Lowering the eROSITA energy threshold to 0.1 keV reveals soft white dwarf sources missed at 0.2 keV, and the German half-sky already hosts 264 high-confidence white dwarf candidates.
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Searching the non-accreting white dwarf population in eROSITA data
Lowering the eROSITA energy threshold to 0.1 keV reveals soft white dwarf sources missed at 0.2 keV, and the German half-sky already hosts 264 high-confidence white dwarf candidates.