Table 1.
Observed and derived properties of currently available z > 10 spectroscopically confirmed super-Eddington galaxies.
| Measured |
ID# | Derived |
|||||||||||
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| z | β | log M⋆ | SFR | sSFR | log ξion | v∞ | fesc | Rb | vp | FWHM | EW | fα | |
| M⊙ | M⊙ yr−1 | Gyr−1 | erg−1 Hz | km s−1 | pMpc | km s−1 | km s−1 | Å | |||||
| 10.60 | −2.40 | 8.70 | 15.7 | 31.3 | 25.70 | GN-z11 | 200 | 0.03 | 0.21 | 555 | 516 | 18.7 | 0.069 |
| 11.40 | −2.32 | 7.78 | 4.2 | 69.7 | 25.70 (a) | Maisie | 124 | 0.02 | 0.11 | 516 | 384 | 7.6 | 0.028 |
| 10.38 | −2.49 | 7.58 | 1.1 | 28.9 | 25.46 | GS-z10-0 | 65 | 0.04 | 0.08 | 490 | 335 | 4.0 | 0.026 |
| 10.17 | −2.60 | 8.10 | 5.1 | 40.5 | 25.20 | MACS0647-JD | 129 | 0.05 | 0.13 | 503 | 387 | 3.4 | 0.040 |
| 12.20 | −3.00 | 8.08 | 10.1 | 84.0 | 25.70 (a) | GHZ2 | 182 | 0.16 | 0.26 | 529 | 503 | 17.6 | 0.065 |
Notes. The photometric candidate GHZ2 is also included. Columns (1)–(6) contain the observed properties of the galaxies taken from Bunker et al. (2023), Arrabal Haro et al. (2023b), Curtis-Lake et al. (2023), Hsiao et al. (2022, 2023), Castellano et al. (2022), Harikane et al. (2023a); Cols. (8)–(10) give the outflow terminal velocity, LyC escape fraction, and H II bubble radius, respectively; Cols. (11)–(14) give the model predictions for the observed Lyα line peak velocity shift, FWHM, EW, and escape fraction, respectively; they are computed for the same outflow H I column density, log NHI = 21.1, fitting the observed GN-z11 line profile for each galaxy.
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