Galaxy Cluster Mass Reconstruction Project - IV. Understanding the effects of imperfect membership on cluster mass estimation

R. Wojtak, L. Old, G. A. Mamon, F. R. Pearce, R. de Carvalho, C. Sifón, M. E. Gray, R. A. Skibba, D. Croton, S. Bamford, D. Gifford, A. von der Linden, J. C. Muñoz-Cuartas, V. Müller, R. J. Pearson, E. Rozo, E. Rykoff, A. Saro, T. Sepp, E. Tempel

Research output: Contribution to journalArticle

8 Scopus citations

Abstract

The primary difficulty in measuring dynamical masses of galaxy clusters from galaxy data lies in the separation between true cluster members from interloping galaxies along the line of sight.We study the impact of membership contamination and incompleteness on cluster mass estimates obtained with 25 commonly used techniques applied to nearly 1000 mock clusters with precise spectroscopic redshifts. We show that all methods overestimate or underestimate cluster masses when applied to contaminated or incomplete galaxy samples, respectively. This appears to be the main source of the intrinsic scatter in the mass scaling relation. Applying corrections based on a prior knowledge of contamination and incompleteness can reduce the scatter to the level of shot noise expected for poorly sampled clusters.We establish an empirical model quantifying the effect of imperfect membership on cluster mass estimation and discuss its universal and method-dependent features.We find that both imperfect membership and the response of the mass estimators depend on cluster mass, effectively causing a flattening of the estimated-true mass relation. Imperfect membership thus alters cluster counts determined from spectroscopic surveys, hence the cosmological parameters that depend on such counts.

Original languageEnglish (US)
Pages (from-to)324-340
Number of pages17
JournalMonthly Notices of the Royal Astronomical Society
Volume481
Issue number1
DOIs
StatePublished - Nov 21 2018

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Keywords

  • Cosmology: observations
  • Galaxies: clusters: general
  • Galaxies: haloes
  • Galaxies: kinematics and dynamics
  • Methods: numerical
  • Methods: statistical

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

Cite this

Wojtak, R., Old, L., Mamon, G. A., Pearce, F. R., de Carvalho, R., Sifón, C., Gray, M. E., Skibba, R. A., Croton, D., Bamford, S., Gifford, D., von der Linden, A., Muñoz-Cuartas, J. C., Müller, V., Pearson, R. J., Rozo, E., Rykoff, E., Saro, A., Sepp, T., & Tempel, E. (2018). Galaxy Cluster Mass Reconstruction Project - IV. Understanding the effects of imperfect membership on cluster mass estimation. Monthly Notices of the Royal Astronomical Society, 481(1), 324-340. https://doi.org/10.1093/mnras/sty2257