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This article has an erratum: [https://doi.org/10.1051/0004-6361/202244547e]


Fig. 1.

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MS0735 in the SZ and X-ray. Left: MUSTANG-2 image of MS0735.6+7421 in units of μKCMB. The image is smoothed by a 1 pixel Gaussian (6″), yielding an effective resolution of 9.5″. Right: exposure-corrected broadband (0.5–7.0 keV) Chandra X-ray image of MS0735.6+7421 using the same ∼500 ksec of data reported in V14. The image is binned 2 × 2 pixels from the native resolution of 0.496″and smoothed by a 0.984″Gaussian. Dashed white contours correspond to the signal to noise of the decrement seen in the MUSTANG-2 image (left), smoothed by 2 pixels, and are at a signal-to-noise ratio S/N = −(1, 2, 3). The green contours correspond to 338 MHz continuum radio emission as traced by VLITE (resolution 21.5″× 16.2″) and trace the jets. At z = 0.216, the 1′ scale bar corresponds to 212 kpc.

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