ALHAMBRA UV LF at two redshift bins as indicated in the panels. The ALHAMBRA measurements are shown as blue squares together with their 2-σ error bars, and the blue line shows our best median Schechter fit, shaded area enclosing 95% of the solutions. Left panels: comparison with literature data from photometrically selected samples of high-z galaxies is shown as follows: triangles (Reddy & Steidel 2009), upside-down triangles (van der Burg et al. 2010), diamonds (Mehta et al. 2017), pentagons and orange dashed-line (Parsa et al. 2016), open circles (Ono et al. 2018), left pointing triangles (Finkelstein et al. 2015), and hexagons (Bouwens et al. 2015). Right panels: comparison with the spectroscopic LF estimate of Cucciati et al. (2012) (black dots and red dotted line).