Table 3
Derived quantities.
| Source | M1500 | log (LUV) | SFR(UV) | log (M⋆(UV)) | β | A UV | SFR(IR) | ||||||
| [mag] | [L⊙] | [M⊙ yr-1] | [M⊙] | [mag] | [M⊙ yr-1] | ||||||||
|
|
|||||||||||||
| A1703-zD1 | –20.3 | 10.45 | 9.0 | 9.2 ± 0.3 | –1.4 | < 1.2 ± 0.4 | < 13.8 | ||||||
| z8-GND-5296 | –21.4 | 10.86 | 23.4 | 9.7 ± 0.3 | –1.4 |
|
< 113 | ||||||
| IOK-1 | –21.3 | 10.8 | 20.4 | 9.7 ± 0.3 | –2.0 |
|
< 16.3 | ||||||
| HCM6A | –20.8 | 10.63 | 13.7 | 9.5 ± 0.3 | –1.7 | < 1.3 ± 0.4 | < 24.5 | ||||||
| Himiko | –21.7 | 11.0 | 32.3 | 9.8 ± 0.3 | –2.0 |
|
< 11.4 | ||||||
Notes. For A1703-zD1 we have assumed a magnification factor of μ = 9, for HCM6A μ = 4.5. The upper limits on the UV attenuation and SFR(IR) are derived from LIR(Td = 35) and using Eq. (1). The SFR values (limit) listed here assume constant SF, ages ≳ 100 Myr, and the Kennicutt (1998) calibration. SFR(UV) is not corrected for reddening. Typical uncertainties for the UV slope β are ± (0.3 − 0.5) (cf. Sect. 4.1).
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