Forecasts on dark energy from the X-ray cluster survey with eROSITA: constraints from counts and clustering

Author:

Pillepich Annalisa123,Reiprich Thomas H4,Porciani Cristiano4,Borm Katharina4,Merloni Andrea5

Affiliation:

1. Max-Planck-Institut für Astronomie, Königstuhl 17, D-69117 Heidelberg, Germany

2. Harvard–Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138, USA

3. Department of Astronomy and Astrophysics, University of California, Santa Cruz, CA 95064, USA

4. Argelander-Institut für Astronomie, Auf dem Hügel 71, D-53121 Bonn,Germany

5. Max-Planck-Institut für Extraterrestriche Physik, Postfach 1312, D-85741 Garching bei München, Gemany

Funder

Deutsche Forschungsgemeinschaft

Ministry of Economy and Technology

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

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1. The SRG/eROSITA All-Sky Survey;Astronomy & Astrophysics;2024-06

2. X-ray Cluster Cosmology;Handbook of X-ray and Gamma-ray Astrophysics;2024

3. The cosmological analysis of X-ray cluster surveys. V. The potential of cluster counts in the 1 < z < 2 range;Astronomy & Astrophysics;2023-12-06

4. Painting baryons on to N-body simulations of galaxy clusters with image-to-image deep learning;Monthly Notices of the Royal Astronomical Society;2023-09-06

5. Benchmarks and explanations for deep learning estimates of X-ray galaxy cluster masses;Monthly Notices of the Royal Astronomical Society;2023-07-05

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