1. Identificação | |
Tipo de Referência | Artigo em Revista Científica (Journal Article) |
Site | mtc-m21d.sid.inpe.br |
Código do Detentor | isadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S |
Identificador | 8JMKD3MGP3W34T/47ERLNS |
Repositório | sid.inpe.br/mtc-m21d/2022/08.16.15.40 |
Última Atualização | 2022:08.16.15.40.04 (UTC) simone |
Repositório de Metadados | sid.inpe.br/mtc-m21d/2022/08.16.15.40.04 |
Última Atualização dos Metadados | 2023:01.03.16.46.12 (UTC) administrator |
DOI | 10.1051/0004-6361/202140887 |
ISSN | 0004-6361 1432-0746 |
Chave de Citação | ZhangMNACWZSXABBQVWFFMSSLL:2022:VIHIHa |
Título | The BINGO project: VI. HI halo occupation distribution and mock building |
Ano | 2022 |
Mês | Aug. |
Data de Acesso | 01 maio 2024 |
Tipo de Trabalho | journal article |
Tipo Secundário | PRE PI |
Número de Arquivos | 1 |
Tamanho | 3450 KiB |
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2. Contextualização | |
Autor | 1 Zhang, Jiajun 2 Motta, Pablo 3 Novaes, Camila Paiva 4 Abdalla, Filipe B. 5 Costa, Andre A. 6 Wang, Bin 7 Zhu, Zhenghao 8 Shan, Chenxi 9 Xu, Haiguang 10 Abdalla, Elcio 11 Barosi, Luciano 12 Brito, Francisco A. 13 Queiroz, Amilcar 14 Villela Neto, Thyrso 15 Wuensche, Carlos Alexandre 16 Ferreira, Elisa G. M. 17 Fornazier, Karin S. F. 18 Marins, Alessandro 19 Santos, Larissa 20 Santos, Marcelo Vargas dos 21 Landim, Ricardo G. 22 Liccardo, Vincenzo |
Identificador de Curriculo | 1 2 3 4 5 6 7 8 9 10 11 12 13 14 8JMKD3MGP5W/3C9JJA6 |
Grupo | 1 2 3 DIAST-CGCE-INPE-MCTI-GOV-BR 4 5 6 7 8 9 10 11 12 13 14 DIAST-CGCE-INPE-MCTI-GOV-BR 15 DIAST-CGCE-INPE-MCTI-GOV-BR 16 17 18 19 20 21 22 DIAST-CGCE-INPE-MCTI-GOV-BR |
Afiliação | 1 Institute for Basic Science (IBS) 2 Universidade de São Paulo (USP) 3 Instituto Nacional de Pesquisas Espaciais (INPE) 4 Universidade de São Paulo (USP) 5 Yangzhou University 6 Yangzhou University 7 Shanghai Jiao Tong University 8 Shanghai Jiao Tong University 9 Shanghai Jiao Tong University 10 Universidade de São Paulo (USP) 11 Universidade Federal de Campina Grande (UFCG) 12 Universidade Federal de Campina Grande (UFCG) 13 Universidade Federal de Campina Grande (UFCG) 14 Instituto Nacional de Pesquisas Espaciais (INPE) 15 Instituto Nacional de Pesquisas Espaciais (INPE) 16 Universidade de São Paulo (USP) 17 Universidade de São Paulo (USP) 18 Universidade de São Paulo (USP) 19 Yangzhou University 20 Universidade Federal de Campina Grande (UFCG) 21 Technische Universität München 22 Instituto Nacional de Pesquisas Espaciais (INPE) |
Endereço de e-Mail do Autor | 1 2 3 camilapnovaes@gmail.com 4 5 6 7 8 9 10 11 12 13 14 15 cawuensche@gmail.com 16 17 18 19 20 21 22 vic2000@hotmail.it |
Revista | Astronomy and Astrophysics |
Volume | 664 |
Páginas | A19 |
Nota Secundária | A1_GEOCIÊNCIAS A1_ENGENHARIAS_III A2_MATEMÁTICA_/_PROBABILIDADE_E_ESTATÍSTICA A2_INTERDISCIPLINAR A2_ENGENHARIAS_IV A2_ASTRONOMIA_/_FÍSICA B2_ENSINO C_ENGENHARIAS_II |
Histórico (UTC) | 2022-08-16 15:40:04 :: simone -> administrator :: 2022-08-16 15:40:05 :: administrator -> simone :: 2022 2022-08-16 15:42:28 :: simone -> administrator :: 2022 2023-01-03 16:46:12 :: administrator -> simone :: 2022 |
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3. Conteúdo e estrutura | |
É a matriz ou uma cópia? | é a matriz |
Estágio do Conteúdo | concluido |
Transferível | 1 |
Tipo do Conteúdo | External Contribution |
Tipo de Versão | publisher |
Palavras-Chave | Cosmology: observations Methods: observational Radio continuum: general Telescopes |
Resumo | Context. BINGO (Baryon Acoustic Oscillations from Integrated Neutral Gas Observations) is a radio telescope designed to survey from 980 MHz to 1260 MHz, observe the neutral hydrogen (HI) 21 cm line, and detect the baryon acoustic oscillation signal with the intensity mapping technique. Here we present our method for generating mock maps of the 21 cm intensity mapping signal that cover the BINGO frequency range and related test results. Aims. We would like to employ N-body simulations to generate mock 21 cm intensity maps for BINGO and study the information contained in 21 cm intensity mapping observations about structure formation, HI distribution and HI mass-halo mass relation. Methods. We fit an HI mass-halo mass relation from the ELUCID semianalytical galaxy catalog and applied it to the Horizen Run 4 halo catalog to generate the 21 cm mock map, which is called HOD. We also applied the abundance-matching method and matched the Horizen Run 4 galaxy catalog with the HI mass function measured from ALFALFA, to generate the 21 cm mock map, which is called HAM. Results. We studied the angular power spectrum of the mock maps and the corresponding pixel histogram. The comparison of two different mock map generation methods (HOD and HAM) is presented. We provide the fitting formula of ΩHi, HI bias, and the lognormal fitting parameter of the maps, which can be used to generate similar maps. We discuss the possibility of measuring ΩHi and HI bias by comparing the angular power spectrum of the mock maps and the theoretical calculation. We also discuss the redshift space distortion effect, the nonlinear effect, and the bin size effect in the mock map. Conclusions. By comparing the angular power spectrum measured from two different types of mock maps and the theoretical calculation, we find that the theoretical calculation can only fit the mock result at large scales. At small scales, neither the linear calculation nor the halofit nonlinear calculation can provide an accurate fitting, which reflects our poor understanding of the nonlinear distribution of HI and its scale-dependent bias. We have found that the bias is highly sensitive to the method of populating HI in halos, which also means that we can place constraints on the HI distribution in halos by observing 21 cm intensity mapping. We also illustrate that only with thin frequency bins (such as 2 MHz), we can discriminate the Finger-of-God effect. All of our investigations using mocks provide useful guidance for our expectation of BINGO experiments and other 21 cm intensity mapping experiments. |
Área | CEA |
Arranjo | urlib.net > BDMCI > Fonds > Produção a partir de 2021 > CGCE > The BINGO project:... |
Conteúdo da Pasta doc | acessar |
Conteúdo da Pasta source | não têm arquivos |
Conteúdo da Pasta agreement | |
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4. Condições de acesso e uso | |
URL dos dados | http://urlib.net/ibi/8JMKD3MGP3W34T/47ERLNS |
URL dos dados zipados | http://urlib.net/zip/8JMKD3MGP3W34T/47ERLNS |
Idioma | en |
Arquivo Alvo | aa40887-21.pdf |
Grupo de Usuários | simone |
Grupo de Leitores | administrator simone |
Visibilidade | shown |
Política de Arquivamento | allowpublisher allowfinaldraft |
Permissão de Atualização | não transferida |
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5. Fontes relacionadas | |
Unidades Imediatamente Superiores | 8JMKD3MGPCW/46KTFK8 |
Lista de Itens Citando | sid.inpe.br/mtc-m21/2012/07.13.15.00.58 2 |
Divulgação | WEBSCI; PORTALCAPES; COMPENDEX; SCOPUS. |
Acervo Hospedeiro | urlib.net/www/2021/06.04.03.40 |
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6. Notas | |
Campos Vazios | alternatejournal archivist callnumber copyholder copyright creatorhistory descriptionlevel e-mailaddress format isbn label lineage mark mirrorrepository nextedition notes number orcid parameterlist parentrepositories previousedition previouslowerunit progress project readpermission rightsholder schedulinginformation secondarydate secondarykey session shorttitle sponsor subject tertiarymark tertiarytype url |
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7. Controle da descrição | |
e-Mail (login) | simone |
atualizar | |
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