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Date and Time of the Query: 2019-07-23 T04:34:54 PDT
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For refcode 2014ApJ...794..175M:
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2014ApJ...794..175M Erratum: "Joint Analysis of Cluster Observations. II. Chandra/XMM-Newton X-Ray and Weak Lensing Scaling Relations for a Sample of 50 Rich Clusters of Galaxies" (2013, ApJ, 767, 116) Mahdavi, Andisheh; Hoekstra, Henk; Babul, Arif; Bildfell, Chris; Jeltema, Tesla; Henry, J. Patrick Abstract. The published version of the article "Joint Analysis of Cluster Observations. II. Chandra/XMM-Newton X-ray and Weak Lensing Scaling Relations for a Sample of 50 Rich Clusters of Galaxies" contained an error in the bolometric correction factor in the reported X-ray luminosities. In addition, Table 1 contained thermodynamic quantities reported at r2500 instead of r500. No other aspects of the analysis were affected. We present a table with updated quantities and fit results.{see Table 1} In the published version of this article, we applied an incorrect bolometric bandpass correction factor to the X-ray flux of all clusters, resulting in bolometric X-ray luminosities that were too high throughout the entire analysis. Since this was a problem only with the bandpass correction factor, none of the other results of the paper were affected. In addition, Table 1 of the published article reported luminosities and temperatures at an aperture of r2500 instead of r500. Here we present updated luminosities and mass-luminosity scaling relations (Table 3) which take the correct bolometric correction factor into account. Note that the Chandra and XMM-Newton Observatory calibrations used are the same one as in the published article. These updated numbers are also present on the Web site of the paper, http://sfstar.sfsu.edu/jaco. Since the error was roughly a constant factor applied to LX, only the intercepts of the LX relations have changed substantially; the slopes and intrinsic scatters of these relations are still within the originally reported limits. {see Table 3}
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