Clustering in the Caltech Faint Galaxy Redshift Survey
| dc.creator | Cohen, Judith G. | |
| dc.date | 1999-10-13 | |
| dc.date.accessioned | 2026-07-07T02:33:50Z | |
| dc.date.available | 2026-07-07T02:33:50Z | |
| dc.description | The Caltech Faint Galaxy Redshift Survey has collected $\sim$2000 spectra taken with multi-slit masks using the Low Resolution Imaging Spectrograph at the Keck Observatory (Oke et al 1995) in two widely separated fields on the sky, each $\sim$1 x 1 deg$^2$. Most of these objects are faint field galaxies; about 10% are Galactic stars and about 1% are broad-lined AGNs. I summarize the small scale clustering of this sample as well as the evidence in support of large scale structure. | |
| dc.description | To appear in proceedings of conference Clustering At High Redshift, ASP Conf. Series, ed. A. Mazuer and O.Le Fevre (Marseilles, July 1999). 7 pages, 4 figures, reformatted from pasptex to aastex | |
| dc.identifier | https://arxiv.org/abs/astro-ph/9910242 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/9910242 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/15004 | |
| dc.subject | Astrophysics | |
| dc.title | Clustering in the Caltech Faint Galaxy Redshift Survey | |
| dc.type | text |