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A COMPARISON AND JOINT ANALYSIS OF SUNYAEV–ZEL’DOVICH EFFECT MEASUREMENTS FROM PLANCK AND BOLOCAM FOR A SET OF 47 MASSIVE GALAXY CLUSTERS

  • Authors: Jack Sayers, Sunil R. Golwala, Adam B. Mantz, Julian Merten, Sandor M. Molnar, Michael Naka, Gregory Pailet, Elena Pierpaoli, Seth R. Siegel, and Ben Wolman

2016 The Astrophysical Journal 832 26.

  • Provider: AAS Journals

Caption: Figure 1.

Examples of the SZ data used in this analysis for the cluster Abell 370. Left: Bolocam data (top) and 1 of the 1000 noise realizations (bottom) smoothed to an effective FWHM of 1.′4 for visualization (the unsmoothed data are used for all analyses). Middle: Planck MILCA y-map (top) and 1 of the 1000 noise realizations (bottom). Right, top: Planck MMF3 PDF (blue contours separated by 0.1 in probability) and the Planck XMM-like constraint on the value of ﹩{\theta }_{{\rm{s}}}﹩ (solid red, with each color separated by 0.1 in probability). Right, bottom: one-dimensional constraint on the value of ﹩{Y}_{5{\rm{R}}500}﹩ based on the Planck PDF and the XMM prior on ﹩{\theta }_{{\rm{s}}}﹩.

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