About: Virial Scaling of Massive Dark Matter Halos: Why Clusters Prefer a High Normalization Cosmology

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scientific article published in the Astrophysical Journal

Attributes	Values
rdf:type	Item
description	artículu científicu (ast) wetenschappelijk artikel (nl) наукова стаття, опублікована в січні 2008 (uk) im Januar 2008 veröffentlichter wissenschaftlicher Artikel (de) article publié dans la revue scientifique Astrophysical Journal (fr) scientific article published in the Astrophysical Journal (en)
publication date	wds:Q57630828-6DFD5223-C317-45E1-85EF-F6A5DEEFE85A
publication date	2008-01-01 00:00:00Z (xsd:dateTime)
language of work or name	wds:Q57630828-B40B9AE6-2E60-49A8-A2B3-43A5AC520B8C
language of work or name	English
author name string	wds:Q57630828-144FD921-898E-43A7-90D2-154412398D17 wds:Q57630828-373C7C13-2CC1-4ABF-B37F-37FEDC55BFF8 wds:Q57630828-42FF6D31-8104-4A49-B60E-A722545AEA82 wds:Q57630828-50CE1364-9BA0-42DD-9E9F-A1DA0C8BADF6 wds:Q57630828-669EE978-92AC-4EA7-B3B9-D74079144800 wds:Q57630828-88845293-AC9B-47C3-89F9-2DEF7555C4BB wds:Q57630828-8B04E9A0-571B-48E8-9661-F46BC6986FD2 wds:Q57630828-B626837E-A066-4646-9F8E-5857BE64A3FF wds:Q57630828-F76FCF6C-7F52-4B9F-93AD-5F1DF77D5140 wds:Q57630828-FFA7CA3B-D42F-44D2-9BC8-7D895D55B19B
author name string	S. Habib L. Gao M. Warren A. E. Evrard S. D. M. White J. Bialek J. Diemand A. R. Jenkins K. Heitmann M. Busha
rdfs:label	Virial Scaling of Massive Dark Matter Halos: Why Clusters Prefer a High Normalization Cosmology (en) Virial Scaling of Massive Dark Matter Halos: Why Clusters Prefer a High Normalization Cosmology (nl)
skos:prefLabel	Virial Scaling of Massive Dark Matter Halos: Why Clusters Prefer a High Normalization Cosmology (en) Virial Scaling of Massive Dark Matter Halos: Why Clusters Prefer a High Normalization Cosmology (nl)
name	Virial Scaling of Massive Dark Matter Halos: Why Clusters Prefer a High Normalization Cosmology (en) Virial Scaling of Massive Dark Matter Halos: Why Clusters Prefer a High Normalization Cosmology (nl)
author	wds:Q57630828-08AFEE8C-FD57-4747-A5C3-5BD9800EE550 wds:Q57630828-0C727646-BB4E-4293-BEEB-1C4607159D88 wds:Q57630828-0F626DF6-738B-4509-85D2-33992AC12BBB wds:Q57630828-2F0F08F6-734A-4FA3-8845-4E30DF5A64F7 wds:Q57630828-52F034C9-21AD-4918-8B1B-FAC52FB005FE wds:Q57630828-6B6A6BE2-1EA9-4998-B461-B8143024392C wds:Q57630828-71126167-E1F6-43C1-B358-F52EB1512436 wds:Q57630828-C521678A-5234-4E96-99EB-34B06759BBF0
author	Carlos Frenk Lauro Moscardini Chris Power Giuseppe Tormen Elena Rasia Martin White Volker Springel Adrian Jenkins
title	wds:Q57630828-C4D5CB30-C07A-4A5F-A967-E550E9FC4553
title	Virial Scaling of Massive Dark Matter Halos: Why Clusters Prefer a High Normalization Cosmology (en)
page(s)	wds:Q57630828-B177A3A5-59C5-4632-B817-6F0CBEBD0BAA
page(s)	122–137
instance of	wds:Q57630828-0E8988C9-45F4-41DE-B994-0EF802533A95
instance of	scholarly article
main subject	wds:Q57630828-AF1B0BF8-8858-4C83-A19C-497870C91C05 wds:Q57630828-DC5A654A-56D2-496C-AA78-D38DF1663E9E
main subject	dark matter cosmology
published in	wds:Q57630828-7FB77FE9-2FDE-495E-9DD8-EB1EDF600590
full work available at URL	wds:Q57630828-BD3F7D92-F112-496F-AB8E-C46DCC6A9BD6
published in	The Astrophysical Journal
full work available at URL	https://iopscience.iop.org/article/10.1086/521616/pdf
issue	wds:Q57630828-62563503-5716-4F92-BA53-EABE073F4BFF
volume	wds:Q57630828-6A6ED090-59C9-4819-A3E7-784DB6CB540E
issue	1
volume	672
DOI	wds:Q57630828-E78EE8AA-B940-44BE-A5BD-57969A5981EE
DOI	http://dx.doi.org/10.1086/521616
DOI	10.1086/521616
arXiv ID	wds:Q57630828-5CAB141B-D1CB-4C4E-917B-9E86CA70E9D3
arXiv ID	astro-ph/0702241
ADS bibcode	wds:Q57630828-159D2C34-4625-4690-BB65-C42E1B7BCACB
ADS bibcode	2008ApJ...672..122E
is about of	https://www.wikidata.org/wiki/Special:EntityData/Q57630828
is cites work of	Galaxy Cluster Mass Reconstruction Project – II. Quantifying scatter and bias using contrasting mock catalogues N-body dark matter haloes with simple hierarchical histories Hubble space telescope discovery of a z = 3.9 multiply imaged galaxy behind the complex cluster lens WARPS J1415.1+36 at z = 1.026 Virial scaling of galaxies in clusters: bright to faint is cool to hot A model for multiproperty galaxy cluster statistics The Atacama Cosmology Telescope: dynamical masses for 44 SZ-selected galaxy clusters over 755 square degrees Gravitational lensing detection of an extremely dense environment around a galaxy cluster Critical look at cosmological perturbation theory techniques SALT spectroscopic observations of galaxy clusters detected by ACT and a type II quasar hosted by a brightest cluster galaxy Dynamical analysis of galaxy cluster merger Abell 2146 A massive core for a cluster of galaxies at a redshift of 4.3. Space Creation Mechanism during the Expansion of Universe Galaxy cluster mass estimation from stacked spectroscopic analysis
is cites work of	wds:Q58915500-100C6842-F0DD-489C-903D-81EE7697AD7B wds:Q58919176-37570F2D-94B6-42C3-A91E-8B5DB22FA270 wds:Q57746460-4638B788-9611-4AA2-A216-CBE7FE44A18F wds:Q57630767-8B46D656-D671-4B2C-AE46-DC840D8FC0A2 wds:Q58831053-42EB8056-78A2-4516-B04F-AE4D4E8944A6 wds:Q56908110-B672B57A-4432-4B02-AD31-0797E4AA8287 wds:Q52562750-07E5230D-2847-4E26-836C-450CC6BA9F33 wds:Q58474410-9BAE9D8D-5E25-49C4-9FE6-06CA7AA190C5

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