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Investigation of flat spectrum radio sources by the interplanetary scintillation method at 111 MHz

dc.contributor.authorAugusto, P.
dc.contributor.authorTyul`bashev, S. A.
dc.date.accessioned2010-05-31T14:42:18Z
dc.date.available2010-05-31T14:42:18Z
dc.date.issued2005
dc.description.abstractAbstract. Interplanetary scintillation observations of 48 of the 55 Augusto et al. (1998) flat spectrum radio sources were carried out at 111 MHz using the interplanetary scintillation method on the Large Phased Array (LPA) in Russia. Due to the large size of the LPA beam (1◦ × 0.5◦) a careful inspection of all possible confusion sources was made using extant large radio surveys: 37 of the 48 sources are not confused. We were able to estimate the scintillating flux densities of 13 sources, getting upper limits for the remaining 35. Gathering more or improving extant VLBI data on these sources might significantly improve our results. This proof-of-concept project tells us that compact (<1 ) flat spectrum radio sources show strong enough scintillations at 111 MHz to establish/constrain their spectra (low-frequency end). Key words. galaxies: general – galaxies: active – galaxies: quasars: generalpt
dc.identifier.citationAstronomy & Astrophysics, 439,(2005)
dc.identifier.issn963-972
dc.identifier.urihttp://hdl.handle.net/10400.13/26
dc.language.isoengpt
dc.publisherESOpt
dc.subjectGalaxiespt
dc.subjectQuasarspt
dc.subject.pt
dc.subjectCentro de Ciências Exatas e da Engenharia
dc.titleInvestigation of flat spectrum radio sources by the interplanetary scintillation method at 111 MHzpt
dc.typejournal article
dspace.entity.typePublication
oaire.citation.endPage279pt
oaire.citation.startPage275pt
oaire.citation.titleAstronomy & Astrophysics, 439pt
person.familyNameAugusto
person.givenNamePedro
person.identifier.ciencia-id1410-460D-54C9
person.identifier.orcid0000-0002-0353-832X
person.identifier.ridL-4677-2014
person.identifier.scopus-author-id55386609700
rcaap.rightsopenAccesspt
rcaap.typearticlept
relation.isAuthorOfPublication76fe7070-0dec-4495-9478-56844f9f879d
relation.isAuthorOfPublication.latestForDiscovery76fe7070-0dec-4495-9478-56844f9f879d

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