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1. Identity statement
Reference TypeJournal Article
Sitemtc-m21d.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier8JMKD3MGP3W34T/47ERLNS
Repositorysid.inpe.br/mtc-m21d/2022/08.16.15.40
Last Update2022:08.16.15.40.04 (UTC) simone
Metadata Repositorysid.inpe.br/mtc-m21d/2022/08.16.15.40.04
Metadata Last Update2023:01.03.16.46.12 (UTC) administrator
DOI10.1051/0004-6361/202140887
ISSN0004-6361
1432-0746
Citation KeyZhangMNACWZSXABBQVWFFMSSLL:2022:VIHIHa
TitleThe BINGO project: VI. HI halo occupation distribution and mock building
Year2022
MonthAug.
Access Date2024, May 13
Type of Workjournal article
Secondary TypePRE PI
Number of Files1
Size3450 KiB
2. Context
Author 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
Resume Identifier 1
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14 8JMKD3MGP5W/3C9JJA6
Group 1
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 3 DIAST-CGCE-INPE-MCTI-GOV-BR
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22 DIAST-CGCE-INPE-MCTI-GOV-BR
Affiliation 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)
Author e-Mail Address 1
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 3 camilapnovaes@gmail.com
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15 cawuensche@gmail.com
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22 vic2000@hotmail.it
JournalAstronomy and Astrophysics
Volume664
PagesA19
Secondary MarkA1_GEOCIÊNCIAS A1_ENGENHARIAS_III A2_MATEMÁTICA_/_PROBABILIDADE_E_ESTATÍSTICA A2_INTERDISCIPLINAR A2_ENGENHARIAS_IV A2_ASTRONOMIA_/_FÍSICA B2_ENSINO C_ENGENHARIAS_II
History (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
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
Version Typepublisher
KeywordsCosmology: observations
Methods: observational
Radio continuum: general
Telescopes
AbstractContext. 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.
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zipped data URLhttp://mtc-m21d.sid.inpe.br/zip/8JMKD3MGP3W34T/47ERLNS
Languageen
Target Fileaa40887-21.pdf
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Next Higher Units8JMKD3MGPCW/46KTFK8
Citing Item Listsid.inpe.br/mtc-m21/2012/07.13.15.00.58 2
DisseminationWEBSCI; PORTALCAPES; COMPENDEX; SCOPUS.
Host Collectionurlib.net/www/2021/06.04.03.40
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