CHEX-MATE: Constraining the origin of the scatter in galaxy cluster radial X-ray surface brightness profilesDOI: info:10.1051/0004-6361/202346189v. 674
Bartalucci, I., Molendi, S., Rasia, E., Pratt, G. W., Arnaud, M., Rossetti, M., Gastaldello, F., Eckert, D., Balboni, M., Borgani, S., Bourdin, H., Campitiello, M. G., De Grandi, S., De Petris, M., Duffy, R. T., Ettori, S., Ferragamo, A., Gaspari, M., Gavazzi, R., Ghizzardi, S., Iqbal, A., Kay, S. T., Lovisari, Lorenzo, Mazzotta, P., Maughan, B. J. et al. 2023. "CHEX-MATE: Constraining the origin of the scatter in galaxy cluster radial X-ray surface brightness profiles." Astronomy and Astrophysics, 674. https://doi.org/10.1051/0004-6361/202346189.