Analysis and Interpretation of Rock Parameters From a Radial Jack Test (In German) (9999)
For Frauenau Dam Project (Bavarian Forest) two radial jack tests in the future power tunnel were accomplished, one in the natural and the other one in the injected rock. The differences in mechanical...
Six more quasars at redshift 6 discovered by the Canada-France High-z Quasar Survey (2009)
Willott, C. J., Delorme, P., Reyle, C., Albert, L., Bergeron, J., Crampton, D., ...
We present imaging and spectroscopic observations for six quasars at z>5.9 discovered by the Canada-France High-z Quasar Survey (CFHQS). The CFHQS contains sub-surveys with a range of flux and area...
Carlberg Morris Yee, R. G. Carlberg, S. L. Morris, H. K. C. Yee, E. Ellingson, R. Abraham, ...
The baryon density of the universe is equal to the product of the baryon-to-light ratio, M b =L, and the luminosity density, j. We estimate M b =L as the sum of the masses of the X-ray gas and the...
Evolution of galaxies and clustering from the Canada-France Redshift Survey (2007)
Le Evre, O. Le F`evre, S. J. Lilly, D. Crampton, F. Hammer, D Hudon, ...
The Canada-France Redshift Survey (CFRS) sample contains 591 galaxies with secure redshift in the range 0 ! z ! 1:2. We discuss here several results: (1) the luminosity function of blue galaxies...
R. G. Carlberg, H. K. C. Yee, H. Lin, C. W. Shepherd And P. Gravel (2007)
University Of, R. G. Carlberg, H. K. C. Yee, H. Lin, C. W. Shepherd, P. Gravel, ...
. Rich galaxy clusters are powerful probes of both cosmological and galaxy evolution parameters. The CNOC cluster survey was primarily designed to distinguish between\Omega = 1 and\Omega ' 0:2...
R. G. Carlberg, H. K. C. Yee, H. Lin, C. W. Shepherd And P. Gravel (2007)
University Of, R. G. Carlberg, H. K. C. Yee, H. Lin, C. W. Shepherd, P. Gravel, ...
. Rich galaxy clusters are powerful probes of both cosmological and galaxy evolution parameters. The CNOC cluster survey was primarily designed to distinguish between\Omega = 1 and\Omega ' 0:2...
NOAO fundamental plane survey, I : survey design, redshifts, and velocity dispersion data. (2004)
Smith, R. J., Hudson, M. J., Nelan, J. E., Moore, S. A. W., Quinney, S. J., Wegner, G. A., ...
We introduce the NOAO Fundamental Plane Survey (NFPS), a wide-field imaging/spectroscopic study of rich, low-redshift galaxy clusters. The survey targets X-rayselected clusters at 0.010 < z < 0.067,...
Galaxy morphology in the rich cluster Abell 2390 (2002)
Hutchings, J. B., Saintonge, A., Schade, D., Frenette, D.
We have analysed images of the field of A2390 obtained with the CFHT and HST. The analysis fits models to bulge and disk components to several hundred galaxies, with about equal samples from the...
Le Fevre, O., Abraham, R., Lilly, S.J., Ellis, R.S., Brinchmann, J., Schade, D., ...
Hubble Space Telescope images of a sample of 285 galaxies with measured redshifts from the Canada-France Redshift Survey (CFRS) and Autofib-Low Dispersion Spectrograph Survey (LDSS) redshift surveys...
Le Fevre, O., Abraham, R., Lilly, S.J., Ellis, R.S., Brinchmann, J., Schade, D., ...
Hubble Space Telescope images of a sample of 285 galaxies with measured redshifts from the Canada-France Redshift Survey (CFRS) and Autofib-Low Dispersion Spectrograph Survey (LDSS) redshift surveys...
Le Fevre, O., Abraham, R., Lilly, S.J., Ellis, R.S., Brinchmann, J., Schade, D., ...
Hubble Space Telescope images of a sample of 285 galaxies with measured redshifts from the Canada-France Redshift Survey (CFRS) and Autofib-Low Dispersion Spectrograph Survey (LDSS) redshift surveys...
Le Fevre, O., Abraham, R., Lilly, S.J., Ellis, R.S., Brinchmann, J., Schade, D., ...
Hubble Space Telescope images of a sample of 285 galaxies with measured redshifts from the Canada-France Redshift Survey (CFRS) and Autofib-Low Dispersion Spectrograph Survey (LDSS) redshift surveys...
Le Fevre, O., Abraham, R., Lilly, S.J., Ellis, R.S., Brinchmann, J., Schade, D., ...
Hubble Space Telescope images of a sample of 285 galaxies with measured redshifts from the Canada-France Redshift Survey (CFRS) and Autofib-Low Dispersion Spectrograph Survey (LDSS) redshift surveys...
Le Fevre, O., Abraham, R., Lilly, S.J., Ellis, R.S., Brinchmann, J., Schade, D., ...
Hubble Space Telescope images of a sample of 285 galaxies with measured redshifts from the Canada-France Redshift Survey (CFRS) and Autofib-Low Dispersion Spectrograph Survey (LDSS) redshift surveys...
Le Fevre, O., Abraham, R., Lilly, S.J., Ellis, R.S., Brinchmann, J., Schade, D., ...
Hubble Space Telescope images of a sample of 285 galaxies with measured redshifts from the Canada-France Redshift Survey (CFRS) and Autofib-Low Dispersion Spectrograph Survey (LDSS) redshift surveys...
Fevre, O. Le, Abraham, R., Lilly, S. J., Ellis, R. S., Brinchmann, J., Schade, D., ...
HST images of a sample of 285 galaxies with measured z from the CFRS and Autofib-LDSS redshift surveys are analysed to derive the evolution of the merger fraction out to z~1. We have performed visual...
The CNOC2 field galaxy redshift survey (1999)
Carlberg, R. G., Yee, H. K. C., Morris, S. L., Lin, H., Sawicki, M., Wirth, G., ...
Kaimer, M., Schade, D., [Hrsg.], Ballschmiter, K., Barniske, L., Berghoff, R., ...
Berlin : Erich Schmidt, 1999
The CNOC2 Field Galaxy Redshift Survey (1998)
Carlberg, R. G., Yee, H. K. C., Morris, S. L, Lin, H., Sawicki, M., Wirth, G., ...
The CNOC2 field galaxy redshift survey is designed to provide measurements of the evolution of galaxies and their clustering over the redshift range 0 to 0.7. The sample is spread over four sky...
The Omega_M-Omega_Lambda Constraint from CNOC Clusters (1998)
Carlberg, R. G., Yee, H. K. C., Ellingson, E., Morris, S. L., Lin, H., Sawicki, M., ...
The CNOC redshift survey of galaxy clusters measures Omega_M from Omega_e(z)= M/L x j/\rho_c which can be applied on a cluster-by-cluster basis. The mass-to-light ratios, M/L, are estimated from rich...
Results on Galaxy Evolution from the CNOC2 Field Galaxy Redshift Survey (1997)
Lin, H., Yee, H. K. C., Carlberg, R. G., Morris, S. L., Sawicki, M., Patton, D. R., ...
The CNOC2 Field Galaxy Redshift Survey presently contains some 5000 galaxy redshifts, plus extensive UBgRI photometry, and is the largest galaxy sample at moderate redshifts 0.1 < z < 0.6. Here we...
HST imaging of CFRS and LDSS galaxies - I: Morphological Properties (1997)
Brinchmann, J., Abraham, R., Schade, D., Tresse, L., Ellis, R. S., Lilly, S. J., ...
(Abridged) We analyse Hubble Space Telescope images of a complete sample of 341 galaxies drawn from both the Canada France and Autofib/Low Dispersion Survey Spectrograph ground-based redshift...
Lilly, S. J., Schade, D., Ellis, R. S., Fevre, O. Le, Brinchmann, J., Abraham, R., ...
(Abridged) Several aspects of the evolution of star-forming galaxies are studied using measures of the 2-dimensional surface brightness profile of a sample of 341 faint objects selected from the CFRS...
Omega_M and the CNOC Surveys (1997)
Carlberg, R. G., Yee, H. K. C., Lin, H., Sawicki, M., Shepherd, C. W., Ellingson, E., ...
The CNOC1 cluster survey measures Omega_M via Oort's method, Omega_M= M/L x j/rho_c, where M/L is the field mass-to-light ratio, j is the field luminosity density and rho_c is the closure density. A...
Omega baryon via Oort's Method (1997)
Carlberg, R. G., Morris, S. L., Yee, H. K. C., Ellingson, E., Abraham, R., Lin, H., ...
The baryon density of the universe is equal to the product of the baryon-to-light ratio, M_b/L, and the luminosity density, j. We estimate M_b/L as the sum of the masses of the X-ray gas and the...
Carlberg, R. G., Yee, H. K. C., Lin, H., Shepherd, C. W., Gravel, P., Ellingson, E., ...
Rich galaxy clusters are powerful probes of both cosmological and galaxy evolution parameters. The CNOC cluster survey was primarily designed to distinguish between Omega=1 and Omega~0.2 cosmologies....
.$\Omega_b$ via Oort's Method (1997)
R. G. Carlberg, S. L. Morris, H. K. C. Yee, E. Ellingson, R. Abraham, H. Lin, ...
The baryon density of the universe is equal to the product of the baryon-to-light ratio, M b =L, and the luminosity density, j. We estimate M b =L as the sum of the masses of the X-ray gas and the...
CFRS XIV: Spectral Properties Of Field Galaxies Up To z = 1 (1996)
Hammer, F., Flores, H., Lilly, S. J., Crampton, David, Fevre, O. Le, Rola, C., ...
The spectral properties of more than 400 CFRS galaxies and their changes over the redshift interval 0 - 1.3 are investigated. Emission line intensities and equivalent widths for accessible lines have...
Evolution of galactic disks in clusters and the field at $0.1 < z < 0.6$ in the CNOC survey (1996)
Schade, D., Carlberg, R. G., Yee, H. K. C., Lopez-Cruz, O., Ellingson, E.
Two-dimensional surface photometry is presented for a sample of 351 late-type galaxies with $0.12 < z < 0.65$. These objects are drawn from the Canadian Network for Observational Cosmology (CNOC)...
Evolution of Cluster and Field Ellipticals at $0.2 < z < 0.6$ in the CNOC Cluster Survey (1996)
Schade, D., Carlberg, R. G., Yee, H. K. C., Lopez-Cruz, O., Ellingson, E.
Two-dimensional surface photometry has been done for 166 {\em early-type} galaxies (bulge/total luminosity $B/T>0.6$) in 3 fields of the Canadian Network for Observational Cosmology (CNOC) cluster...