Shedding Light on the Matter of Abell 781

Abstract

The galaxy cluster Abell 781 West has been viewed as a challenge to weak gravitational lensing mass calibration, as Cook and dell'Antonio (2012) found that the weak lensing signal-to-noise in three independent sets of observations was consistently lower than expected from mass models based on X-ray and dynamical measurements. We correct some errors in statistical inference in Cook and dell'Antonio (2012) and show that their own results agree well with the dynamical mass and exhibit at most 2.2--2.9$\sigma$ low compared to the X-ray mass, similar to the tension between the dynamical and X-ray masses. Replacing their simple magnitude cut with weights based on source photometric redshifts eliminates the tension between lensing and X-ray masses; in this case the weak lensing mass estimate is actually higher than, but still in agreement with, the dynamical estimate. A comparison of lensing analyses with and without photometric redshifts shows that a 1--2$\sigma$ chance alignment of low-redshift sources lowers the signal-to-noise observed by all previous studies which used magnitude cuts rather than photometric redshifts. The fluctuation is unexceptional, but appeared to be highly significant in Cook and dell'Antonio (2012) due to the errors in statistical interpretation.

7 pages, submitted to MNRAS

References in corpus (6)

• What Lies Beneath: Using p(z) to Reduce Systematic Photometric Redshift Errors
• Shear-Selected Clusters From the Deep Lens Survey III: Masses from Weak Lensing
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• Merging Cluster Collaboration: A Panchromatic Atlas of Radio Relic Mergers
• Can giant radio halos probe the merging rate of galaxy clusters?
• Detection of universality of dark matter profile from Subaru weak lensing measurements of 50 massive clusters
• The spectacular cluster chain Abell 781 as observed with LOFAR, GMRT, and XMM-Newton
• Probabilistic Cosmological Mass Mapping from Weak Lensing Shear
• X-ray Temperatures, Luminosities, and Masses From XMM-Newton Follow-up of the First Shear-selected Galaxy Cluster Sample