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|a (TOE)ost1766077
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|a (TOE)1766077
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|a E 1.99:SLAC-PUB-17589
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|a E 1.99:SLAC-PUB-17589
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|a SLAC-PUB-17589
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|a CODEX weak lensing mass catalogue and implications on the mass?richness relation
|h [electronic resource]
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|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.
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300 |
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|a Size: p. 1494-1526 :
|b digital, PDF file.
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|a text
|b txt
|2 rdacontent.
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|a computer
|b c
|2 rdamedia.
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|a online resource
|b cr
|2 rdacarrier.
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|a Published through Scitech Connect.
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|a 12/23/2020.
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|a "SLAC-PUB-17589."
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|a "Journal ID: ISSN 0035-8711."
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|a ": US2206288."
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|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.
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|a SLAC National Accelerator Lab., Menlo Park, CA (United States)
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|a Finnish Academy.
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|a Shanghai Committee of Science and Technology.
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|a Brazilian National Council for Scientific and Technological Development (CNPq)
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|a Coordination for the Improvement of Higher Education Personnel (CAPES)
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|a S?ao Paolo Research Foundation (FAPESP)
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|a Science and Technology Commission of Shanghai Municipality.
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|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 ?
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|b AC02-76SF00515.
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|b ST/N000919/1.
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|b 266918.
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|b 19ZR1466600.
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|b 292882.
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|a 79 astronomy and astrophysics
|2 local.
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|a Galaxy: clusters
|2 local.
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|a Cosmology: observations
|2 local.
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|a Gravitational lensing: weak
|2 local.
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|a 72 physics of elementary particles and fields
|2 local.
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|a Clusters of galaxies
|2 local.
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|a Dark energy
|2 local.
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|a Xray observations
|2 local.
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650 |
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7 |
|a Gravitational lensing
|2 local.
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650 |
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7 |
|a Astronomy and astrophysics
|2 local.
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|a Physics of elementary particles and fields
|2 local.
|
650 |
|
7 |
|a X-ray observations
|2 local.
|
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1 |
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|a United States.
|b Department of Energy.
|b Office of Science.
|4 spn.
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710 |
2 |
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|a Science and Technology Facilities Council (Great Britain).
|4 spn.
|
710 |
1 |
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|a United States.
|b Department of Energy.
|b Office of High Energy Physics.
|4 spn.
|
710 |
1 |
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|a United States.
|b Department of Energy.
|4 spn.
|
710 |
2 |
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|a Stanford Linear Accelerator Center.
|f res.
|
710 |
1 |
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|a United States.
|b Department of Energy.
|b Office of Scientific and Technical Information
|4 dst.
|
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|u https://www.osti.gov/servlets/purl/1766077
|z Full Text (via OSTI)
|
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|a .b128273690
|b 02-28-23
|c 12-08-22
|
998 |
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|a web
|b 12-08-22
|c f
|d m
|e p
|f eng
|g
|h 0
|i 1
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|a Information bridge
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|i 5a5e7f79-dfbc-56d6-a6d8-efff762519dc
|s 7e84132f-819e-55a9-ad71-18b612b49824
|
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f |
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|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
|