A multi-instrument non-parametric reconstruction of the electron pressure profile in the galaxy cluster CLJ1226.9+3332

C. Romero; M. McWilliam; J.-F. Macías-Pérez; R. Adam; P. Ade; P. André; H. Aussel; A. Beelen; A. Benoît; A. Bideaud; N. Billot; O. Bourrion; M. Calvo; A. Catalano; G. Coiffard; B. Comis; M. de Petris; F.-X. Désert; S. Doyle; J. Goupy; C. Kramer; G. Lagache; S. Leclercq; J.-F. Lestrade; P. Mauskopf; F. Mayet; A. Monfardini; E. Pascale; L. Perotto; G. Pisano; N. Ponthieu; V. Revéret; A. Ritacco; H. Roussel; F. Ruppin; K. Schuster; A. Sievers; S. Triqueneaux; C. Tucker; R. Zylka

doi:10.1051/0004-6361/201731599

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Volume 612 (April 2018)

A&A, 612 (2018) A39

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Table 2

Non parametric pressure profile fits.

R	P_e
(kpc)	(keV cm⁻³)	(keV cm⁻³)	(keV cm⁻³)
NIKA

73	0.225	0.051	0.035
134	0.150	0.049	0.065
216	0.0744	0.0181	0.0226
349	0.0358	0.0053	0.0060
564	0.00508	0.00068	0.00071
910	0.00200	0.00024	0.00024

MUSTANG

37	0.257	0.151	0.115
67	0.311	0.146	0.216
110	0.0436	0.0243	0.0352
180	0.0874	0.0231	0.0270
294	0.0133	0.0064	0.0091
479	0.000959	0.00082	0.00284

Bolocam

233	0.0367	0.0147	0.0092
429	0.0332	0.0139	0.0181
698	0.00795	0.0035	0.0045
1135	0.00141	0.00081	0.00104
1845	0.00320	0.00083	0.00084
3000	0.00101	0.00044	0.00047

Notes. P_e is taken as the 50th percentile, and the corresponding errors bars (σ) are taken atthe 16th and 84th percentiles. The red rows correspond to bins which have been trimmed.

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