i(cm)z, a semi-analytic model for the thermodynamic properties in galaxy clusters: Calibrations with mass and redshift, and implication for the hydrostatic biasDOI: info:10.1051/0004-6361/202245002v. 669A133
Lovisari, L., Eckert, D., and Ettori, S. 2023. "i(cm)z, a semi-analytic model for the thermodynamic properties in galaxy clusters: Calibrations with mass and redshift, and implication for the hydrostatic bias." Astronomy and Astrophysics, 669 A133. https://doi.org/10.1051/0004-6361/202245002.