Fig. 6.

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Significant correlations between luminosity and the observed UFO properties and energetics. Panel a: LX versus vout (upper plot), ξ (middle plot), and NH (lower plot). Panel b: LX versus Ṁwind (upper plot), (middle plot), and Ṗwind (lower plot). The S23 UFO sub-sample is shown in red circles, T10 in blue diamonds, and C21 in black squares. The solid lines represent the best-fitting linear correlation and the dark and light gray shadowed areas indicate the 68% and 90% confidence bands, respectively. In the legend, we report the best-fit coefficients, logNHP, and the intrinsic scatters for the correlations.
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