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1. Identity statement
Reference TypeBook Section
Sitemtc-m16b.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier6qtX3pFwXQZGivnK2Y/NoV8z
Repositorysid.inpe.br/mtc-m17@80/2006/12.08.12.08   (restricted access)
Last Update2017:01.09.15.22.01 (UTC) marciana
Metadata Repositorysid.inpe.br/mtc-m17@80/2006/12.08.12.08.04
Metadata Last Update2018:06.05.03.44.21 (UTC) administrator
Secondary KeyINPE--/
ISBN0-7354-0332-5
Citation KeyDAmicoJabRodCieHic:2006:SeInCo
TitleSearch for an Infrared Counterpart of IGR J16358-4756
Year2006
Access Date2024, May 08
Secondary TypePRE LI
Number of Files1
Size2054 KiB
2. Context
Author1 D' Amico, Flávio
2 Jablonski, Francisco José
3 Rodrigues, Cláudia Vilega
4 Cieslinski, Deonísio
5 Hickel, Gabriel
Group1 DAS-INPE-MCT-BR
2 DAS-INPE-MCT-BR
3 DAS-INPE-MCT-BR
4 DAS-INPE-MCT-BR
Affiliation1 Instituto Nacional de Pesquisas Espaciais (INPE)
2 Instituto Nacional de Pesquisas Espaciais (INPE)
3 Instituto Nacional de Pesquisas Espaciais (INPE)
4 Instituto Nacional de Pesquisas Espaciais (INPE)
5 Universidade do Vale do Paraíba (UNIVAP)
EditorBraga, João
D'Amico, Flávio
Rothschild, Ricard E.
Book TitleThe transient milk way: a perspective for mirax
PublisherAmerican Institute of Physics
Volume840
Pages97-101
Series TitleAIP Conference Proceedings
History (UTC)2006-12-08 12:08:04 :: simone -> administrator ::
2012-10-22 21:02:08 :: administrator -> simone ::
2013-02-20 15:19:55 :: simone -> administrator :: 2006
2013-10-01 01:06:32 :: administrator -> marciana :: 2006
2017-01-09 15:22:01 :: marciana -> administrator :: 2006
2018-06-05 03:44:21 :: administrator -> simone :: 2006
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
KeywordsInfrared imaging
near infrared observations
x-ray binaries
AbstractWe report here on near infrared observations of the field around IGR J16358-4726. The source belongs to the new class of highly absorbed X-ray binaries discovered by IBIS/INTEGRAL. Our primary goal was to identify the infrared counterpart of the source, previously suggested to be a LMXB and then further reclassified as a HMXB. We have made use of Chandra observations of the source in order to better constrain the number of possible counterparts. Using the differential photometry technique, in observations spanning a timescale of 1 month, we found no long term variability in our observations. This is compatible, and we suggest here, that the source is a HMXB.
AreaCEA
Arrangementurlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDAS > Search for an...
doc Directory Contentaccess
source Directory Contentthere are no files
agreement Directory Contentthere are no files
4. Conditions of access and use
Languageen
Target Filedamico_search.pdf
User Groupadministrator
simone
Visibilityshown
Read Permissiondeny from all and allow from 150.163
Update Permissionnot transferred
5. Allied materials
Next Higher Units8JMKD3MGPCW/3ETR8EH
DisseminationNTRSNASA; BNDEPOSITOLEGAL.
Host Collectioncptec.inpe.br/walmeida/2003/04.25.17.12
6. Notes
Empty Fieldsarchivingpolicy archivist callnumber city copyholder copyright creatorhistory descriptionlevel doi e-mailaddress edition electronicmailaddress format issn label lineage mark mirrorrepository nextedition notes numberofvolumes orcid parameterlist parentrepositories previousedition previouslowerunit progress project readergroup resumeid rightsholder schedulinginformation secondarydate secondarymark serieseditor session shorttitle sponsor subject tertiarymark tertiarytype translator url versiontype
7. Description control
e-Mail (login)simone
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