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Table 3

Different values of f obtained from literature.

Author f z range Sample Method

Calzetti et al. (2000) 0.44 (0.58) 0.0030.05 starburst galaxies Balmer decrement
Kashino et al. (2013) 0.83 ± 0.10 1.41.7 sBzk galaxies Balmer decrement (stacked spectra)
" 0.69 ± 0.02 " " Hα to UV SFRs
Wuyts et al. (2011) 0.44 03 Ks selected galaxies SFR indicators
Price et al. (2014) 0.55 ± 0.16 1.361.5 MS star forming galaxies Balmer decrement (stacked spectra)
Pannella et al. (2015) 0.58 <1 UVJ selected galaxies comparison between AUVM/AHαM
" 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 1.52.6 Lyman Break Galaxies matching X-ray, UV and Hα SFRs
This work 0.93 ± 0.06 0.71.5 far-IR selected galaxies Hα to UV SFRs

Notes. Table also specifies the redshift ranges (third column of Table 3), the types of sample, and the methods implied to measure the differential extinction on nebular lines (fourth and fifth columns of Table 3, respectively).

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