Fig. 3.
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IN2H+/ICO as function of IHCN/TCO for all data points and subsets above a 3σ noise level. We show the average uncertainty in the bottom right corner, as well as the best-fit from Jiménez-Donaire et al. (2023, Eq. (2)) with a power law slope of 1.0 derived for extragalactic and Galactic data points (green line). Contours indicate the number density of data points.
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