Table 2
Schechter parameters M* and α of field LF and CLFs from the literature.
| Reference | Gal. type | Radius | Method | Nclus | Ssample | z | M* | α |
|---|---|---|---|---|---|---|---|---|
| Blanton et al. (2001) | All | field | spec | SDSS | z < 0.2 | −21.6±0.03 | −1.20±0.03 | |
| Goto et al. (2002) | All | 0.75 Mpc | phot | 204 | SDSS CE | 0.02 < z < 0.25 | −22.21±0.05 | −0.85±0.03 |
| Goto et al. (2002) | All | 0.75 Mpc | spec | 75 | SDSS CE | 0.02 < z < 0.25 | −22.31±0.13 | −0.88±0.07 |
| Popesso et al. (2006)a,b | All | r500 | phot | 69 | RASS+SDSS | ⟨ z⟩ = 0.1 | −20.84±0.13 | −1.05±0.07 |
| Popesso et al. (2006)a,c | All | r500 | phot | 69 | RASS+SDSS | ⟨ z⟩ = 0.1 | −21.16±0.26 | −1.26±0.12 |
| Rudnick et al. (2009) | RS | 0.75 Mpc | colour | 167 | SDSS | z < 0.06 | −21.21±0.24 | −0.78±0.08 |
| Rudnick et al. (2009) | RS | 0.75 Mpc | colour | 16 | EDisCS | 0.4 < z < 0.8 | −21.51 |
−0.36 |
| Martinet et al. (2015) | RS | 1 Mpc | photo-z+colour | 16 | DAFT/FADA | ⟨ z⟩ = 0.58 | −22.4±0.2 | −0.80±0.14 |
| Martinet et al. (2015) | BC | 1 Mpc | photo-z+colour | 6 | DAFT/FADA | ⟨ z⟩ = 0.62 | −22.4±0.5 | −1.32±0.36 |
Notes. (a)These values were obtained using h0 = 1; we converted them to our cosmology in Fig. 10, (b)These values correspond to the bright part of a LF fitted using a double Schechter function (dS), (c)These values correspond to the bright part of a LF fitted using a Schechter plus an exponential function (S+e).
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