The MicroArcsecond Scintillation-Induced Variability (MASIV) Survey: Detection of Angular Broadening at High Redshift?

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...

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Main Authors: Pursimo, T., Ojha, R., Jauncey, J., Lovell, J., Dutka, M., Bignall, Hayley, Macquart, Jean-Pierre, rickett, B., Kedziora-Chudczer, L.
Other Authors: Travis A. Rector
Format: Conference Paper
Published: Astronomical Society of the Pacific 2008
Online Access:http://hdl.handle.net/20.500.11937/24880
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author Pursimo, T.
Ojha, R.
Jauncey, J.
Lovell, J.
Dutka, M.
Bignall, Hayley
Macquart, Jean-Pierre
rickett, B.
Kedziora-Chudczer, L.
author2 Travis A. Rector
author_facet Travis A. Rector
Pursimo, T.
Ojha, R.
Jauncey, J.
Lovell, J.
Dutka, M.
Bignall, Hayley
Macquart, Jean-Pierre
rickett, B.
Kedziora-Chudczer, L.
author_sort Pursimo, T.
building Curtin Institutional Repository
collection Online Access
description 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.
first_indexed 2025-11-14T07:54:32Z
format Conference Paper
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institution Curtin University Malaysia
institution_category Local University
last_indexed 2025-11-14T07:54:32Z
publishDate 2008
publisher Astronomical Society of the Pacific
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spelling curtin-20.500.11937-248802022-11-21T06:47:06Z The MicroArcsecond Scintillation-Induced Variability (MASIV) Survey: Detection of Angular Broadening at High Redshift? Pursimo, T. Ojha, R. Jauncey, J. Lovell, J. Dutka, M. Bignall, Hayley Macquart, Jean-Pierre rickett, B. Kedziora-Chudczer, L. Travis A. Rector David S. De Young 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. 2008 Conference Paper http://hdl.handle.net/20.500.11937/24880 Astronomical Society of the Pacific restricted
spellingShingle Pursimo, T.
Ojha, R.
Jauncey, J.
Lovell, J.
Dutka, M.
Bignall, Hayley
Macquart, Jean-Pierre
rickett, B.
Kedziora-Chudczer, L.
The MicroArcsecond Scintillation-Induced Variability (MASIV) Survey: Detection of Angular Broadening at High Redshift?
title The MicroArcsecond Scintillation-Induced Variability (MASIV) Survey: Detection of Angular Broadening at High Redshift?
title_full The MicroArcsecond Scintillation-Induced Variability (MASIV) Survey: Detection of Angular Broadening at High Redshift?
title_fullStr The MicroArcsecond Scintillation-Induced Variability (MASIV) Survey: Detection of Angular Broadening at High Redshift?
title_full_unstemmed The MicroArcsecond Scintillation-Induced Variability (MASIV) Survey: Detection of Angular Broadening at High Redshift?
title_short The MicroArcsecond Scintillation-Induced Variability (MASIV) Survey: Detection of Angular Broadening at High Redshift?
title_sort microarcsecond scintillation-induced variability (masiv) survey: detection of angular broadening at high redshift?
url http://hdl.handle.net/20.500.11937/24880