Deep Blazar Surveys
| dc.creator | Padovani, Paolo | |
| dc.date | 2000-12-15 | |
| dc.date.accessioned | 2026-07-25T11:28:44Z | |
| dc.description | I address the need for deep blazar surveys by showing that our current understanding of blazars is based on a relatively small number of intrinsically luminous sources. I then review the on-going deeper surveys, addressing in particular their limits and limitations. Finally, I present some preliminary results on the evolutionary properties of faint blazars as derived from the Deep X-ray Radio Blazar Survey (DXRBS). | |
| dc.description | 13 pages, 4 figures. Self-invited talk at the Workshop "Blazar Demographics and Physics", Baltimore, July 2000, ASP Conf. Series, P. Padovani and C. M. Urry eds., in press. Postscript file also available at http://www.stsci.edu/~padovani/survey.html | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0012355 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0012355 | |
| dc.identifier.uri | https://dspace.dare.co.zw/handle/123456789/3041 | |
| dc.subject | Astrophysics | |
| dc.title | Deep Blazar Surveys | |
| dc.type | text |