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Table 1.
Overview of the simulation inputs used for the calibration of the WL bias and scatter.
Name | Use case | Section |
---|---|---|
TNG300 | Projected surface mass density of massive halos at different redshift snapshots | 4.1 |
MAGNETICUM PATHFINDER | Offsets between X-ray surface brightness peak and projected halo center | 4.2.1 |
eROSITA all-sky survey twin | Offsets between X-ray surface brightness peak and measured X-ray position | 4.2.2 |
Mapping between halo mass and redshift, and detection likelihood and extent | 4.4 | |
Monte Carlo realizations | Propagation of systematic uncertainties to error budget on the WL bias | 4.5 |
Notes. The respective references, as well as detailed explanations, are given in the respective sections.
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