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McWilliam, N. Billot, N. Ponthieu1, O. Bourrion, P. Ade, P. Andre, P. Mauskopf, R. Adam, R. Zylka, S. Doyle, S. Leclercq, S. Triqueneaux, V. Reveret","submitted_at":"2017-07-19T14:28:06Z","abstract_excerpt":"Context: In the past decade, sensitive, resolved Sunyaev-Zel'dovich (SZ) studies of galaxy clusters have become common. Whereas many previous SZ studies have parameterized the pressure profiles of galaxy clusters, non-parametric reconstructions will provide insights into the thermodynamic state of the intracluster medium (ICM). Aims: We seek to recover the non-parametric pressure profiles of the high redshift ($z=0.89$) galaxy cluster CLJ 1226.9+3332 as inferred from SZ data from the MUSTANG, NIKA, Bolocam, and Planck instruments, which all probe different angular scales. 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