Table 1
Properties of the galaxies in my sample.
| Name | z | log (Mdust/M⊙) | log (Mstar/M⊙) | log (Mdyn/M⊙) | log (Mgas/M⊙) | Ref. | |||||||
| HFLS3 | 6.340 |
|
··· | ··· |
|
|
a
|
11.43 |
|
1 | |||
| ULASJ1120+0641 | 7.085 |
|
|
|
··· | ··· | ··· | 11.00 |
b
|
2, 3 | |||
| A1689-zD1 | 7.500 |
|
|
|
|
|
|
··· | ··· | 4 | |||
|
|
|||||||||||||
| HCM6A | 6.560 | < 7.44 | ··· | ··· |
|
··· | ··· | ··· | ··· | 5, 6 | |||
| Himiko | 6.595 | < 6.94 | ··· | ··· |
|
|
··· | ··· | ··· | 7, 8, 9 | |||
| A1703-zD1 | 6.800 | < 7.19 | ··· | ··· |
|
··· | ··· | ··· | ··· | 10, 6 | |||
| IOK-1 | 6.960 | < 7.27 | ··· | ··· |
|
··· | ··· | ··· | ··· | 11, 6 | |||
| z8-GND-5296 | 7.508 | < 8.11 | ··· | ··· |
|
··· | ··· | ··· | ··· | 12, 6 | |||
Notes. Unless noted otherwise the values are from the references listed in the last column. Stellar masses are listed for the Chabrier (2003) IMF.
I calculated the stellar mass from the photometry (Riechers et al. 2013) using the Grasil code.
I calculated the gas mass from the LCII luminosity (Venemans et al. 2012) using the empirical calibration of Swinbank et al. (2012): Mgas = (10 ± 2)(LCII/L⊙).
Reference. 1) Riechers et al. (2013); 2) Mortlock et al. (2011); 3) Venemans et al. (2012); 4) Watson et al. (2015); 5) Hu et al. (2002); 6) Schaerer et al. (2015); 7) Ouchi et al. (2009); 8) Hirashita et al. (2014); 9) Ouchi et al. (2013); 10) Bradley et al. (2012); 11) Iye et al. (2006); 12) Finkelstein et al. (2013).
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