Mining The Local Universe for Data: the QSO Luminosity Function with the Asiago-ESO/RASS QSO Survey
| dc.creator | Cristiani, S. | |
| dc.creator | Grazian, A. | |
| dc.creator | Omizzolo, A. | |
| dc.date | 2000-07-04 | |
| dc.date.accessioned | 2026-07-07T01:54:15Z | |
| dc.date.available | 2026-07-07T01:54:15Z | |
| dc.description | We present progress results of a new survey for bright QSOs (V<14.5, R<15.4, B_J<15.2) covering the whole sky at |b|>30. The surface density of QSOs brighter than B_J=14.8 turns out to be $2.9 \pm 0.8 \cdot 10^{-3} deg^{-2}$. The optical Luminosity Function at 0.04 < z < 0.3 shows significant departures from the standard pure luminosity evolution, providing new insights in the modelling of the QSO phenomenon. | |
| dc.description | 4 pages Latex, with 3 PostScript figures. Proceedings of the Meeting "AGN nel 2000", Trieste 15-18 May 2000 | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0007033 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0007033 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/1273 | |
| dc.subject | Astrophysics | |
| dc.title | Mining The Local Universe for Data: the QSO Luminosity Function with the Asiago-ESO/RASS QSO Survey | |
| dc.type | text |