Fig. 2.
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Resulting WD component (thick salmon) of the AGWB compared to the LVK results (upper limit to BH/NS AGWB (dashed grey) and estimates for the BBH and BNS components in green and blue), the LISA Powerlaw Integrated sensitivity (black, Thrane & Romano 2013; Alonso et al. 2020), and an estimate of the Galactic foreground (brown) based on Karnesis et al. (2021). A fit to the WD component is shown in dark red.
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