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Cited article:

Differences in baryonic and dark matter scaling relations of galaxy clusters: A comparison between IllustrisTNG simulations and observations

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The splashback radius and the radial velocity profile of galaxy clusters in IllustrisTNG

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Astronomy & Astrophysics 683 A82 (2024)
https://doi.org/10.1051/0004-6361/202348643

The mass distribution in the outskirts of clusters of galaxies as a probe of the theory of gravity

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Astronomy & Astrophysics 682 A80 (2024)
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Caustic and hydrostatic mass bias: Implications for modified gravity

Minahil Adil Butt, Balakrishna S. Haridasu, Yacer Boumechta, Francesco Benetti, Lorenzo Pizzuti, Carlo Baccigalupi and Andrea Lapi
Physical Review D 109 (6) (2024)
https://doi.org/10.1103/PhysRevD.109.064006

Galaxy cluster mass accretion rates from IllustrisTNG

Michele Pizzardo, Margaret J. Geller, Scott J. Kenyon, Ivana Damjanov and Antonaldo Diaferio
Astronomy & Astrophysics 680 A48 (2023)
https://doi.org/10.1051/0004-6361/202347470