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Fig. 20

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Partial Hubble diagram residuals (and profiles) as a function of colour (top) and X1 (bottom) for the identified (green filled circles and profiles) and unidentified (black open circles and profiles) subsamples of photometrically selected SNe Ia with iM < 23. The straight lines are linear fits to the full sample of events with iM < 23.

This figure is made of several images, please see below:

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