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1. Identity statement
Reference TypeJournal Article
Sitemtc-m21d.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier8JMKD3MGP3W34T/47ERTR2
Repositorysid.inpe.br/mtc-m21d/2022/08.16.17.06
Last Update2022:08.16.17.06.00 (UTC) simone
Metadata Repositorysid.inpe.br/mtc-m21d/2022/08.16.17.06.01
Metadata Last Update2023:01.03.16.46.12 (UTC) administrator
DOI10.1051/0004-6361/202140886
ISSN0004-6361
1432-0746
Citation KeyLiccardoMWAABBQVPWCFFNSSRZDHLMV:2022:IVSiMi
TitleThe BINGO project: IV. Simulations for mission performance assessment and preliminary component separation steps
Year2022
MonthAug.
Access Date2024, May 14
Type of Workjournal article
Secondary TypePRE PI
Number of Files1
Size7448 KiB
2. Context
Author 1 Liccardo, Vincenzo
 2 Mericia, Eduardo Jubini de
 3 Wuensche, Carlos Alexandre
 4 Abdalla, Elcio
 5 Abdalla, Filipe B.
 6 Barosi, Luciano
 7 Brito, Francisco A.
 8 Queiroz, Amilcar
 9 Villela Neto, Thyrso
10 Peel, Michael W.
11 Wang, Bin
12 Costa, Andre A.
13 Ferreira, Elisa G. M.
14 Fornazier, Karin S. F.
15 Novaes, Camila Paiva
16 Santos, Larissa
17 Santos, Marcelo V. dos
18 Remazeilles, Mathieu
19 Zhang, Jiajun
20 Dickinson, Clive
21 Harper, Stuart
22 Landim, Ricardo G.
23 Marins, Alessandro
24 Vieira, Frederico Augusto Silva
Resume Identifier 1
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 9 8JMKD3MGP5W/3C9JJA6
Group 1 DIAST-CGCE-INPE-MCTI-GOV-BR
 2 AST-CEA-DIPGR-INPE-MCTI-GOV-BR
 3 DIAST-CGCE-INPE-MCTI-GOV-BR
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 9 DIAST-CGCE-INPE-MCTI-GOV-BR
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24 AST-CEA-DIPGR-INPE-MCTI-GOV-BR
Affiliation 1 Instituto Nacional de Pesquisas Espaciais (INPE)
 2 Instituto Nacional de Pesquisas Espaciais (INPE)
 3 Instituto Nacional de Pesquisas Espaciais (INPE)
 4 Universidade de São Paulo (USP)
 5 Universidade de São Paulo (USP)
 6 Universidade Federal de Campina Grande (UFCG)
 7 Universidade Federal de Campina Grande (UFCG)
 8 Universidade Federal de Campina Grande (UFCG)
 9 Instituto Nacional de Pesquisas Espaciais (INPE)
10 Instituto de Astrofísica de Canarias
11 Yangzhou University
12 Yangzhou University
13 Universidade de São Paulo (USP)
14 Universidade de São Paulo (USP)
15 Instituto Nacional de Pesquisas Espaciais (INPE)
16 Yangzhou University
17 Universidade Federal de Campina Grande (UFCG)
18 The University of Manchester
19 Institute for Basic Science (IBS)
20 The University of Manchester
21 The University of Manchester
22 Technische Universität München
23 Universidade de São Paulo (USP)
24 Instituto Nacional de Pesquisas Espaciais (INPE)
Author e-Mail Address 1 vic2000@hotmail.it
 2 ejubini@gmail.com
 3 cawuensche@gmail.com
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15 camilapnovaes@gmail.com
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24 fredsvieira@gmail.com
JournalAstronomy and Astrophysics
Volume664
PagesA17
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 17:06:01 :: simone -> administrator ::
2022-08-16 17:06:01 :: administrator -> simone :: 2022
2022-08-16 17:08:44 :: 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
AbstractAims. The large-scale distribution of neutral hydrogen (HI) in the Universe is luminous through its 21 cm emission. The goal of the Baryon Acoustic Oscillations from Integrated Neutral Gas Observations (BINGO) radio telescope is to detect baryon acoustic oscillations at radio frequencies through 21 cm intensity mapping (IM). The telescope will span the redshift range 0.127<z<0.449 with an instantaneous field-of-view of 14.75 - 6.0. Methods. In this work we investigate different constructive and operational scenarios of the instrument by generating sky maps as they would be produced by the instrument. In doing this we use a set of end-to-end IM mission simulations. The maps will additionally be used to evaluate the efficiency of a component separation method (GNILC). Results. We have simulated the kind of data that would be produced in a single-dish IM experiment such as BINGO. According to the results obtained, we have optimized the focal plane design of the telescope. In addition, the application of the GNILC method on simulated data shows that it is feasible to extract the cosmological signal across a wide range of multipoles and redshifts. The results are comparable with the standard principal component analysis method.
AreaCEA
Arrangement 1urlib.net > Produção pgr ATUAIS > AST > The BINGO project:...
Arrangement 2urlib.net > BDMCI > Fonds > Produção a partir de 2021 > CGCE > The BINGO project:...
doc Directory Contentaccess
source Directory Contentthere are no files
agreement Directory Content
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4. Conditions of access and use
data URLhttp://mtc-m21d.sid.inpe.br/ibi/8JMKD3MGP3W34T/47ERTR2
zipped data URLhttp://mtc-m21d.sid.inpe.br/zip/8JMKD3MGP3W34T/47ERTR2
Languageen
Target Fileaa40886-21.pdf
User Groupsimone
Reader Groupadministrator
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Visibilityshown
Archiving Policyallowpublisher allowfinaldraft
Update Permissionnot transferred
5. Allied materials
Next Higher Units8JMKD3MGPCW/3F2NE4L
8JMKD3MGPCW/46KTFK8
Citing Item Listsid.inpe.br/mtc-m21/2012/07.13.15.00.58 1
sid.inpe.br/bibdigital/2022/04.03.17.52 1
DisseminationWEBSCI; PORTALCAPES; COMPENDEX; SCOPUS.
Host Collectionurlib.net/www/2021/06.04.03.40
6. Notes
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