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1. Identity statement
Reference TypeJournal Article
Sitemtc-m21c.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier8JMKD3MGP3W34R/3UHRN3L
Repositorysid.inpe.br/mtc-m21c/2019/12.12.15.57   (restricted access)
Last Update2019:12.12.15.57.03 (UTC) simone
Metadata Repositorysid.inpe.br/mtc-m21c/2019/12.12.15.57.03
Metadata Last Update2021:07.28.22.22.42 (UTC) administrator
DOI10.1088/1742-6596/1269/1/012002
ISSN1742-6588
Citation KeyWuensche:2019:NeInEx
TitleThe BINGO telescope: a new instrument exploring the new 21 cosmology window
Year2019
Access Date2024, May 17
Type of Workconference paper
Secondary TypePRE PI
Number of Files1
Size3344 KiB
2. Context
AuthorWuensche, Carlos Alexandre
GroupDIDAS-CGCEA-INPE-MCTIC-GOV-BR
AffiliationInstituto Nacional de Pesquisas Espaciais (INPE)
Author e-Mail Addressca.wuensche@inpe.br
JournalJournal of Physics: Conference Series
Volume1269
Pagese012002
Secondary MarkB2_INTERDISCIPLINAR B2_ENGENHARIAS_III B3_MEDICINA_II B3_GEOCIÊNCIAS B4_MATERIAIS B4_ENGENHARIAS_II B4_BIOTECNOLOGIA C_QUÍMICA C_MATEMÁTICA_/_PROBABILIDADE_E_ESTATÍSTICA C_ENGENHARIAS_IV C_ECONOMIA C_ASTRONOMIA_/_FÍSICA
History (UTC)2019-12-12 15:57:04 :: simone -> administrator ::
2019-12-12 15:57:04 :: administrator -> simone :: 2019
2019-12-12 15:57:14 :: simone -> administrator :: 2019
2021-07-28 22:22:42 :: administrator -> simone :: 2019
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
Version Typepublisher
AbstractBINGO is a unique radio telescope designed to make the first detection of Baryon Acoustic Oscillations (BAO) at radio frequencies. This will be achieved by measuring the distribution of neutral hydrogen gas at cosmological distances using a technique called Intensity Mapping. Along with the Cosmic Microwave Background anisotropies, the scale of BAO is one of the most powerful probes of cosmological parameters, including dark energy. The telescope will be built in a very low RFI site in South America and will operate in the frequency range from 0.96 GHz to 1.26 GHz. The telescope design consists of two ∼ 40-m compact mirrors with no moving parts. Such a design will give the excellent polarization performance and very low sidelobe levels required for intensity mapping. With a feedhorn array of 50 receivers, it will map a 15◦ declination strip as the sky drifts past the field-of-view of the telescope. The BINGO consortium is composed Universidade de Sao Paulo, Instituto Nacional de Pesquisas Espaciais (Brazil), University of Manchester and University College London (United Kingdom), ETH Z¨urich (Switzerland) and Universidad de La Republica (Uruguay). The telescope assembly and horn design and fabrication are under way in Brazil. The receiver was designed in UK and will be developed in Brazil, with most of the components for the receiver will also be supplied by Brazilian industry. The experience and science goals achieved by the BINGO team will be advantageous as a pathfinder mission for the Square Kilometre Array (SKA) project. This paper reports the current status of the BINGO mission, as well as preliminary results already obtained for the instrumentation development.
AreaCEA
Arrangementurlib.net > BDMCI > DIDAS > The BINGO telescope:...
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4. Conditions of access and use
Languageen
Target Filewuensche_bingo.pdf
User Groupsimone
Reader Groupadministrator
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Visibilityshown
Archiving Policydenypublisher denyfinaldraft12
Read Permissiondeny from all and allow from 150.163
Update Permissionnot transferred
5. Allied materials
Mirror Repositoryurlib.net/www/2017/11.22.19.04.03
Next Higher Units8JMKD3MGPCW/3ETR8EH
Citing Item Listsid.inpe.br/bibdigital/2013/10.01.00.07 1
DisseminationWEBSCI; PORTALCAPES; COMPENDEX.
Host Collectionurlib.net/www/2017/11.22.19.04
6. Notes
NotesFourth Algerian Conference on Astronomy and Astrophysics, 2017
Empty Fieldsalternatejournal archivist callnumber copyholder copyright creatorhistory descriptionlevel e-mailaddress format isbn keywords label lineage mark month nextedition number orcid parameterlist parentrepositories previousedition previouslowerunit progress project resumeid rightsholder schedulinginformation secondarydate secondarykey session shorttitle sponsor subject tertiarymark tertiarytype url
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