scholarly journals Topology of large-scale structure in the 2dF Galaxy Redshift Survey

2007 ◽  
Vol 375 (1) ◽  
pp. 128-136 ◽  
Author(s):  
J. B. James ◽  
G. F. Lewis ◽  
M. Colless
Keyword(s):  
Large Scale ◽  
Large Scale Structure ◽  
Scale Structure ◽  
Redshift Survey ◽  
Galaxy Redshift

scholarly journals The Durham/UKST Galaxy Redshift Survey -- I. Large-scale structure in the Universe

1996 ◽  
Vol 281 (3) ◽  
pp. L47-L52 ◽  
Author(s):  
A. Ratcliffe ◽  
T. Shanks ◽  
A. Broadbent ◽  
Q. A. Parker ◽  
F. G. Watson ◽  
...  
Keyword(s):  
Large Scale ◽  
Large Scale Structure ◽  
Scale Structure ◽  
Redshift Survey ◽  
Galaxy Redshift ◽  
The Universe

scholarly journals Large-scale structure in a new deep IRAS galaxy redshift survey

1996 ◽  
Vol 280 (3) ◽  
pp. 673-688 ◽  
Author(s):  
S. J. Oliver ◽  
M. Rowan-Robinson ◽  
T. J. Broadhurst ◽  
R. G. McMahon ◽  
W. Saunders ◽  
...  
Keyword(s):  
Large Scale ◽  
Large Scale Structure ◽  
Scale Structure ◽  
Redshift Survey ◽  
Galaxy Redshift ◽  
Iras Galaxy

scholarly journals The CNOC2 Field Galaxy Redshipt Survey

1998 ◽  
Vol 11 (1) ◽  
pp. 460-463
Author(s):  
H.K.C. Yee ◽  
M.J. Sawicki ◽  
R.G. Carlberg ◽  
H. Lin ◽  
S.L. Morris ◽  
...  
Keyword(s):  
Large Scale ◽  
Cosmological Parameters ◽  
Large Scale Structure ◽  
Scale Structure ◽  
Observational Cosmology ◽  
Data Set ◽  
Redshift Survey ◽  
Galaxy Redshift ◽  
Galaxy Population ◽  
Field Galaxy

Fundamental to our understanding of the universe is the evolution of structures, from galaxies to clusters of galaxies to large-scale sheets and filaments of galaxies and voids. The investigation of the evolution of large-scale structure not only provides us with the key test of theories of structure formation, but also allows us to measure fundamental cosmological parameters. The CNOC2 (Canadian Network for Observational Cosmology) Field Galaxy Redshift Survey is the first large redshift survey of faint galaxies carried out with the explicit goal of investigating the evolution of large scale structure. This survey also provides the largest redshift and photometric data set currently available for the study of galaxy population and evolution at the moderate redshift range between 0.1 and 0.6. In this paper we describe the scope and technique of the survey, its status, and some preliminary results.

Large-Scale Structure in the Durham/UKST Galaxy Redshift Survey

1994 ◽  
pp. 693-697
Author(s):  
A. Broadbent ◽  
T. Shanks ◽  
R. Fong ◽  
C. A. Collins ◽  
F. G. Watson ◽  
...  
Keyword(s):  
Large Scale ◽  
Large Scale Structure ◽  
Scale Structure ◽  
Redshift Survey ◽  
Galaxy Redshift

scholarly journals Large-Scale Structure in the Durham/Ukst Galaxy Redshift Survey

1994 ◽  
Vol 161 ◽  
pp. 693-697
Author(s):  
A. Broadbent ◽  
T. Shanks ◽  
F.G. Watson ◽  
Q.A. Parker ◽  
R. Fong ◽  
...  
Keyword(s):  
Correlation Function ◽  
Statistical Analysis ◽  
Large Scale ◽  
Large Scale Structure ◽  
Scale Structure ◽  
Point Correlation ◽  
Point Correlation Function ◽  
Redshift Survey ◽  
Galaxy Redshift ◽  
The Universe

We report on the progress of the compilation and analysis of the Durham/UKST galaxy redshift survey. This survey will probe a large contiguous volume of space within a 1500 sq. deg. area of sky around the SGP. It will contain redshifts of ∼ 4000 galaxies of bJ < 17m providing detailed information about the structure of the Universe on large scales. Large features on scales of ∼ 100h−1 Mpc are clearly visible on examination of the completed section of the survey, although a statistical analysis of the survey by means of the two-point correlation function is close to zero on scales of r > 10h−1 Mpc.

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