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Table 2.

Comparison of SRG/eROSITA forecasts with other cosmological probes.

Experiment ΔΩm ΔΩb Δh Δns Δσ8 ΔS8

SRG/eRosita (1) ±0.016 ±0.014 ±0.172 ±0.108 ±0.005 ±0.019

SRG/eRosita (1)h, nsPlanck prior ±0.008 ±0.004 ±0.004 ±0.003 ±0.003 ±0.012

Planck (CMB+lensing) (2) ±0.0074 ±0.0007 ±0.0054 ±0.0042 ±0.0061 ±0.013

SDSS BOSS (3)

DES 3×2pt4

DES 3×2pt +BAO+RSD+SNIa+CMB (4)

SRG/eRosita ±0.0031 ±0.0492 ±0.364 ±0.143 ±0.003

Cluster mass function (5)

Euclid (6) ±0.0038 ±0.046 ±0.020 ±0.0037 ±0.0017

Notes. Forecast Fisher marginalised errors for cosmological parameters in the flat ΛCDM model. SRG/eROSITA results are for the combined data of AGNs and clusters of galaxies, with and without Planck priors.

References:(1)This work; (2)Planck Collaboration VI (2020); (3)Loureiro et al. (2019); (4)Abbott et al. (2022a); (5)Pillepich et al. (2012); (6)Euclid Collaboration (2020).

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