The MicroArcsecond Scintillation-Induced Variability (MASIV) Survey: Detection of Angular Broadening at High Redshift?
MetadataShow full item record
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.
Showing items related by title, author, creator and subject.
Cosmological decrease in brightness and angular broadening in the ionized inter-galactic mediumdetected in the MASIV quasar surveyrickett, B.; Lovell, J.; Macquart, Jean-Pierre; Jauncey, D.; Bignall, Hayley; Kedziora-Chudczer, L.; Ojha, R.; Pursimo, T.; Shabala, S.; Senkbeil, C. (2008)
Jauncey, D.; Lovell, J.; Senkbeil, C.; Bignall, Hayley; Macquart, Jean-Pierre; Ojha, R.; Pursimo, T.; Rickett, B.; Shabala, S. (2007)A variety of surveys, both serendipitous and systematic, have revealed the dramatic phenomenon of cm-wavelength refractive inter-stellar scintillation. Throughout these discoveries, the presence of accurate and reliable ...
The Micro-Arcsecond Scintillation-Induced Variability (Masiv) Survey. III. Optical Identifications and New RedshiftsPursimo, T; Ojha, R; Jauncey, David; Rickett, B; Dutka, M; Koay, J; Lovell, J; Bignall, Hayley; Kedziora-Chudczer, L; Macquart, Jean-Pierre (2013)Intraday variability (IDV) of the radio emission from active galactic nuclei is now known to be predominantly due to interstellar scintillation (ISS). The MASIV (The Micro-Arcsecond Scintillation-Induced Variability) ...