The eROSITA Final Equatorial-Depth Survey (eFEDS) - X-ray 
observable-to-mass-and-redshift relations of galaxy clusters and groups with 
weak-lensing mass calibration from the Hyper Suprime-Cam Subaru Strategic 
Program survey

nCChhiiuu, NI-oNno; Ghirardini, Vittorio; Liu, Ang; Grandis, Sebastian; Bulbul, Esra; Bahar, Y. Emre; Comparat, Johan; Bocquet, Sebastian; Clerc, Nicolas; Klein, Matthias; Liu, Teng; Li, Xiangchong; Miyatake, Hironao; Mohr, Joseph; More, Surhud; Oguri, Masamune; Okabe, Nobuhiro; Pacaud, Florian; Ramos-Ceja, Miriam E.; Reiprich, Thomas H.; Schrabback, Tim; Umetsu, Keiichi

doi:10.1051/0004-6361/202141755

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The eROSITA Final Equatorial-Depth Survey (eFEDS) - X-ray observable-to-mass-and-redshift relations of galaxy clusters and groups with weak-lensing mass calibration from the Hyper Suprime-Cam Subaru Strategic Program survey

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Ghirardini, Vittorio
High Energy Astrophysics, MPI for Extraterrestrial Physics, Max Planck Society;

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Liu, Ang
High Energy Astrophysics, MPI for Extraterrestrial Physics, Max Planck Society;

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Bulbul, Esra
High Energy Astrophysics, MPI for Extraterrestrial Physics, Max Planck Society;

/persons/resource/persons284363

Bahar, Y. Emre
High Energy Astrophysics, MPI for Extraterrestrial Physics, Max Planck Society;

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Comparat, Johan
High Energy Astrophysics, MPI for Extraterrestrial Physics, Max Planck Society;

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Liu, Teng
High Energy Astrophysics, MPI for Extraterrestrial Physics, Max Planck Society;

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Mohr, Joseph
Optical and Interpretative Astronomy, MPI for Extraterrestrial Physics, Max Planck Society;

/persons/resource/persons247131

Ramos-Ceja, Miriam E.
High Energy Astrophysics, MPI for Extraterrestrial Physics, Max Planck Society;

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nCChhiiuu, N.-o., Ghirardini, V., Liu, A., Grandis, S., Bulbul, E., Bahar, Y. E., et al. (2022). The eROSITA Final Equatorial-Depth Survey (eFEDS) - X-ray observable-to-mass-and-redshift relations of galaxy clusters and groups with weak-lensing mass calibration from the Hyper Suprime-Cam Subaru Strategic Program survey. Astronomy and Astrophysics, 661: A11. doi:10.1051/0004-6361/202141755.

Cite as: https://hdl.handle.net/21.11116/0000-000B-FC0F-A

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