A hole in the sky - The dependence of the galaxy luminosity function on the environment
| dc.creator | Phleps, S. | |
| dc.creator | Wolf, C. | |
| dc.creator | Peacock, J. A. | |
| dc.creator | Meisenheimer, K. | |
| dc.creator | van Kampen, E. | |
| dc.date | 2006-11-09 | |
| dc.date.accessioned | 2026-07-07T07:30:44Z | |
| dc.date.available | 2026-07-07T07:30:44Z | |
| dc.description | We have developed a method to calculate overdensities in multicolour surveys, and compare the local density contrast measured in galaxy samples with different redshift error distributions. We calculated overdensities for three COMBO-17 fields, and identified a region in the CDFS, where the density is lower by a factor of 2 compared to the other two fields. This is mainly due to a deficiency of faint red galaxies. This result is in agreement with local observations in the 2dF. | |
| dc.description | To appear in the ASP Conference Series (Proceedings of the Cosmic Frontiers conference held in Durham, 31st July - 4th August 2006) | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0611287 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0611287 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/118502 | |
| dc.subject | Astrophysics | |
| dc.title | A hole in the sky - The dependence of the galaxy luminosity function on the environment | |
| dc.type | text |