Fig. 1.
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Distribution of radio luminosities as a function of redshift. Our sample is shown in red, and the searches reported in the literature are shown in black. At z < 0.25, the plot shows the sample of Maccagni et al. (2017). At z > 0.25 the searches are from Carilli & van Gorkom (1992), Carilli et al. (1998), Pihlström et al. (2003), Vermeulen et al. (2003), Gupta et al. (2006), Orienti et al. (2006), Curran et al. (2006, 2011, 2017, 2019), Allison et al. (2015), Yan et al. (2016), Ostorero et al. (2017), Aditya & Kanekar (2018a,b), Aditya (2019), Grasha et al. (2019), Mhaskey et al. (2020), and Murthy et al. (2021).
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