High redshift galaxies in the ALHAMBRA survey - II. Strengthening the evidence of bright-end excess in UV luminosity functions at 2.5 ≤ z≤ 4.5 by PDF analysis

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Table C.1

Compilation of literature data for UV LF parameters and the corresponding luminosity densities calculated by us.

Reference	Z			α	log(LD) [W Hz⁻¹ Mpc⁻³]
Wyder et al. (2005)	0.05				18.56
Cucciati et al. (2012)	0.125	−18.12			18.74
Cucciati et al. (2012)	0.300				18.85
Cucciati et al. (2012)	0.500				18.84
Gabasch et al. (2004)	0.63			− 1.07	18.97
Cucciati et al. (2012)	0.700		9.53		18.92
Oesch et al. (2010)	0.75				19.05
Cucciati et al. (2012)	0.9				19.04
Gabasch et al. (2004)	0.96			− 1.07	19.21
Cucciati et al. (2012)	1.100				19.09
Oesch et al. (2010)	1.25				19.49
Gabasch et al. (2004)	1.36			− 1.07	19.20
Cucciati et al. (2012)	1.45				19.12
Oesch et al. (2010)	1.5				19.14
Sawicki & Thompson (2006)	1.7				19.75
Parsa et al. (2016)	1.7				19.44
Oesch et al. (2010)	1.75				19.42
Gabasch et al. (2004)	1.88			− 1.07	19.16
Oesch et al. (2010)	1.9				19.39
Parsa et al. (2016)	1.9				19.48
Cucciati et al. (2012)	2.1			− 1.30	19.44
Sawicki & Thompson (2006)	2.2				19.42
Parsa et al. (2016)	2.25				19.50
Parsa et al. (2016)	2.25				19.54
Oesch et al. (2010)	2.50				19.94
Gabasch et al. (2004)	2.53			− 1.07	19.41
Parsa et al. (2016)	2.8				19.56
Sawicki & Thompson (2006)	3.0				19.42
Cucciati et al. (2012)	3.0			− 1.50	19.38
Bouwens et al. (2015)	3.0				19.78
This work	3.0	− 21.62 ± 0.11	0.51 ± 0.07	− 1.53 ± 0.15
Gabasch et al. (2004)	3.46			− 1.07	19.31
Paltani et al. (2007)	3.5			− 1.4	19.50
Bouwens et al. (2007)	3.8				19.67
Bouwens et al. (2015)	3.8				19.68
Bouwens et al. (2015)	3.8				19.68
Parsa et al. (2016)	3.8				19.43
Sawicki & Thompson (2006)	4.0				19.06
Cucciati et al. (2012)	4.0			− 1.73	19.08
This work	4.0	−21.67 ± 0.10	0.54 ± 0.08	− 1.65 ± 0.17
Gabasch et al. (2004)	4.51			− 1.07	19.06
Bouwens et al. (2015)	4.9				19.54
Bouwens et al. (2015)	4.9				19.54
Bouwens et al. (2007)	5.0				19.33
Iwata et al. (2007)	5.0				18.99
McLure et al. (2009)	5.0				19.30
Bouwens et al. (2007)	5.9				19.42
Bouwens et al. (2015)	5.9				19.51
Bouwens et al. (2015)	5.9				19.55
McLure et al. (2009)	6.0				19.39

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