Clustering studies with the 2dF galaxy redshift survey
| dc.creator | Couch, Warrick | |
| dc.creator | Colless, Matthew | |
| dc.creator | De Propris, Roberto | |
| dc.date | 2003-09-12 | |
| dc.date.accessioned | 2026-07-07T02:09:33Z | |
| dc.date.available | 2026-07-07T02:09:33Z | |
| dc.description | The 2dF Galaxy Redshift Survey has now been completed and has mapped the three-dimensional distribution, and hence clustering, of galaxies in exquisite detail over an unprecedentedly large ($\sim 10^{8} h^{-3}$ Mpc$^{3}$) volume of the local Universe. Here we highlight some of the major results to come from studies of clustering within the survey: galaxy correlation function and power spectrum analyses and the constraints they have placed on cosmological parameters; the luminosity functions of rich galaxy clusters, their dependence on global cluster properties and galaxy type, and how they compare with the field; and the variation of galactic star formation activity with environment, both within clusters and in galaxy groups. | |
| dc.description | 16 pages, refereed conference proceedings,to appear in Carnegie Observatories Astrophysics Series, vol.3: Clusters of Galaxies: Probes of Cosmological Structure and Galaxy Evolution, edited by J. S. Mulcahey, A. Dressler, A. Oemler (CUP). Also available at: http://www.ociw.edu/ociw/symposia/series/symposium3/proceedings.html Needs cupbook.cls, caps.cls,ociwsymp3.sty (included) Figures 1,9,10,11 are low resolution bitmaps because of arxiv size limits | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0309342 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0309342 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/6470 | |
| dc.subject | Astrophysics | |
| dc.title | Clustering studies with the 2dF galaxy redshift survey | |
| dc.type | text |