Solution for as derived in this work (red line) and, using black dashed line, the CSFR used by Vangioni et al. (2018) plotted for comparison. Left: evolution of the CSFR from the local Universe to z = 20. Right: same as for the left panel, but zooming into 0 ≤ z ≤ 10, allowing for a better visualization of the two CSFRs within the range of the available observational data. Data used in this figure: IR (Magnelli et al. 2011, 2013 – dark gray filled circles; Gruppioni et al. 2013 – dark orange open circles); UV (Wyder et al. 2005 – slate gray open triangle; Schiminovich et al. 2005 – blue crosses; Dahlen et al. 2007 – turquoise open squares; Reddy & Steidel 2009 – dark green filled squares; Robotham & Driver 2011 – chocolate cross; Cucciati et al. 2012 – green stars; Bouwens et al. 2012a, 2012b – teal filled triangles); and GRB (Kistler et al. 2009 – deep pink open triangles).