Clustering in the Caltech Faint Galaxy Redshift Survey

Details Clustering in the Caltech Faint Galaxy Redshift Survey Clustering in the Caltech Faint Galaxy Redshift Survey

1999-10-13

arxiv.org/abs/astro-ph/9910242v1

Astronomy and Astrophysics

Astrophysics

To appear in proceedings of conference Clustering At High Redshift, ASP Conf. Series, ed. A. Mazuer and O.Le Fevre (Marseilles

Scientific paper

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.

Affiliated with

Also associated with

No associations

Rating

Clustering in the Caltech Faint Galaxy Redshift Survey does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Clustering in the Caltech Faint Galaxy Redshift Survey, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Clustering in the Caltech Faint Galaxy Redshift Survey will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-105433