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Table 3
Schechter coefficients of the luminosity function of star-forming galaxies at z ~ 3.
| LF | M ∗ | Φ∗ | α | Reference | Notes |
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| 01 | –20.71 | 0.00055 | –1.94 | Alavi et al. (2016) | LF at 2.2 <z< 3.0 1500 Å rest frame |
| 02 | –20.20 | 0.00532 | –1.31 | Parsa et al. (2016) | LF at z = 2.8 1500 Å rest frame |
| 03 | –20.71 | 0.00206 | –1.43 | Parsa et al. (2016) | LF at z = 3.8 1500 Å rest frame |
| 04 | –20.61 | 0.00161 | –1.54 | Parsa et al. (2016) | best fit at z = 3.3 1500 Å rest frame |
| 05 | –20.45 | 0.00410 | –1.36 | Weisz et al. (2014) | LF z = 3.0 1500 Å rest frame |
| 06 | –21.40 | 0.00086 | –1.50 | Cucciati et al. (2012) | 1500 Å rest frame |
| 07 | –20.94 | 0.00179 | –1.65 | van der Burg et al. (2010) | z = 3.0 1600 Å rest frame |
| 08 | –20.97 | 0.00171 | –1.73 | Reddy & Steidel (2009) | z = 3.05 1700 Å rest frame |
| 09 | –20.90 | 0.00167 | –1.43 | Sawicki & Thompson (2006) | z = 3.0 1700 Å rest frame |
Notes. Cucciati et al. (2012) did not actually measure the faint end slope at z> 1.7, but fixed this value based on luminosity functions at lower redshifts.
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