CARS: The CFHTLS-Archive-Research Survey - III. First detection of cosmic magnification in samples of normal high-z galaxies

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Table 1:

Schechter (1976) function parameters for the external LFs.
Reference	M_*	$\alpha_{\rm LF}$ ^a
$z\sim3$
Steidel et al. (1999)	-21.00	-1.60
Sawicki & Thompson (2006)	-20.90	-1.43
Bouwens et al. (2007)^b	-20.98	-1.73
$z\sim4$
Steidel et al. (1999)	-21.20	-1.60
Sawicki & Thompson (2006)	-21.00	-1.26
Bouwens et al. (2007)	-20.98	-1.73
$z\sim5$
Steidel et al. (1999)^b	-21.20	-1.60^c
Sawicki & Thompson (2006)^b	-21.00	-1.26
Bouwens et al. (2007)	-20.64	-1.66

^a This $\alpha_{\rm LF}$ is the faint-end-slope of the Schechter LF. The $\alpha(m)$ introduced in Eq. (2) approaches this value for faint magnitudes; ^b extrapolated from $z\sim4$ ; ^c fixed.

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