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086 0 |a E 1.99:SLAC-PUB-17589 
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088 |a SLAC-PUB-17589 
245 0 0 |a CODEX weak lensing mass catalogue and implications on the mass?richness relation  |h [electronic resource] 
260 |a Washington, D.C. :  |b United States. Department of Energy. Office of Science ;  |a Oak Ridge, Tenn. :  |b Distributed by the Office of Scientific and Technical Information, U.S. Department of Energy,  |c 2020. 
300 |a Size: p. 1494-1526 :  |b digital, PDF file. 
336 |a text  |b txt  |2 rdacontent. 
337 |a computer  |b c  |2 rdamedia. 
338 |a online resource  |b cr  |2 rdacarrier. 
500 |a Published through Scitech Connect. 
500 |a 12/23/2020. 
500 |a "SLAC-PUB-17589." 
500 |a "Journal ID: ISSN 0035-8711." 
500 |a ": US2206288." 
500 |a Kiiveri, K. ; Gruen, D. ; Finoguenov, A. ; Erben, T. ; van Waerbeke, L. ; Rykoff, E. ; Miller, L. ; Hagstotz, S. ; Dupke, R. ; Patrick Henry, J. ; et al. 
500 |a SLAC National Accelerator Lab., Menlo Park, CA (United States) 
500 |a Finnish Academy. 
500 |a Shanghai Committee of Science and Technology. 
500 |a Brazilian National Council for Scientific and Technological Development (CNPq) 
500 |a Coordination for the Improvement of Higher Education Personnel (CAPES) 
500 |a S?ao Paolo Research Foundation (FAPESP) 
500 |a Science and Technology Commission of Shanghai Municipality. 
520 3 |a 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 ?, normalization ?, and scatter ?ln ? 
536 |b AC02-76SF00515. 
536 |b ST/N000919/1. 
536 |b 266918. 
536 |b 19ZR1466600. 
536 |b 292882. 
650 7 |a 79 astronomy and astrophysics  |2 local. 
650 7 |a Galaxy: clusters  |2 local. 
650 7 |a Cosmology: observations  |2 local. 
650 7 |a Gravitational lensing: weak  |2 local. 
650 7 |a 72 physics of elementary particles and fields  |2 local. 
650 7 |a Clusters of galaxies  |2 local. 
650 7 |a Dark energy  |2 local. 
650 7 |a Xray observations  |2 local. 
650 7 |a Gravitational lensing  |2 local. 
650 7 |a Astronomy and astrophysics  |2 local. 
650 7 |a Physics of elementary particles and fields  |2 local. 
650 7 |a X-ray observations  |2 local. 
710 1 |a United States.  |b Department of Energy.  |b Office of Science.  |4 spn. 
710 2 |a Science and Technology Facilities Council (Great Britain).  |4 spn. 
710 1 |a United States.  |b Department of Energy.  |b Office of High Energy Physics.  |4 spn. 
710 1 |a United States.  |b Department of Energy.  |4 spn. 
710 2 |a Stanford Linear Accelerator Center.  |f res. 
710 1 |a United States.  |b Department of Energy.  |b Office of Scientific and Technical Information  |4 dst. 
856 4 0 |u https://www.osti.gov/servlets/purl/1766077  |z Full Text (via OSTI) 
907 |a .b128273690  |b 02-28-23  |c 12-08-22 
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952 f f |p Can circulate  |a University of Colorado Boulder  |b Online  |c Online  |d Online  |e E 1.99:SLAC-PUB-17589  |h Superintendent of Documents classification  |i web  |n 1