ATCA radio monitoring of blazars observed with BeppoSAX
| dc.contributor.author | Bignall, Hayley | |
| dc.contributor.author | Tzioumis, A. | |
| dc.contributor.author | Jauncey, D. | |
| dc.contributor.author | Venturi, T. | |
| dc.contributor.author | Clay, R. | |
| dc.date.accessioned | 2017-01-30T14:35:28Z | |
| dc.date.available | 2017-01-30T14:35:28Z | |
| dc.date.created | 2012-12-03T07:24:55Z | |
| dc.date.issued | 2004 | |
| dc.identifier.citation | Bignall, H.E. and Tzioumis, A.K. and Jauncey, D.L. and Venturi, T. and Clay, R.W. 2004. ATCA radio monitoring of blazars observed with BeppoSAX. Nuclear Physics B. 132: pp. 149-152. | |
| dc.identifier.uri | http://hdl.handle.net/20.500.11937/39622 | |
| dc.identifier.doi | 10.1016/j.nuclphysbps.2004.04.020 | |
| dc.description.abstract |
Between 1997 and 2000, a sample of radio-bright blazars, selected from the BeppoSAX target list, was monitored with the Australia Telescope Compact Array (ATCA). Observations were obtained approximately every two months, at wavelengths of 21, 12, 6 and 3 cm simultaneously. Variability in both total flux density and linear polarization was observed in all sources, on a variety of timescales, due to both source-intrinsic effects and interstellar scintillation. | |
| dc.publisher | Elsevier | |
| dc.subject | interstellar scintillation | |
| dc.title | ATCA radio monitoring of blazars observed with BeppoSAX | |
| dc.type | Journal Article | |
| dcterms.source.volume | 132 | |
| dcterms.source.startPage | 149 | |
| dcterms.source.endPage | 152 | |
| dcterms.source.issn | 0920-5632 | |
| dcterms.source.title | Nuclear Physics B | |
| curtin.department | ||
| curtin.accessStatus | Fulltext not available |