TL;DR
The paper discusses how the eROSITA X-ray survey will significantly enhance the detection and study of nearby young stars by providing a highly sensitive all-sky X-ray dataset, surpassing previous surveys.
Contribution
It introduces the eROSITA survey's capabilities and its potential to identify and analyze a vast number of young stars in X-rays, advancing stellar astrophysics.
Findings
Expected detection of over half a million stars in X-rays
Enhanced sensitivity over previous surveys by more than an order of magnitude
Potential for new insights into magnetic activity of young stars
Abstract
X-ray surveys are well suited to detect, identify and study young stars based on their high levels of magnetic activity and thus X-ray brightness. The eROSITA instrument onboard the Spectrum-Roentgen-Gamma (SRG) satellite will perform an X-ray all-sky survey that surpasses existing data by a sensitivity increase of more than an order of magnitude. The 4 yr survey is expected to detect more than half a million stars and stellar systems in X-rays.
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