The evolution of type 1 AGN at 15um from the ELAIS
| dc.creator | La Franca, F. | |
| dc.creator | Matute, I. | |
| dc.creator | Gruppioni, C. | |
| dc.creator | Alexander, D. | |
| dc.creator | consortium, plus ELAIS | |
| dc.date | 2000-06-13 | |
| dc.date.accessioned | 2026-07-07T01:53:57Z | |
| dc.date.available | 2026-07-07T01:53:57Z | |
| dc.description | We present the first preliminary estimate of the evolution of type 1 AGNs at 15 um. A new sample of sources selected from the ELAIS-S1 survey has been used together with the RMS sample. The ELAIS-S1 survey covers an effective area of 2.2 deg^2 (total: 4 deg^2) down to 1.2 mJy at 15 um. Spectroscopic identifications have been carried out in the range 17.2<R<20.0 at the 3.6m/ESO, NTT/ESO and 2dF/AAT. The luminosity function is steeper at bright luminosities in comparison to the previous estimates of Rush, Malkan & Spinoglio (1993). The evolution is compatible with a Pure Luminosity Evolution model with L(z)=L(0)(1+z)^3.4. | |
| dc.description | 3 pages, to appear in the proceedings of the Fourth Italian Conference on AGNs (MemSAIt) | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0006177 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0006177 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/1158 | |
| dc.subject | Astrophysics | |
| dc.title | The evolution of type 1 AGN at 15um from the ELAIS | |
| dc.type | text |