CODEX weak lensing: concentration of galaxy clusters at z ~ 0.5

Cibirka, N.; Cypriano, E. S.; Brimioulle, F.; Gruen, D.; Erben, T.; van Waerbeke, L.; Miller, L.; Finoguenov, A.; Kirkpatrick, C.; Henry, J. Patrick; Rykoff, E.; Rozo, E.; Dupke, R.; Kneib, J. -P.; Shan, H.; Spinelli, P.

doi:10.1093/mnras/stx484

Title: CODEX weak lensing: concentration of galaxy clusters at z ~ 0.5

Journal Article · Fri Mar 03 23:00:00 EST 2017 · Monthly Notices of the Royal Astronomical Society

DOI: https://doi.org/10.1093/mnras/stx484 · OSTI ID:1360791

Cibirka, N. ^[1]; Cypriano, E. S. ^[2]; Brimioulle, F. ^[3]; Gruen, D. ^[4]; Erben, T. ^[5]; van Waerbeke, L. ^[6]; Miller, L. ^[7]; Finoguenov, A. ^[8]; Kirkpatrick, C. ^[9]; Henry, J. Patrick ^[10]; Rykoff, E. ^[4]; Rozo, E. ^[11]; Dupke, R. ^[12]; Kneib, J. -P. ^[13]; Shan, H. ^[14]; Spinelli, P. ^[15]

Univ. of Sao Paulo (Brazil). Inst. of Astronomy, Geophysics and Atmospheric Sciences; Ludwig Maximilian Univ., Munich (Germany)
Univ. of Sao Paulo (Brazil). Inst. of Astronomy, Geophysics and Atmospheric Sciences
Max Planck Inst. fur Extraterrestrische Physik, Garching (Germany); National Observatory, Rio de Janeiro (Brazil); Ludwig Maximilian Univ., Munich (Germany)
Stanford Univ., CA (United States). Kavli Inst. for Particle Astrophysics & Cosmology; SLAC National Accelerator Lab., Menlo Park, CA (United States)
Argelander-Inst. fur Astronomie, Bonn (Germany)
Univ. of British Columbia, Vancouver, BC (Canada). Dept. of Physics and Astronomy
Univ. of Oxford (United Kingdom). Dept. of Physics
Univ. of Helsinki (Finland). Dept. of Physics; Max Planck Inst. fur Extraterrestrische Physik, Garching (Germany)
Univ. of Helsinki (Finland). Dept. of Physics; Univ. of Helsinki (Finland). Helsinki Inst. of Physics
Inst. for Astronomy, Honolulu, HI (United States)
Univ. of Arizona, Tucson, AZ (United States). Dept. of Physics
National Observatory, Rio de Janeiro (Brazil); Univ. of Michigan, Ann Arbor, MI (United States). Dept. of Astronomy; Univ. of Alabama, Tuscaloosa, AL (United States). Dept. of Physics and Astronomy; Eureka Scientic Inc., Oakland, CA (United States)
Ecole Polytechnique Federale Lausanne (Switzlerland). Lab. d'Astrophysique, Observatoire de Sauverny; Aix-Marseille Univ., and CNRS/IN2P3, Marseille (France). Lab. d'Astrophysique de Marseille
Ecole Polytechnique Federale Lausanne (Switzlerland). Lab. d'Astrophysique, Observatoire de Sauverny
Museum of Astronomy and Related Sciences (MAST), Rio de Janeiro (Brazil)

Here, we present a stacked weak-lensing analysis of 27 richness selected galaxy clusters at 0.40 ≤ z ≤ 0.62 in the COnstrain Dark Energy with X-ray galaxy clusters (CODEX) survey. The fields were observed in five bands with the Canada–France–Hawaii Telescope (CFHT). We measure the stacked surface mass density profile with a 14σ significance in the radial range 0.1 < RMpch^-1 < 2.5. The profile is well described by the halo model, with the main halo term following a Navarro–Frenk–White profile (NFW) profile and including the off-centring effect. We select the background sample using a conservative colour–magnitude method to reduce the potential systematic errors and contamination by cluster member galaxies. We perform a Bayesian analysis for the stacked profile and constrain the best-fitting NFW parameters M_200c=6.6$$+1.0\atop{-0.8}$$×10¹⁴h^-1 M⊙ and c_200c=3.7$$+0.7\atop{-0.6}$$. The off-centring effect was modelled based on previous observational results found for redMaPPer Sloan Digital Sky Survey clusters. Our constraints on M200c and c200c allow us to investigate the consistency with numerical predictions and select a concentration–mass relation to describe the high richness CODEX sample. Comparing our best-fitting values for M200c and c200c with other observational surveys at different redshifts, we find no evidence for evolution in the concentration–mass relation, though it could be mitigated by particular selection functions. Similar to previous studies investigating the X-ray luminosity–mass relation, our data suggest a lower evolution than expected from self-similarity.

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Research Organization:: SLAC National Accelerator Laboratory (SLAC), Menlo Park, CA (United States)

Sponsoring Organization:: USDOE; National Aeronautic and Space Administration (NASA)

Grant/Contract Number:: AC02-76SF00515

OSTI ID:: 1360791

Journal Information:: Monthly Notices of the Royal Astronomical Society, Journal Name: Monthly Notices of the Royal Astronomical Society Journal Issue: 1 Vol. 468; ISSN 0035-8711

Publisher:: Royal Astronomical SocietyCopyright Statement

Country of Publication:: United States

Language:: English

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CFHTLenS: improving the quality of photometric redshifts with precision photometry★: CFHTLenS: photometric redshifts Hildebrandt, H.; Erben, T.; Kuijken, K. Monthly Notices of the Royal Astronomical Society, Vol. 421, Issue 3 https://doi.org/10.1111/j.1365-2966.2012.20468.x	journal	February 2012
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Halo concentrations in the standard Λ cold dark matter cosmology: ΛCDM halo concentrations Prada, Francisco; Klypin, Anatoly A.; Cuesta, Antonio J. Monthly Notices of the Royal Astronomical Society, Vol. 423, Issue 4 https://doi.org/10.1111/j.1365-2966.2012.21007.x	journal	June 2012
The effects of baryonic cooling on the concentration-mass relation: On the concentration-mass relation Fedeli, C. Monthly Notices of the Royal Astronomical Society, Vol. 424, Issue 2 https://doi.org/10.1111/j.1365-2966.2012.21302.x	journal	June 2012
Means of confusion: how pixel noise affects shear estimates for weak gravitational lensing: How pixel noise affects shear estimates Melchior, P.; Viola, M. Monthly Notices of the Royal Astronomical Society, Vol. 424, Issue 4 https://doi.org/10.1111/j.1365-2966.2012.21381.x	journal	July 2012
Noise bias in weak lensing shape measurements: Noise bias in lensing shape measurement Refregier, Alexandre; Kacprzak, Tomasz; Amara, Adam Monthly Notices of the Royal Astronomical Society, Vol. 425, Issue 3 https://doi.org/10.1111/j.1365-2966.2012.21483.x	journal	August 2012
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Miscentring in galaxy clusters: dark matter to brightest cluster galaxy offsets in 10 000 Sloan Digital Sky Survey clusters: Miscentring in galaxy clusters Zitrin, Adi; Bartelmann, Matthias; Umetsu, Keiichi Monthly Notices of the Royal Astronomical Society, Vol. 426, Issue 4 https://doi.org/10.1111/j.1365-2966.2012.21886.x	journal	October 2012
The dynamical state and mass–concentration relation of galaxy clusters: The concentrations of massive galaxy clusters Ludlow, Aaron D.; Navarro, Julio F.; Li, Ming Monthly Notices of the Royal Astronomical Society, Vol. 427, Issue 2 https://doi.org/10.1111/j.1365-2966.2012.21892.x	journal	November 2012
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Constraining self-interacting dark matter with scaling laws of observed halo surface densities Bondarenko, Kyrylo; Boyarsky, Alexey; Bringmann, Torsten Journal of Cosmology and Astroparticle Physics, Vol. 2018, Issue 04 https://doi.org/10.1088/1475-7516/2018/04/049	journal	April 2018
How proper are Bayesian models in the astronomical literature? Tak, Hyungsuk; Ghosh, Sujit K.; Ellis, Justin A. Monthly Notices of the Royal Astronomical Society, Vol. 481, Issue 1 https://doi.org/10.1093/mnras/sty2326	journal	August 2018
Sunyaev–Zel’dovich effect and X-ray scaling relations from weak lensing mass calibration of 32 South Pole Telescope selected galaxy clusters Dietrich, J. P.; Bocquet, S.; Schrabback, T. Monthly Notices of the Royal Astronomical Society, Vol. 483, Issue 3 https://doi.org/10.1093/mnras/sty3088	journal	December 2018
Dark Energy Survey Year 1 Results: redshift distributions of the weak-lensing source galaxies Hoyle, B.; Gruen, D.; Bernstein, G. M. Monthly Notices of the Royal Astronomical Society, Vol. 478, Issue 1 https://doi.org/10.1093/mnras/sty957	journal	April 2018
Exploring relations between BCG and cluster properties in the SPectroscopic IDentification of eROSITA Sources survey from 0.05 < 0.3 Furnell, Kate E.; Collins, Chris A.; Kelvin, Lee S. Monthly Notices of the Royal Astronomical Society, Vol. 478, Issue 4 https://doi.org/10.1093/mnras/sty991	journal	June 2018
Weak lensing analysis of codex clusters using dark energy camera legacy survey: mass–richness relation Phriksee, Anirut; Jullo, Eric; Limousin, Marceau Monthly Notices of the Royal Astronomical Society, Vol. 491, Issue 2 https://doi.org/10.1093/mnras/stz3049	journal	November 2019
Halo concentration, galaxy red fraction, and gas properties of optically defined merging clusters† Okabe, Nobuhiro; Oguri, Masamune; Akamatsu, Hiroki Publications of the Astronomical Society of Japan, Vol. 71, Issue 4 https://doi.org/10.1093/pasj/psz059	journal	July 2019
Halo Profiles and the Concentration–Mass Relation for a ΛCDM Universe Child, Hillary L.; Habib, Salman; Heitmann, Katrin The Astrophysical Journal, Vol. 859, Issue 1 https://doi.org/10.3847/1538-4357/aabf95	journal	May 2018
Dark Energy Survey Year 1 Results: Redshift distributions of the weak lensing source galaxies Hoyle, B.; Gruen, D.; Bernstein, G. M. arXiv https://doi.org/10.48550/arxiv.1708.01532	text	January 2017
Halo Concentration, Galaxy Red Fraction, and Gas Properties of Optically-defined Merging Clusters Okabe, Nobuhiro; Oguri, Masamune; Akamatsu, Hiroki arXiv https://doi.org/10.48550/arxiv.1812.07481	text	January 2018
The galaxy cluster mass scale and its impact on cosmological constraints from the cluster population Pratt, G. W.; Arnaud, M.; Biviano, A. arXiv https://doi.org/10.48550/arxiv.1902.10837	text	January 2019

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