Fig. 17.
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Redshift distribution of the eROSITA/DR1 extragalactic sources in the footprint of LS10, split among the sources that are also detected in Gaia, Quaia, and AllWISE/R90, respectively. The majority of the sources that are unique to eRASS1 are at low redshift, where the contribution from the host galaxy dominates the SED in optical and NIR.
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