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1. Identificação
Tipo de ReferênciaArtigo em Revista Científica (Journal Article)
Sitemtc-m21b.sid.inpe.br
Código do Detentorisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identificador8JMKD3MGP3W34P/3QL7HSP
Repositóriosid.inpe.br/mtc-m21b/2018/03.02.16.20
Última Atualização2018:05.03.13.04.23 (UTC) simone
Repositório de Metadadossid.inpe.br/mtc-m21b/2018/03.02.16.20.14
Última Atualização dos Metadados2019:01.14.17.05.24 (UTC) administrator
DOI10.1093/mnras/stx3241
ISSN0035-8711
1365-2966
Rótuloself-archiving-INPE-MCTIC-GOV-BR
Chave de CitaçãoOldWPGMSTBYCMSSCBPLS:2018:ImDySu
TítuloGalaxy cluster mass reconstruction project - III: the impact of dynamical substructure on cluster mass estimates
Ano2018
Data de Acesso09 maio 2024
Tipo de Trabalhojournal article
Tipo SecundárioPRE PI
Número de Arquivos1
Tamanho1027 KiB
2. Contextualização
Autor 1 Old, L.
 2 Wojtak, R.
 3 Pearce, F. R.
 4 Gray, M. E.
 5 Mamon, G. A.
 6 Sifón, C.
 7 Tempel, E.
 8 Biviano, A.
 9 Yee, H. K. C.
10 Carvalho, Reinaldo Ramos de
11 Müller, V.
12 Sepp, T.
13 Skibba, R. A.
14 Croton, D.
15 Bamford, S. P.
16 Power, C.
17 von der Linden, A.
18 Saro, A.
Identificador de Curriculo 1
 2
 3
 4
 5
 6
 7
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10 8JMKD3MGP5W/3C9JJ5B
Grupo 1
 2
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10 DIDAS-CGCEA-INPE-MCTIC-GOV-BR
Afiliação 1 University of Toronto
 2 Stanford University
 3 University of Nottingham
 4 University of Nottingham
 5 Sorbonne Universités
 6 Princeton University
 7 Leibniz-Institut für Astrophysik Potsdam (AIP)
 8 INAF-Osservatorio Astronomico di Trieste
 9 University of Toronto
10 Instituto Nacional de Pesquisas Espaciais (INPE)
11 Leibniz-Institut für Astrophysik Potsdam (AIP)
12 Tartu Observatory
13 University of California
14 Swinburne University of Technology
15 University of Nottingham
16 University of Western Australia
17 Stony Brook University
18 INAF-Osservatorio Astronomico di Trieste
Endereço de e-Mail do Autor 1
 2
 3
 4
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10 reinaldo.decarvalho@inpe.br
RevistaMonthly Notices of the Royal Astronomical Society
Volume475
Número1
Páginas853-866
Nota SecundáriaA1_QUÍMICA A1_INTERDISCIPLINAR A1_GEOCIÊNCIAS A1_ENGENHARIAS_III A2_MATEMÁTICA_/_PROBABILIDADE_E_ESTATÍSTICA A2_ASTRONOMIA_/_FÍSICA B2_ENSINO B5_ENGENHARIAS_IV
Histórico (UTC)2018-03-02 16:25:08 :: simone -> administrator :: 2018
2018-03-03 04:09:36 :: administrator -> simone :: 2018
2018-05-03 13:04:23 :: simone -> administrator :: 2018
2019-01-04 16:56:03 :: administrator -> simone :: 2018
2019-01-07 11:32:26 :: simone -> administrator :: 2018
2019-01-14 17:05:24 :: administrator -> simone :: 2018
3. Conteúdo e estrutura
É a matriz ou uma cópia?é a matriz
Estágio do Conteúdoconcluido
Transferível1
Tipo do ConteúdoExternal Contribution
Tipo de Versãopublisher
Palavras-ChaveCosmological parameters
Galaxies: Clusters: General
Galaxies: Groups: General
Galaxies: Haloes
Galaxies: Kinematics and dynamics
Large-scale structure of Universe
ResumoWith the advent of wide-field cosmological surveys, we are approaching samples of hundreds of thousands of galaxy clusters. While such large numbers will help reduce statistical uncertainties, the control of systematics in cluster masses is crucial. Here we examine the effects of an important source of systematic uncertainty in galaxy-based cluster mass estimation techniques: the presence of significant dynamical substructure. Dynamical substructure manifests as dynamically distinct subgroups in phase-space, indicating an 'unrelaxed' state. This issue affects around a quarter of clusters in a generally selected sample. We employ a set of mock clusters whose masses have been measured homogeneously with commonly used galaxy-based mass estimation techniques (kinematic, richness, caustic, radial methods). We use these to study how the relation between observationally estimated and true cluster mass depends on the presence of substructure, as identified by various popular diagnostics.We find that the scatter for an ensemble of clusters does not increase dramatically for clusters with dynamical substructure. However, we find a systematic bias for all methods, such that clusters with significant substructure have higher measured masses than their relaxed counterparts. This bias depends on cluster mass: the most massive clusters are largely unaffected by the presence of significant substructure, but masses are significantly overestimated for lower mass clusters, by ~10 per cent at 1014 and ≳20 per cent for ≲1013.5. The use of cluster samples with different levels of substructure can therefore bias certain cosmological parameters up to a level comparable to the typical uncertainties in current cosmological studies.
ÁreaCEA
Arranjourlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDAS > Galaxy cluster mass...
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4. Condições de acesso e uso
URL dos dadoshttp://urlib.net/ibi/8JMKD3MGP3W34P/3QL7HSP
URL dos dados zipadoshttp://urlib.net/zip/8JMKD3MGP3W34P/3QL7HSP
Idiomaen
Grupo de Usuáriossimone
Grupo de Leitoresadministrator
simone
Visibilidadeshown
Política de Arquivamentoallowpublisher allowfinaldraft
Permissão de Leituraallow from all
Permissão de Atualizaçãonão transferida
5. Fontes relacionadas
Unidades Imediatamente Superiores8JMKD3MGPCW/3ETR8EH
Lista de Itens Citandosid.inpe.br/mtc-m21/2012/07.13.14.58.48 1
DivulgaçãoWEBSCI; PORTALCAPES; MGA; COMPENDEX.
Acervo Hospedeirosid.inpe.br/mtc-m21b/2013/09.26.14.25.20
6. Notas
Campos Vaziosalternatejournal archivist callnumber copyholder copyright creatorhistory descriptionlevel e-mailaddress format isbn lineage mark mirrorrepository month nextedition notes orcid parameterlist parentrepositories previousedition previouslowerunit progress project rightsholder schedulinginformation secondarydate secondarykey session shorttitle sponsor subject targetfile tertiarymark tertiarytype url
7. Controle da descrição
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