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Erratum: “Inferences from Surface Brightness Fluctuations of Zwicky 3146 via the Sunyaev–Zel’dovich Effect and X-Ray Observations” (2023, ApJ, 951, 41)

  • Authors: Charles E. Romero, Massimo Gaspari, Gerrit Schellenberger, Tanay Bhandarkar, Mark Devlin, Simon R. Dicker, William Forman, Rishi Khatri, Ralph Kraft, Luca Di Mascolo, Brian S. Mason, Emily Moravec, Tony Mroczkowski, Paul Nulsen, John Orlowski-Scherer, Karen Perez Sarmiento, Craig Sarazin, Jonathan Sievers, Yuanyuan Su

Charles E. Romero et al 2024 The Astrophysical Journal 965 .

  • Provider: AAS Journals

Caption: Figure 16.

The bias induced by the PSF (shaded regions) relative to the PSF correction (dashed lines). The solid lines indicate the bias when α = 3 for XMM and α = 2 for MUSTANG-2. The shaded regions encompass the bias between α = 1.5 and α = 4.5 for XMM and between α = 0.5 and α = 3.5 for MUSTANG-2. For a full comparison the orange dotted lines show the biases for α = 1.5 and α = 4.5 with the MUSTANG-2 beam.

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