Fig. 20
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X-ray luminosity function of the eRASS1 cluster sample. Left panel: results for the full sample. Literature results are plotted as the shaded area for comparison: COSMOS (Finoguenov et al. 2007), WARPS (Koens et al. 2013), XXL-100 (Pacaud et al. 2016), XXL-C1 (Adami et al. 2018), SPIDERS (Clerc et al. 2020) surveys. Right panel: results in three redshift bins. No significant XLF evolution is detected in eRASS1 clusters.
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