Table B.1.
Application to high redshift UV-continuum and Lyα selected LAEs (see compilation by Matthee et al. 2017b).
| Name | z | log10(LLyα) | EW0 | MUV | βUV | SFR
|
SFR
|
SFRLyα | Reference |
|---|---|---|---|---|---|---|---|---|---|
| (UV selected) | (erg s−1) | (Å) | (mag) | (M⊙ yr−1) | (M⊙ yr−1) | (M⊙ yr−1) | |||
| A383-5.2 | 6.03 | 42.8 | 138 | −19.3 | βf |  |
 |
 |
Stark et al. (2015a) |
| RXCJ22-ID3 | 6.11 | 42.5 | 40 | −20.1 | −2.3 ± 0.2 |  |
 |
 |
Mainali et al. (2017) |
| RXCJ22-4431 | 6.11 | 42.9 | 68 | −20.2 | −2.3 ± 0.2 |  |
 |
 |
Schmidt et al. (2017) |
| SDF-46975 | 6.84 | 43.2 | 43 | −21.5 | βf |  |
 |
 |
Ono et al. (2012) |
| IOK-1 | 6.96 | 43.0 | 42 | −21.3 | −2.0 ± 0.3 |  |
 |
 |
Ono et al. (2012) |
| BDF-521 | 7.01 | 43.0 | 64 | −20.6 | −2.3 ± 0.4 |  |
 |
 |
Cai et al. (2015) |
| A1703 zd6 | 7.04 | 42.5 | 65 | −19.3 | −2.4 ± 0.2 |  |
 |
 |
Stark et al. (2015b) |
| BDF-3299 | 7.11 | 42.8 | 50 | −20.6 | −2.0 ± 0.5 |  |
 |
 |
Vanzella et al. (2011) |
| GLASS-stack | 7.20 | 43.0 | 210 | −19.7 | βf |  |
 |
 |
Smidt et al. (2016) |
| EGS-zs8-2 | 7.48 | 42.7 | 9 | −21.9 | −1.8 ± 0.4 |  |
 |
 |
Stark et al. (2015a) |
| FIGSGN1-1292 | 7.51 | 42.8 | 49 | −21.2 | βf |  |
 |
 |
Tilvi et al. (2016) |
| GN-108036 | 7.21 | 43.2 | 33 | −21.8 | βf |  |
 |
 |
Stark et al. (2015a) |
| EGS-zs8-1 | 7.73 | 43.1 | 21 | −22.1 | −1.7 ± 0.1 |  |
 |
 |
Oesch et al. (2015) |
| (Lyα selected) | |||||||||
| SR6a | 5.68 | 43.4 | 210 | −21.1 | −1.8 ± 0.4 |  |
 |
 |
Matthee et al. (2017b) |
| Ding-3 | 5.69 | 42.8 | 62 | −20.9 | βg |  |
 |
 |
Ding et al. (2017) |
| Ding-4 | 5.69 | 42.3 | 106 | −20.5 | βg |  |
 |
 |
Ding et al. (2017) |
| Ding-5 | 5.69 | 43.2 | 79 | −21.0 | βg |  |
 |
 |
Ouchi et al. (2008) |
| Ding-1 | 5.70 | 43.0 | 21 | −22.2 | βg |  |
 |
 |
Ding et al. (2017) |
| J233454b | 5.73 | 43.7 | 210 | −21.5 | βg |  |
 |
 |
Shibuya et al. (2018) |
| J021835 | 5.76 | 43.7 | 107 | −21.7 | βg |  |
 |
 |
Shibuya et al. (2018) |
| VR7a | 6.53 | 43.4 | 35 | −22.5 | −2.0 ± 0.3 |  |
 |
 |
Matthee et al. (2017b) |
| J162126b | 6.55 | 43.9 | 99 | −22.8 | βg |  |
 |
 |
Shibuya et al. (2018) |
| J160234 | 6.58 | 43.5 | 81 | −21.9 | βg |  |
 |
 |
Shibuya et al. (2018) |
| Himikoc | 6.59 | 43.6 | 65 | −22.1 | −2.0 ± 0.4 |  |
 |
 |
Ouchi et al. (2009) |
| COLA1 | 6.59 | 43.6 | 120 | −21.6 | βg |  |
 |
 |
Matthee et al. (2018) |
| CR7d | 6.60 | 43.9 | 211 | −22.2 | −2.3 ± 0.3 |  |
 |
 |
Sobral et al. (2015) |
Notes. Errors on Lyα luminosity and EW0 are assumed to be ≈0.1 dex, while errors on MUV are taken as ≈0.2 dex. We compute the UV SFRs (SFRUV, dust corrected) using Kennicutt (1998) and β values, individually measured when available, or β = −1.6 ± 0.2 for UV-selected and β = −1.9 ± 0.2 for Lyα selected sources when not available. Furthermore, we also compute dust corrected UV SFRs by using β = −1.6 ± 0.2 for all sources (SFR
). Lyα SFRs (SFRLyα; calibrated to be dust-corrected) are computed with our Eq. (8). (a)EW0 have been recomputed and rest-framed when compared to original reference. (b)MUV have been recomputed when compared to original reference. (c)Values used are from Zabl et al. (2015). (d)Computed as in Matthee et al. (2017c). (e)COLA1’s discovery is reported in Hu et al. (2016); here we use the latest measurements from Matthee et al. (2018). (f)β values not available; calculated assuming β = −1.6 ± 0.2. (g)β values not available; calculated assuming β = −1.9 ± 0.2. This table is also provided in FITS format.
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