Fig. 4.
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Comparison between observed and modelled locations of core-collapse supernovae (CCSNe). Left: CCSN offsets from the ATLAS volumetric survey (Srivastav et al. 2022; Srivastav et al., in prep.) compared to those seen in our models (note that these are exclusively binary systems that can lead to BNS mergers, not an exhaustive theoretical population of CCSNe). Right: same as in the left panel, with the observed normalised offsets of CCSNe from Kelly & Kirshner (2012).
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