Fig. 9.

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Comparison of the host-galaxy properties of CDF-S XT1 and XT2 with the cumulative distributions of galaxy stellar mass (left panel) and star-formation rate (right panel) for LGRBs (Li et al. 2016; Blanchard et al. 2016), SGRBs (Fong et al. 2010, 2012, 2014; Margutti et al. 2012; Sakamoto et al. 2013; Berger et al. 2013; Fong et al. 2022; Nugent et al. 2022), FRBs (Heintz et al. 2020), CC-SNe and Ia-SNe (Tsvetkov & Bartunov 1993; Prieto et al. 2008; Galbany et al. 2014), low-luminosity LGRBs (GRB 980425, GRB 020903, GRB 030329, GRB 031203, GRB 050826, GRB 060218, GRB 100316D, GRB 111005A, and GRB 171205A; Christensen et al. 2008; Michałowski et al. 2014; Levesque 2014; Krühler et al. 2017; Wiersema et al. 2007; Izzo et al. 2017; Wang et al. 2018; MichałowskI et al. 2018; Arabsalmani et al. 2019), and SLSNe (Schulze et al. 2021). The dashed vertical lines depict the mean values of CDF-S XT1 (red vertical lines) and XT2 (blue vertical lines).
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