The MicroArcsecond Scintillation-Induced Variability (MASIV) Survey: Detection of Angular Broadening at High Redshift?
dc.contributor.author | Pursimo, T. | |
dc.contributor.author | Ojha, R. | |
dc.contributor.author | Jauncey, D. | |
dc.contributor.author | Lovell, J. | |
dc.contributor.author | Dutka, M. | |
dc.contributor.author | Bignall, H. | |
dc.contributor.author | Macquart, J.-P. | |
dc.contributor.author | Rickett, B. | |
dc.contributor.author | Kedziora-Chudczer, L. | |
dc.date.accessioned | 2020-03-10T15:46:34Z | |
dc.date.available | 2020-03-10T15:46:34Z | |
dc.date.issued | 2008 | |
dc.description | Extragalactic Jets: Theory and Observation from Radio to Gamma Ray ASP Conference Series, Vol. 386, © 2008 T. A. Rector and D. S. De Young, eds. | en_US |
dc.description.abstract | Interstellar scintillation has been shown to be primarily responsible for intra-day variability exhibited by extragalactic sources at centimeter wavelengths. The recent MASIV survey has shown that a very high proportion of flat spectrum extragalactic radio sources scintillate; such behaviour is both too common and too important to ignore. A study of the physical properties of the MASIV objects is severely handicapped by the absence of reliable redshift measurements for most of the objects. We present the first results of the studies of the physical properties of the MASIV sources, based on archival and our own redshift measurements. | en_US |
dc.description.sponsorship | RO acknowledges the Access to Major Research Facilities Program (AMRFP) of the Australian Government for travel support (Grant Number: 05/06-0-04) for observations with the Nordic Optical Telescope (NOT) during July 2005. | en_US |
dc.description.uri | http://aspbooks.org/publications/386/517.pdf | en_US |
dc.format.extent | 5 pages | en_US |
dc.genre | conference papers and proceedings | en_US |
dc.identifier | doi:10.13016/m2cxfp-pmmt | |
dc.identifier.citation | Pursimo, T.; Ojha, R.; Jauncey, D.; Lovell, J.; Dutka, M.; Bignall, H.; Macquart, J.-P.; Rickett, B.; Kedziora-Chudczer, L.; The MicroArcsecond Scintillation-Induced Variability (MASIV) Survey: Detection of Angular Broadening at High Redshift?; Extragalactic Jets: Theory and Observation from Radio to Gamma Ray (2008); http://aspbooks.org/publications/386/517.pdf | en_US |
dc.identifier.uri | http://hdl.handle.net/11603/17521 | |
dc.language.iso | en_US | en_US |
dc.publisher | Astronomical Society of the Pacific | en_US |
dc.relation.isAvailableAt | The University of Maryland, Baltimore County (UMBC) | |
dc.relation.ispartof | UMBC Physics Department Collection | |
dc.relation.ispartof | UMBC Center for Space Sciences and Technology (CSST) / Center for Research and Exploration in Space Sciences & Technology II (CRSST II) | |
dc.rights | This 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.subject | interstellar scintillation | en_US |
dc.subject | intra-day variability exhibited by extragalactic sources at centimeter wavelengths | en_US |
dc.subject | extragalactic sources | en_US |
dc.subject | MASIV survey | en_US |
dc.subject | physical properties of the MASIV sources | en_US |
dc.subject | redshift measurements | en_US |
dc.title | The MicroArcsecond Scintillation-Induced Variability (MASIV) Survey: Detection of Angular Broadening at High Redshift? | en_US |
dc.type | Text | en_US |
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