Weighing the giants - III. Methods and measurements of accurate galaxy cluster weak-lensing masses

Douglas E. Applegate, Anja Von der linden, Patrick L. Kelly, Mark T. Allen, Steven W. Allen, Patricia R. Burchat, David L. Burke, Harald Ebeling, Adam Mantz, R. Glenn Morris

Research output: Contribution to journalArticlepeer-review

160 Scopus citations

Abstract

We report weak-lensing masses for 51 of the most X-ray luminous galaxy clusters known. This cluster sample, introduced earlier in this series of papers, spans redshifts 0.15{less-than or approximate}zcl{less-than or approximate}0.7, and is well suited to calibrate mass proxies for current cluster cosmology experiments. Cluster masses are measured with a standard 'colour-cut' lensing method from three-filter photometry of each field. Additionally, for 27 cluster fields with at least five-filter photometry, we measure high-accuracy masses using a new method that exploits all information available in the photometric redshift posterior probability distributions of individual galaxies. Using simulations based on the COSMOS-30 catalogue, we demonstrate control of systematic biases in the mean mass of the sample with this method, from photometric redshift biases and associated uncertainties, to better than 3 per cent. In contrast, we show that the use of single-point estimators in place of the full photometric redshift posterior distributions can lead to significant redshift-dependent biases on cluster masses. The performance of our new photometric redshift-based method allows us to calibrate 'colour-cut' masses for all 51 clusters in the present sample to a total systematic uncertainty of ≈7 per cent on the mean mass, a level sufficient to significantly improve current cosmology constraints from galaxy clusters. Our results bode well for future cosmological studies of clusters, potentially reducing the need for exhaustive spectroscopic calibration surveys as compared to other techniques, when deep, multifilter optical and near-IR imaging surveys are coupled with robust photometric redshift methods.

Original languageEnglish (US)
Pages (from-to)48-72
Number of pages25
JournalMonthly Notices of the Royal Astronomical Society
Volume439
Issue number1
DOIs
StatePublished - Mar 2014

Keywords

  • Cosmology: Observations
  • Galaxies: Clusters: General
  • Galaxies: Distances and redshifts
  • Gravitational lensing: Weak
  • Methods: Data analysis
  • Methods: Statistical

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