Fig. 3.
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1.17 mm source number count of the deep SSA22 field. For comparison, we show interferometric number counts of random fields from the literature, with fluxes converted to 1.17 mm: Karim et al. (2013), Ono et al. (2014), Carniani et al. (2015), Hatsukade et al. (2016, 2018), Stach et al. (2018), González-López et al. (2020), Simpson et al. (2020), Béthermin et al. (2020), Gómez-Guijarro et al. (2022), Chen et al. (2023), and Fujimoto et al. (2024). We also present the total number count of the z = 2.16 Spiderweb protocluster (Zhang et al. 2024). The dashed line shows the best-fit Schechter function from Gómez-Guijarro et al. (2022).
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