Table 2.
UV radius, observed and intrinsic C III] line emission flux, C III] intrinsic luminosity, and surface brightness of the full galaxy sample.
| ID | rUV |
 |
 |
 |
 |
Ref. |
|---|---|---|---|---|---|---|
| (kpc) | (10−18 erg s−1 cm−2) | (10−18 erg s−1 cm−2) | (108 L⊙) | (108 L⊙ kpc−2) | ||
| New C III] data on galaxies at 5.5 < z < 7 | ||||||
| HZ10 | 1.1 (a) | 36.7 ± 11.1 |
 |
 |
8.1 ± 4.1 | [1, †] |
| HZ1 | 1.2 | < 8.7 | < 8.7 | < 8.4 | < 0.9 | [1, †] |
| RXJ 1347−1216 | 0.8 | < 5.2 | < 5.2 | < 7.5 | < 1.8 | [2, †] |
| GDS3073 | 0.11 ± 0.01 | < 2.6 | < 2.6 | < 2.4 | < 31.6 | [3, †] |
| UVISTA-Z-002 | 2.1 ± 0.1 (b) | < 1.5 | < 1.5 | < 2.0 | < 0.3 | [†] |
| New C III] data on galaxies at z ∼ 2 | ||||||
| 9347 | 3.08 ± 0.07 | < 336.2 | < 336.2 | < 22.1 | < 0.4 | [†] |
| 6515 | 2.2 ± 0.4 | < 605.9 | < 605.9 | < 39.4 | < 1.3 | [†] |
| 10076 | 2.35 ± 0.03 | < 1430.4 | < 1430.4 | < 106.2 | < 3.1 | [†] |
| 9834 | 0.97 ± 0.02 | < 2115.6 | < 2115.6 | < 123.6 | < 20.9 | [†] |
| 9681 | 1.93 ± 0.03 | < 1088.9 | < 1088.9 | < 74.8 | < 3.2 | [†] |
| 8490 | 1.6 ± 0.01 | < 536.0 | < 536.0 | < 37.8 | < 2.4 | [†] |
| Literature sample of galaxies at 6 < z < 7.5 | ||||||
| COS-3018 | 1.3 ± 0.1 (b) | 1.3 ± 0.3 | 8.5 ± 6.8 | 12.6 ± 10.2 | 1.3 ± 1.0 | [4, 6] |
| A383-5.2 | 0.9 | 3.7 ± 1.1 | 5.6 ± 1.9 | 6.2 ± 2.1 | 1.1 ± 0.6 | [1, 7] |
| z7_GND_42912 | 0.72 ± 0.01 | 2.6 ± 0.5 | 12.0 ± 5.7 | 2.2 ± 1.1 | 6.8 ± 3.2 | [†, 8] |
| Himiko | 0.9 (a) | < 5.8 | < 5.8 | < 7.9 | < 1.6 | [1, 9] |
| CR7 | 0.9 (a) | < 17.0 | < 17.0 | < 23.1 | < 4.6 | [1, 10] |
| CR7a | 0.9 | < 15.0 | < 15.0 | < 20.4 | < 4.0 | [1, 10] |
| CR7b | 0.9 | < 13.0 | < 13.0 | < 18.0 | < 3.5 | [1, 10] |
| CR7c | 0.9 | < 14.0 | < 14.0 | < 19.1 | < 3.7 | [1, 10] |
| COS-13679 | 0.8 | < 0.8 | < 0.8 | < 1.4 | < 0.4 | [1, 6] |
| COS-2987 | 1.6 ± 0.5 (b) | < 1.6 | < 1.6 | < 2.3 | < 0.2 | [4, 6] |
| VR7 | 1.6 ± 0.1 | < 21.0 | < 21.0 | < 27.9 | < 1.8 | [5, 11] |
Notes. We assume 20% uncertainties on the rUV when they are not provided.
References. Redshift, rUV, and C III] flux references: [†] This work, [1] Carniani et al. (2018a), [2] Bradač et al. (2017), [3] Vanzella et al. (2010), [4] Smit et al. (2018), [5] Matthee et al. (2019), [6] Laporte et al. (2017), [7] Stark et al. (2015), [8] Hutchison et al. (2019), [9] Zabl et al. (2015), [10] Sobral et al. (2018), [11] Matthee et al. (2017b).
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