Finding Extremely Compact Sources Using the ASKAP VAST Survey

dc.contributor.authorBignall, Hayley E.
dc.contributor.authorJauncey, David L.
dc.contributor.authorLovell, James E. J.
dc.contributor.authorOjha, Roopesh
dc.contributor.authorReynolds, Cormac
dc.date.accessioned2020-04-30T17:46:51Z
dc.date.available2020-04-30T17:46:51Z
dc.date.issued2010
dc.descriptionIVS 2010 General Meeting Proceedingsen_US
dc.description.abstractVLBI observations of intraday variable (IDV) quasars found in the MASIV (Micro-Arcsecond Scintillation-Induced Variability) 5 GHz VLA Survey of 500 flat-spectrum sources in the northern sky have shown that these sources are extremely compact, often unresolved, on milliarcsecond scales, and more core-dominated than their non-IDV counterparts. VAST: an ASKAP Survey for Variables and Slow Transients, proposes to observe 10,000 square degrees of southern sky daily for 2 years in the VAST-Wide survey component. This is expected to reveal of order 30,000 compact sources brighter than 10 mJy showing refractive interstellar scintillation (the cause of centimeter-wavelength IDV) at the survey frequency of about 1.4 GHz. Many of these sources may be suitable astrometric calibrators for VLBI at higher frequencies.en_US
dc.description.urihttps://ivscc.gsfc.nasa.gov/publications/gm2010/bignall.pdfen_US
dc.format.extent5 pagesen_US
dc.genreconference papers and proceedingsen_US
dc.identifierdoi:10.13016/m2nojq-mcgx
dc.identifier.citationBignall, Hayley E.; Jauncey, David L.; Lovell, James E. J.; Ojha, Roopesh; Reynolds, Cormac; Finding Extremely Compact Sources Using the ASKAP VAST Survey; IVS 2010 General Meeting Proceedings, p.325–329 (2010); https://ivscc.gsfc.nasa.gov/publications/gm2010/bignall.pdfen_US
dc.identifier.urihttp://hdl.handle.net/11603/18386
dc.language.isoen_USen_US
dc.publisherIVS Publicationsen_US
dc.relation.isAvailableAtThe University of Maryland, Baltimore County (UMBC)
dc.relation.ispartofUMBC Physics Department Collection
dc.relation.ispartofUMBC Center for Space Sciences and Technology (CSST) / Center for Research and Exploration in Space Sciences & Technology II (CRSST II)
dc.rightsThis item is likely protected under Title 17 of the U.S. Copyright Law. Unless on a Creative Commons license, for uses protected by Copyright Law, contact the copyright holder or the author.
dc.rightsPublic Domain Mark 1.0*
dc.rightsThis is a work of the United States Government. In accordance with 17 U.S.C. 105, no copyright protection is available for such works under U.S. Law.
dc.rights.urihttp://creativecommons.org/publicdomain/mark/1.0/*
dc.titleFinding Extremely Compact Sources Using the ASKAP VAST Surveyen_US
dc.typeTexten_US

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