Fig. 2.
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Flux distribution in the 0.6–2.3 keV band of the star-forming galaxies in the HEC-eR1 sample as a function of the exposure time. Black stars show the mode value of the source’s intensity for the galaxies with reliable fluxes and their 68% C.I. uncertainties. Grey down arrows show the upper 90% C.I. for the galaxies with uncertain flux measurements.
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