FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W2038386635> ?p ?o ?g. }

• W2038386635 abstract "Abstract The submillimeter universe has now been explored with the Submillimeter Common User Bolometer Array (SCUBA) camera on the James Clerk Maxwell Telescope, and claims have been made to the presence of a new population of optically unidentified starforming dusty galaxies at high redshifts. An alternative interpretation of the submillimeter (submm) emission from these sources, however, is that their far infrared emission is due to the presence of an active galactic nucleus (AGN) enshrouded by dust. Using examples of submm sources, selected primarily due to the availability of multiwavelength observations, we investigate whether the spectral energy distribution (SED) selected sources is consistent with either the dusty starforming or dusty AGN scenarios. Among these sources, we find that the SED of HDF850.4, one of the sources detected in the Hubble Deep Field (HDF), and CFRS14F, one of the sources in the Canada France Redshift Survey Fields, are fully consistent with the dusty starformation hypothesis, while the SED of APM 08279+5255 is consistent with a dusty AGN. For some submm sources, it is suggested that observations at rest wavelengths between ∼1 μm and 100 μm may be needed to differentiate between the dusty starformation and dusty AGN scenarios. We discuss implications of our results for the interpretation of submm sources and suggest that dusty AGNs can contribute up to ∼30% of the submm source counts. However, an exact observational determination on the ratio of dusty star-forming to dusty AGN contribution to submm counts require detailed followup observations of a flux limited source catalog, beyond what is currently available." @default.
• W2038386635 created "2016-06-24" @default.
• W2038386635 creator A5072280155 @default.
• W2038386635 date "1999-08-01" @default.
• W2038386635 modified "2023-09-27" @default.
• W2038386635 title "Spectral energy distribution of submillimeter sources" @default.
• W2038386635 cites W1484400061 @default.
• W2038386635 cites W1545676728 @default.
• W2038386635 cites W1607434071 @default.
• W2038386635 cites W1620896033 @default.
• W2038386635 cites W1666786580 @default.
• W2038386635 cites W1674586338 @default.
• W2038386635 cites W1681063222 @default.
• W2038386635 cites W1841113251 @default.
• W2038386635 cites W1858079601 @default.
• W2038386635 cites W1965372241 @default.
• W2038386635 cites W1966519460 @default.
• W2038386635 cites W1973808059 @default.
• W2038386635 cites W1974315100 @default.
• W2038386635 cites W1982057427 @default.
• W2038386635 cites W1994703407 @default.
• W2038386635 cites W2007442140 @default.
• W2038386635 cites W2014260104 @default.
• W2038386635 cites W2017100570 @default.
• W2038386635 cites W2020827391 @default.
• W2038386635 cites W2024995063 @default.
• W2038386635 cites W2044872435 @default.
• W2038386635 cites W2045848632 @default.
• W2038386635 cites W2047503612 @default.
• W2038386635 cites W2049506246 @default.
• W2038386635 cites W2050874569 @default.
• W2038386635 cites W2053267081 @default.
• W2038386635 cites W2065761316 @default.
• W2038386635 cites W2073285288 @default.
• W2038386635 cites W2084461662 @default.
• W2038386635 cites W2110294314 @default.
• W2038386635 cites W2117629212 @default.
• W2038386635 cites W2131382718 @default.
• W2038386635 cites W2155122056 @default.
• W2038386635 cites W2156255672 @default.
• W2038386635 cites W2161105816 @default.
• W2038386635 cites W2951408172 @default.
• W2038386635 cites W3005696757 @default.
• W2038386635 cites W3100294349 @default.
• W2038386635 cites W3100762759 @default.
• W2038386635 cites W3101388854 @default.
• W2038386635 cites W3101999519 @default.
• W2038386635 cites W3106403556 @default.
• W2038386635 cites W3125598333 @default.
• W2038386635 doi "https://doi.org/10.1016/s1384-1076(99)00030-5" @default.
• W2038386635 hasPublicationYear "1999" @default.
• W2038386635 type Work @default.
• W2038386635 sameAs 2038386635 @default.
• W2038386635 citedByCount "3" @default.
• W2038386635 crossrefType "journal-article" @default.
• W2038386635 hasAuthorship W2038386635A5072280155 @default.
• W2038386635 hasConcept C121332964 @default.
• W2038386635 hasConcept C125857072 @default.
• W2038386635 hasConcept C1276947 @default.
• W2038386635 hasConcept C133971210 @default.
• W2038386635 hasConcept C144024400 @default.
• W2038386635 hasConcept C149923435 @default.
• W2038386635 hasConcept C191897082 @default.
• W2038386635 hasConcept C192562407 @default.
• W2038386635 hasConcept C2778716715 @default.
• W2038386635 hasConcept C2780974285 @default.
• W2038386635 hasConcept C2908647359 @default.
• W2038386635 hasConcept C33024259 @default.
• W2038386635 hasConcept C43481613 @default.
• W2038386635 hasConcept C44870925 @default.
• W2038386635 hasConcept C50425793 @default.
• W2038386635 hasConcept C68709404 @default.
• W2038386635 hasConcept C98444146 @default.
• W2038386635 hasConceptScore W2038386635C121332964 @default.
• W2038386635 hasConceptScore W2038386635C125857072 @default.
• W2038386635 hasConceptScore W2038386635C1276947 @default.
• W2038386635 hasConceptScore W2038386635C133971210 @default.
• W2038386635 hasConceptScore W2038386635C144024400 @default.
• W2038386635 hasConceptScore W2038386635C149923435 @default.
• W2038386635 hasConceptScore W2038386635C191897082 @default.
• W2038386635 hasConceptScore W2038386635C192562407 @default.
• W2038386635 hasConceptScore W2038386635C2778716715 @default.
• W2038386635 hasConceptScore W2038386635C2780974285 @default.
• W2038386635 hasConceptScore W2038386635C2908647359 @default.
• W2038386635 hasConceptScore W2038386635C33024259 @default.
• W2038386635 hasConceptScore W2038386635C43481613 @default.
• W2038386635 hasConceptScore W2038386635C44870925 @default.
• W2038386635 hasConceptScore W2038386635C50425793 @default.
• W2038386635 hasConceptScore W2038386635C68709404 @default.
• W2038386635 hasConceptScore W2038386635C98444146 @default.
• W2038386635 hasLocation W20383866351 @default.
• W2038386635 hasOpenAccess W2038386635 @default.
• W2038386635 hasPrimaryLocation W20383866351 @default.
• W2038386635 hasRelatedWork W1437991842 @default.
• W2038386635 hasRelatedWork W1500722571 @default.
• W2038386635 hasRelatedWork W1646465061 @default.
• W2038386635 hasRelatedWork W1829347215 @default.
• W2038386635 hasRelatedWork W1979729838 @default.
• W2038386635 hasRelatedWork W2058152646 @default.
• W2038386635 hasRelatedWork W2089602737 @default.

• next