CCCP and MENeaCS: (updated) weak-lensing masses for 100 galaxy clusters

Herbonnet, Ricardo; Sifón, Cristóbal; Hoekstra, Henk; Bahé, Yannick; van der Burg, Remco F. J.; Melin, Jean-Baptiste; von der Linden, Anja; Sand, David; Kay, Scott; Barnes, David

doi:10.1093/mnras/staa2303

CCCP and MENeaCS: (updated) weak-lensing masses for 100 galaxy clusters

Journal Article · Wed Aug 05 00:00:00 EDT 2020 · Monthly Notices of the Royal Astronomical Society

DOI:https://doi.org/10.1093/mnras/staa2303· OSTI ID:1650396

Herbonnet, Ricardo ^[1]; Sifón, Cristóbal ^[2]; ^[3]; ^[3]; van der Burg, Remco F. J. ^[4]; Melin, Jean-Baptiste ^[5]; von der Linden, Anja ^[6]; Sand, David ^[7]; ^[8]; ^[9]

Department of Physics and Astronomy, Stony Brook University, Stony Brook, NY 11794, USA, Leiden Observatory, Leiden University, P.O. Box 9513, NL-2300 RA, Leiden, The Netherlands
Leiden Observatory, Leiden University, P.O. Box 9513, NL-2300 RA, Leiden, The Netherlands, Instituto de Física, Pontificia Universidad Católica de Valparaíso, Casilla 4059, Valparaíso, Chile
Leiden Observatory, Leiden University, P.O. Box 9513, NL-2300 RA, Leiden, The Netherlands
European Southern Observatory, Karl-Schwarzschild-Str. 2, D-85748, Garching, Germany
IRFU, CEA, Université Paris-Saclay, F-91191 Gif-sur-Yvette, France
Department of Physics and Astronomy, Stony Brook University, Stony Brook, NY 11794, USA
Department of Astronomy/Steward Observatory, 933 North Cherry Avenue, Rm. N204, Tucson, AZ 85721-0065, USA
Jodrell Bank Centre for Astrophysics, Department of Physics and Astronomy, The University of Manchester, Manchester M13 9PL, UK
Department of Physics, Kavli Institute for Astrophysics and Space Research, Massachusetts Institute of Technology, Cambridge, MA 02139, USA

ABSTRACT

Large area surveys continue to increase the samples of galaxy clusters that can be used to constrain cosmological parameters, provided that the masses of the clusters are measured robustly. To improve the calibration of cluster masses using weak gravitational lensing we present new results for 48 clusters at 0.05 < z < 0.15, observed as part of the Multi Epoch Nearby Cluster Survey, and re-evaluate the mass estimates for 52 clusters from the Canadian Cluster Comparison Project. Updated high-fidelity photometric redshift catalogues of reference deep fields are used in combination with advances in shape measurements and state-of-the-art cluster simulations, yielding an average systematic uncertainty in the lensing signal below 5 per cent, similar to the statistical uncertainty for our cluster sample. We derive a scaling relation with Planck measurements for the full sample and find a bias in the Planck masses of 1 − b = 0.84 ± 0.04 (stat) ±0.05 (syst). We find no statistically significant trend of the mass bias with redshift or cluster mass, but find that different selections could change the bias by up to 0.07. We find a gas fraction of 0.139 ± 0.014 (stat) for eight relaxed clusters in our sample, which can also be used to infer cosmological parameters.

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Research Organization:: State Univ. of New York (SUNY), Albany, NY (United States)

Sponsoring Organization:: European Research Council (ERC); National Science Foundation (NSF); USDOE; USDOE Office of Science (SC)

Grant/Contract Number:: SC0018053

OSTI ID:: 1650396

Alternate ID(s):: OSTI ID: 1852478

Journal Information:: Monthly Notices of the Royal Astronomical Society, Journal Name: Monthly Notices of the Royal Astronomical Society Journal Issue: 4 Vol. 497; ISSN 0035-8711

Publisher:: Oxford University PressCopyright Statement

Country of Publication:: United Kingdom

Language:: English

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