Fig. 9.
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Cumulative distribution of sources within the LS10 footprint sorted in order of reliability of the star and galaxy classification. Sources with a STAREX probability to be extragalactic below 50% are further split into classes (from 3 to –1) using a combination of STAREX output and diagnostic colour-colour diagrams (grzW1 and W1X) as described in 5.3.2.
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