activity
19952026
most citedThe 2dF Galaxy Redshift Survey: Spectra and redshifts

2.4k citations · 33.2k across the 236 of their papers we have counts for

collaborators
Showing 1996Show all

11 papers · 1 filter

astro-ph1996★ 18 cited

Are the Perseus-Pisces chain and the Pavo-Indus wall connected?

Helene Di Nella, W. Couch, G. Paturel +1

A significant empty region was found between the southern Pavo- Indus (PI) wall and the northern Perseus-Pisces (PP) chain. This survey tests the reality of this void which may sim…

astro-ph1996★ 155 cited

A Catalog of Morphological Types in 10 Distant Rich Clusters of Galaxies

Ian Smail, Alan Dressler, Warrick J. Couch +4

We present catalogs of objects detected in deep images of 11 fields in 10 distant clusters obtained using WFPC-2 on board the Hubble Space Telescope. The clusters span the redshift…

astro-ph1996★ 57 cited

The Faint End of the Galaxy Luminosity Function In Moderate Redshift Clusters

Gillian Wilson, Ian Smail, Richard S. Ellis +1

We present deep two-colour photometry of two rich clusters at z=0.18, A665 and A1689. We use these data to construct number counts as a function of magnitude in the two fields. By…

astro-ph1996★ 1.6k cited

Measurements of the Cosmological Parameters Omega and Lambda from the First 7 Supernovae at z >= 0.35

S. Perlmutter, S. Gabi, G. Goldhaber +21

We have developed a technique to systematically discover and study high-redshift supernovae that can be used to measure the cosmological parameters. We report here results based on…

astro-ph1996★ 415 cited

The Homogeneity of Spheroidal Populations in Distant Clusters

Richard S. Ellis, Ian Smail, Alan Dressler +4

The small scatter observed for the U-V colors of spheroidal galaxies in nearby clusters of galaxies provides a powerful constraint on the history of star formation in dense environ…

astro-ph1996★ 44 cited

Starcounts in the Hubble Deep Field: Constraining Galactic Structure Models

R. A. Mendez, D. Minniti, G. de Marchi +2

Stellar sources are identified in the Hubble Deep Field, and accurate colours and magnitudes are presented. The predictions of a Galactic starcounts model are compared with the fai…