 1010 | 5.15 × 109 | 1.88 × 109 | 0.40 | 0.36 | 5.0 |
 |
 |
 |
| B | 3.1 | 28 | 5.30 × 1010 | 5.13 × 109 | 2.08 × 109 | 0.43 | 0.40 | 2.2 |
 |
 |
 |
| C | 3.0 | 29 | 5.56 × 1010 | 4.83 × 109 | 2.27 × 109 | 0.43 | 0.42 | 4.2 |
 |
 |
 |
Notes. All the masses are computed inside the virial radius and the metallicities in a sphere of a tenth of the virial radius. The SFR is averaged over the last 10 Myr. LyC fesc is the escape fraction of hydrogen ionizing photons computed at the virial radius (Sect. 2.6). M1500 is the absolute magnitude of the galaxy at 1500 Å, including dust attenuation. A1500 represents the attenuation by dust, following the equation: 
. The escape fractions, magnitudes, and attenuation by dust, which are the only three quantities depending on the direction of observation, were computed for 1728 isotropically distributed directions. We show the mean of the results and the 10th and 90th percentiles.
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