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CODEX weak lensing mass catalogue and implications on the mass-richness relation

Kiiveri, K. (author)
Gruen, D. (author)
Finoguenov, A. (author)
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Erben, T. (author)
van Waerbeke, L. (author)
Rykoff, E. (author)
Miller, L. (author)
Hagstotz, Steffen (author)
Stockholms universitet,Fysikum,Oskar Klein-centrum för kosmopartikelfysik (OKC)
Dupke, R. (author)
Henry, J. Patrick (author)
Kneib, J.-P. (author)
Gozaliasl, G. (author)
Kirkpatrick, C. C. (author)
Cibirka, N. (author)
Clerc, N. (author)
Costanzi, M. (author)
Cypriano, E. S. (author)
Rozo, E. (author)
Shan, H. (author)
Spinelli, P. (author)
Valiviita, J. (author)
Weller, J. (author)
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 (creator_code:org_t)
2020-12-23
2021
English.
In: Monthly notices of the Royal Astronomical Society. - : Oxford University Press (OUP). - 0035-8711 .- 1365-2966. ; 502:1, s. 1494-1526
  • Journal article (peer-reviewed)
Abstract Subject headings
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  • The COnstrain Dark Energy with X-ray clusters (CODEX) sample contains the largest flux limited sample of X-ray clusters at 0.35 < z < 0.65. It was selected from ROSAT data in the 10 000 square degrees of overlap with BOSS, mapping a total number of 2770 high-z galaxy clusters. We present here the full results of the CFHT CODEX programme on cluster mass measurement, including a reanalysis of CFHTLS Wide data, with 25 individual lensing-constrained cluster masses. We employ LENSFIT shape measurement and perform a conservative colour–space selection and weighting of background galaxies. Using the combination of shape noise and an analytic covariance for intrinsic variations of cluster profiles at fixed mass due to large-scale structure, miscentring, and variations in concentration and ellipticity, we determine the likelihood of the observed shear signal as a function of true mass for each cluster. We combine 25 individual cluster mass likelihoods in a Bayesian hierarchical scheme with the inclusion of optical and X-ray selection functions to derive constraints on the slope α, normalization β, and scatter σln λ|μ of our richness–mass scaling relation model in log-space: |${\langle {\rm In}\,\, \lambda\!\!\mid\!\!\mu\rangle = \alpha\mu + \beta,} $| with μ = ln (M200c/Mpiv), and Mpiv = 1014.81M⊙. We find a slope |$\alpha = 0.49^{+0.20}_{-0.15}$|⁠, normalization |$\exp (\beta) = 84.0^{+9.2}_{-14.8}$|⁠, and |$\sigma _{\ln \lambda | \mu } = 0.17^{+0.13}_{-0.09}$| using CFHT richness estimates. In comparison to other weak lensing richness–mass relations, we find the normalization of the richness statistically agreeing with the normalization of other scaling relations from a broad redshift range (0.0 < z < 0.65) and with different cluster selection (X-ray, Sunyaev–Zeldovich, and optical).

Subject headings

NATURVETENSKAP  -- Fysik (hsv//swe)
NATURAL SCIENCES  -- Physical Sciences (hsv//eng)

Keyword

gravitational lensing: weak
galaxies: clusters: general
cosmology: observations

Publication and Content Type

ref (subject category)
art (subject category)

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