Conclusions from the image analysis of the VSOP Survey
| dc.creator | Dodson, R. | |
| dc.creator | Fomalont, E. | |
| dc.creator | Wiik, K. | |
| dc.date | 2009-01-12 | |
| dc.date.accessioned | 2026-07-07T12:32:48Z | |
| dc.date.available | 2026-07-07T12:32:48Z | |
| dc.description | In February 1997, the Japanese radio astronomy satellite HALCA was launched to provide the space-bourne element for the VLBI Space Observatory Programme (VSOP) mission. A significant fraction of the mission time was to be dedicated to the VSOP Survey of bright compact Active Galactic Nuclei (AGN) at 5 GHz, which was lead by ISAS. The VSOP Survey Sources are an unbiased dataset of 294 targets, of which 82% were successfully observed. These are now undergoing statistical analysis to tease out the characteristics of typical AGN sources. We present here the summary of the imaging and conclusions we have reached. | |
| dc.description | Approaching Micro-Arcsecond Resolution with VSOP-2 Symposium, Dec 2007 | |
| dc.identifier | https://arxiv.org/abs/0901.1493 | |
| dc.identifier | http://arxiv.org/abs/0901.1493 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/216905 | |
| dc.subject | Astrophysics of Galaxies | |
| dc.title | Conclusions from the image analysis of the VSOP Survey | |
| dc.type | text |