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1. Identity statement
Reference TypeJournal Article
Sitemtc-m21c.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier8JMKD3MGP3W34R/44QANMB
Repositorysid.inpe.br/mtc-m21c/2021/06.02.12.51
Last Update2021:11.05.13.48.44 (UTC) simone
Metadata Repositorysid.inpe.br/mtc-m21c/2021/06.02.12.51.17
Metadata Last Update2022:04.03.19.24.45 (UTC) administrator
DOI10.1051/0004-6361/202039936
ISSN0004-6361
1432-0746
Citation KeyCarvalhoBerAviNovNog:2021:BAAnSc
TitleBAO angular scale at z eff= 0.11 with the SDSS blue galaxies
Year2021
MonthMay
Access Date2024, Apr. 25
Type of Workjournal article
Secondary TypePRE PI
Number of Files1
Size830 KiB
2. Context
Author1 Carvalho, Edilson de
2 Bernui, Armando
3 Avila, Felipe
4 Novaes, Camila Paiva
5 Nogueira Cavalcante, J. P.
ORCID1
2 0000-0003-3034-0762
Group1
2
3
4 DIAST-CGCE-INPE-MCTI-GOV-BR
Affiliation1 Universidade do Estado do Amazonas (UEA)
2 Observatório Nacional
3 Observatório Nacional
4 Instituto Nacional de Pesquisas Espaciais (INPE)
5 Observatório Nacional
Author e-Mail Address1
2
3
4 camilapnovaes@gmail.com
JournalAstronomy & Astrophysics
Volume649
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)2021-06-02 12:51:17 :: simone -> administrator ::
2021-06-02 12:51:18 :: administrator -> simone :: 2021
2021-06-02 12:52:45 :: simone -> administrator :: 2021
2021-07-28 23:02:28 :: administrator -> simone :: 2021
2021-11-05 13:48:44 :: simone -> administrator :: 2021
2022-04-03 19:24:45 :: administrator -> simone :: 2021
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
Version Typepublisher
KeywordsCosmological parameters
Cosmology: observations
Large-scale structure of Universe
AbstractAims. We measure the transverse baryon acoustic oscillations (BAO) signal in the local Universe using a sample of blue galaxies from the Sloan Digital Sky Survey (SDSS) survey as a cosmological tracer. Methods. The method is weakly dependent on a cosmological model and is suitable for 2D analyses in thin redshift bins to investigate the SDSS data in the interval z [0.105, 0.115]. Results. We detect the transverse BAO signal θBAO = 19.8°±1.05° at zeff = 0.11, with a statistical significance of 2.2σ. Additionally, we perform tests that confirm the robustness of this angular BAO signature. Supported by a large set of log-normal simulations, our error analyses include statistical and systematic contributions. In addition, considering the sound horizon scale calculated by the Planck Collaboration, rsPlanck, and the θBAO value obtained here, we obtain a measurement of the angular diameter distance DA(0.11) =258.31 ± 13.71 h-1 Mpc. Moreover, combining this θBAO measurement at low redshift with other BAO angular scale data reported in the literature, we perform statistical analyses for the cosmological parameters of some Lambda cold dark matter type models.
AreaCEA
Arrangementurlib.net > BDMCI > Fonds > Produção a partir de 2021 > CGCE > BAO angular scale...
doc Directory Contentaccess
source Directory Contentthere are no files
agreement Directory Content
agreement.html 02/06/2021 09:51 1.0 KiB 
4. Conditions of access and use
data URLhttp://urlib.net/ibi/8JMKD3MGP3W34R/44QANMB
zipped data URLhttp://urlib.net/zip/8JMKD3MGP3W34R/44QANMB
Languageen
Target Filecarvalho_bao.pdf
User Groupsimone
Reader Groupadministrator
simone
Visibilityshown
Archiving Policyallowpublisher allowfinaldraft
Update Permissionnot transferred
5. Allied materials
Next Higher Units8JMKD3MGPCW/46KTFK8
DisseminationWEBSCI; PORTALCAPES; MGA; COMPENDEX.
Host Collectionurlib.net/www/2017/11.22.19.04
6. Notes
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