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Fig. 7.

image

Evolution of the total SFRD (Eq. (2)) with redshift. The red symbols are the total SFRDs, derived in this paper. Small offsets of ±0.08 are applied to their redshift for clarity. The triangles are the lower limits for SFRDIR derived in Sect. 4.3.1. The blue symbols are dust-corrected SFRD derived from the FUV data (Cucciati et al. 2012; Dahlen et al. 2007; Reddy & Steidel 2009; Bouwens et al. 2012, 2015b; Schenker et al. 2013; Pelló et al. 2018; Khusanova et al. 2020), orange symbols are derived from reradiated dust emission from forming stars as measured from the IR (Magnelli et al. 2013; Gruppioni et al. 2013, 2020; Rowan-Robinson et al. 2016; Koprowski et al. 2017; Wang et al. 2019a; Riechers et al. 2020). The magenta points are from other SFR tracers: [CII] luminosity function based on the ALPINE field sample of Loiacono et al. (2021) and number counts of γ-ray bursts (Kistler et al. 2009). The dotted line is the fit of SFRD evolution from Madau & Dickinson (2014).

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