activity
19962001
most citedThe CNOC2 Field Galaxy Luminosity Function I: A Description of Luminosity Function Evolution

236 citations · 580 across the 14 of their papers we have counts for

collaborators

14 papers

astro-ph2001★ 53 cited

Environment and Galaxy Evolution at Intermediate Redshift in the CNOC2 Survey

R. G. Carlberg, H. K. C. Yee, S. L. Morris +5

(abridged) The systematic variation of galaxy colors and types with clustering environment could either be the result of local conditions at formation or subsequent environmental e…

astro-ph2000★ 104 cited

Galaxy Groups at Intermediate Redshift

R. G. Carlberg, H. K. C. Yee, S. L. Morris +5

Galaxy groups likely to be virialized are identified within the CNOC2 intermediate redshift galaxy survey using an iterative method. The number-velocity dispersion relation is in a…

astro-ph2000★ 10 cited

Active Galactic Nuclei in the CNOC2 Field Galaxy Redshift Survey

Patrick B. Hall, H. K. C. Yee, Huan Lin +7

We present a sample of 47 confirmed and 14 candidate Active Galactic Nuclei (AGN) discovered in the Canadian Network for Observational Cosmology field galaxy redshift survey (CNOC2…

astro-ph2000★ 8 cited

Spectroscopic Gravitational Lens Candidates in the CNOC2 Field Galaxy Redshift Survey

Patrick B. Hall, H. K. C. Yee, Huan Lin +7

We present five candidate gravitational lenses discovered spectroscopically in the Canadian Network for Observational Cosmology Field Galaxy Redshift Survey (CNOC2), along with one…

astro-ph2000★ 105 cited

The CNOC2 Field Galaxy Redshift Survey I: The Survey and the Catalog for the Patch CNOC 0223+00

H. K. C. Yee, S. L. Morris, H. Lin +7

The Canadian Network for Observational Cosmology (CNOC2) Field Galaxy Redshift Survey is a spectroscopic/photometric survey of faint galaxies over 1.5 square degrees of sky with a…

astro-ph1999

Galaxy Clustering in the CNOC2 Redshift Survey

R. G. Carlberg, H. K. C. Yee, S. L. Morris +5

The correlation evolution of a high luminosity subsample of the CNOC2 redshift survey is examined. The sample is restricted to galaxies for which the k corrected and evolution corr…