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1. Identity statement
Reference TypeJournal Article
Siteplutao.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
IdentifierJ8LNKAN8RW/3D544BS
Repositorydpi.inpe.br/plutao/2012/11.28.18.58   (restricted access)
Last Update2013:01.23.12.31.42 (UTC) administrator
Metadata Repositorydpi.inpe.br/plutao/2012/11.28.18.58.22
Metadata Last Update2018:06.05.00.02.12 (UTC) administrator
Secondary KeyINPE--PRE/
DOI10.1088/0264-9381/29/20/205018
ISSN0264-9381
Labellattes: 2701172317925881 1 CostaTorr:2012:NeApSe
Citation KeyCostaTorr:2012:NeApSe
TitleThe critical coupling likelihood method: a new approach for seamless integration of environmental and operating conditions of gravitational wave detectors into gravitational wave searches
ProjectNSF grants (PHY-0905184 and PHY-0757058); CNPq (300001/2012-6)
Year2012
Access Date2024, Apr. 25
Secondary TypePRE PI
Number of Files1
Size1825 KiB
2. Context
Author1 Costa, César Augusto
2 Torres, Cristina V
Group1 DAS-CEA-INPE-MCTI-GOV-BR
Affiliation1 Instituto Nacional de Pesquisas Espaciais (INPE)
Author e-Mail Address1 cesar.costa@das.inpe.br
e-Mail Addresscesar.costa@das.inpe.br
JournalClassical and Quantum Gravity
Volume29
Number20
Pages205018
Secondary MarkB1_ASTRONOMIA_/_FÍSICA A2_ENGENHARIAS_I B1_ENGENHARIAS_IV C_ENSINO_DE_CIÊNCIAS_E_MATEMATICA A1_INTERDISCIPLINAR B1_MATEMÁTICA_/_PROBABILIDADE_E_ESTATÍSTICA
History (UTC)2012-11-28 23:06:35 :: lattes -> administrator :: 2012
2012-11-30 03:42:25 :: administrator -> marciana :: 2012
2013-01-23 12:31:42 :: marciana -> administrator :: 2012
2018-06-05 00:02:12 :: administrator -> marciana :: 2012
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
Version Typepublisher
Keywordsgravitational wave detectors and experiments
gravitational radiation detectors
mass spectromet
interferometers
gravitational waves
AbstractAny search effort for gravitationalwaves (GWs) using interferometric detectors like LIGO needs to be able to identify if and when noise couples into the detectors output signal. The critical coupling likelihood (CCL) method has been developed to characterize potential noise coupling and in the future aid GW search efforts. By testing two hypotheses about pairs of channels, CCL is able to identify undesirable coupled instrumental noise from potential GW candidates. Our preliminary results show that CCL can associate up to ∼80% of observed artifacts with SNR 8 with local noise sources, while reducing the duty cycle of the instrument by 15%. An approach like CCL will become increasingly important as GW research moves into the advanced LIGO era, going from the first GW detection to GW astronomy.
AreaCEA
Arrangementurlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDAS > The critical coupling...
doc Directory Contentaccess
source Directory Contentthere are no files
agreement Directory Contentthere are no files
4. Conditions of access and use
Languageen
Target File0264-9381_29_20_205018.pdf
User Groupadministrator
lattes
marciana
Visibilityshown
Archiving Policydenypublisher denyfinaldraft12
Read Permissiondeny from all and allow from 150.163
Update Permissionnot transferred
5. Allied materials
Next Higher Units8JMKD3MGPCW/3ETR8EH
DisseminationWEBSCI; PORTALCAPES; COMPENDEX.
Host Collectiondpi.inpe.br/plutao@80/2008/08.19.15.01
6. Notes
NotesSetores de Atividade: Pesquisa e desenvolvimento científico.
Empty Fieldsalternatejournal archivist callnumber copyholder copyright creatorhistory descriptionlevel format isbn lineage mark mirrorrepository month nextedition orcid parameterlist parentrepositories previousedition previouslowerunit progress readergroup resumeid rightsholder schedulinginformation secondarydate session shorttitle sponsor subject tertiarymark tertiarytype typeofwork url
7. Description control
e-Mail (login)marciana
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