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Table 3
Different values of f obtained from literature.
| Author | f | z range | Sample | Method |
|
|
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| Calzetti et al. (2000) | 0.44 (0.58) | 0.003−0.05 | starburst galaxies | Balmer decrement |
| Kashino et al. (2013) | 0.83 ± 0.10 | 1.4−1.7 | sBzk galaxies | Balmer decrement (stacked spectra) |
| " | 0.69 ± 0.02 | " | " | Hα to UV SFRs |
| Wuyts et al. (2011) | 0.44 | 0−3 | Ks selected galaxies | SFR indicators |
| Price et al. (2014) | 0.55 ± 0.16 | 1.36−1.5 | MS star forming galaxies | Balmer decrement (stacked spectra) |
| Pannella et al. (2015) | 0.58 | <1 | UVJ selected galaxies | comparison between AUV−M⋆/AHα−M⋆ |
| " | 0.77 | 1 | " | " |
| " | 1 | >1 | " | " |
| Valentino et al. (2015) | 0.74 ± 0.05 | 2 | CL J1449+0856 | Balmer decrement (stacked spectra) |
| Erb et al. (2006) | 1 | 2 | rest-frame UV selected galaxies | matching UV and Hα SFRs |
| Reddy et al. (2010) | 1 | 1.5−2.6 | Lyman Break Galaxies | matching X-ray, UV and Hα SFRs |
| This work | 0.93 ± 0.06 | 0.7−1.5 | far-IR selected galaxies | Hα to UV SFRs |
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