Table 5
Size of high-z simulated LARS galaxies.
| Continuum | rP20ell | σrP20ell | rP20minA | σrP20minA | r50 | σ r50 |
| kpc | kpc | kpc | kpc | kpc | kpc | |
| line | ξ(rP20ell) | σξ(rP20ell) | ξ(rP20minA) | σξ(rP20minA) | ξ(r50) | σξ(r50) |
|
|
||||||
| Bond2010(z ~ 3.1) | ||||||
| Rest-UVF606W | 1.3 | |||||
| LyαF502N | ~1 | |||||
| Finkelstein2011(z ~ 4.5) | ||||||
| Rest-UVF775W_1 | 0.67 |
|||||
| LyαF658N_1 | 1.1 |
|||||
| Rest-UVF775W_2 | 1.07  |
|||||
| LyαF658N_2 | 1.3  |
|||||
| Rest-UVF775W_3 | 0.67  |
|||||
| LyαF658N_3 | 2.0  |
|||||
|
|
||||||
| L01 | ||||||
| Rest-UV | ||||||
| 30 | 2.58 | 0.20 | 1.33 | 0.33 | 1.17 | 0.17 |
| 29 | 2.16 | 0.41 | 1.32 | 0.34 | 1.08 | 0.19 |
| 28 | 1.83 | 0.47 | 1.32 | 0.50 | 0.94 | 0.26 |
| Rest-optical | ||||||
| 29 | 4.38 | 0.20 | 3.18 | 0.37 | 2.00 | 0.17 |
| 28 | 4.51 | 0.29 | 3.19 | 0.46 | 2.01 | 0.17 |
| 27 | 4.37 | 0.49 | 3.17 | 0.80 | 1.98 | 0.20 |
| 26 | 4.25 | 0.87 | 3.35 | 1.42 | 1.88 | 0.28 |
| Lyα | ||||||
| 5E-19 | 2.20 | 0.22 | 2.57 | 0.37 | 1.82 | 0.28 |
| 3E-18 | 2.08 | 0.28 | 2.05 | 0.59 | 1.73 | 0.21 |
| 8E-18 | 1.78 | 0.52 | 1.74 | 0.89 | 1.59 | 0.39 |
| Hα | ||||||
| 2E-19 | 0.47 | 0.04 | 0.37 | 0.12 | 0.53 | 0.09 |
| 6E-19 | 0.49 | 0.05 | 0.34 | 0.11 | 0.57 | 0.09 |
| 1E-18 | 0.48 | 0.05 | 0.35 | 0.12 | 0.54 | 0.09 |
| 3E-18 | 0.45 | 0.06 | 0.35 | 0.12 | 0.51 | 0.10 |
|
|
||||||
| L02 | ||||||
| Rest-UV | ||||||
| 30 | 3.57 | 1.42 | 1.86 | 0.45 | 2.10 | 0.91 |
| 29 | 3.53 | 1.39 | 2.54 | 1.43 | 2.09 | 0.92 |
| Rest-optical | ||||||
| 29 | 10.62 | 0.89 | 8.82 | 1.45 | 4.16 | 0.25 |
| 28 | 9.76 | 1.48 | 6.89 | 2.02 | 4.08 | 0.40 |
| 27 | 7.07 | 2.30 | 5.34 | 2.38 | 3.48 | 0.71 |
| Lyα | ||||||
| 5E-19 | 3.12 | 0.31 | 2.43 | 0.63 | 2.53 | 0.16 |
| 3E-18 | 2.63 | 0.39 | 1.72 | 0.68 | 2.40 | 0.41 |
| 8E-18 | 1.77 | 0.80 | 1.24 | 0.57 | 1.71 | 0.71 |
| Hα | ||||||
| 2E-19 | 0.16 | 0.09 | 0.13 | 0.05 | 0.20 | 0.14 |
| 6E-19 | 0.23 | 0.03 | 0.23 | 0.04 | 0.33 | 0.04 |
| 1E-18 | 0.24 | 0.04 | 0.23 | 0.05 | 0.34 | 0.05 |
Notes. Sizes in the continuum are reported as rP20ell. Owing pixel re-sampling, the Petrosian radius can have a variation of 20% with respect to the value estimated in the original image. The Lyα effective radii of two existent individual-source measurements are also shown (Bond et al. 2010; Finkelstein et al. 2011b).
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