activity
19951999
collaborators

8 papers

astro-ph1999

Hubble Space Telescope Imaging of the CFRS and LDSS Redshift Surveys---III. Field elliptical galaxies at 0.2 < z < 1.0

David Schade, S. J. Lilly, D. Crampton +9

Surface photometry has been performed on a sample of 46 field elliptical galaxies. These galaxies are described well by a deVaucouleurs R^{1/4} profile. The sample was selected fro…

astro-ph1996

The Canada-France Redshift Survey XII: Nature of emission-line field galaxy population up to z = 0.3

L. Tresse, C. Rola, F. Hammer +4

We present a spectroscopic study of the 138 field galaxies to a redshift z = 0.3 from the I-selected Canada-France Redshift Survey. 117(85%) spectra exhibit at least H alpha in emi…

astro-ph1996

The CANADA-FRANCE REDSHIFT SURVEY XI: Morphology of high-redshift field galaxies from high-resolution ground-based imaging

David Schade, S. J. Lilly, O. Le Fevre +2

The 143 galaxies with secure redshifts (median z = 0.62) from the 1415+52 field of the Canada-France Redshift Survey have been imaged at CFHT with median seeing of 0.67 arcseconds.…

astro-ph1995

The Canada-France Redshift Survey X: The Quasar Sample

David Schade, David Crampton, F. Hammer +2

Six objects with broad emission lines and redshifts from 0.48 to 2.07 were discovered among 736 extragalactic objects in the Canada-France Redshift Survey (CFRS). Although the lumi…

astro-ph1995

THE CANADA-FRANCE REDSHIFT SURVEY IX: HST Imaging of High-Redshift Field Galaxies

D. J. Schade, S. J. Lilly, David Crampton +3

HST B and I images are presented of 32 CFRS galaxies with secure redshifts in the range 0.5 < z < 1.2. These galaxies exhibit the same range of morphological types as seen locally,…

astro-ph1995

THE CANADA-FRANCE REDSHIFT SURVEY IV: Spectroscopic Selection Effects and 0300+00 Field Spectroscopic Data

F. Hammer, David Crampton, O. Le Fevre +1

Possible surface brightness selection effects in the redshift catalogs of the Canada-France Redshift Survey are investigated through comparisons of subsamples of the data. Our anal…