Empirical H-alpha emitter count predictions for dark energy surveys (2009)
Geach, J. E., Cimatti, A., Percival, W., Wang, Y., Guzzo, L., Zamorani, G., ...
Future galaxy redshift surveys aim to measure cosmological quantities from the galaxy power spectrum. A prime example is the detection of baryonic acoustic oscillations (BAOs), providing a standard...
Cosmological Constraints from the SDSS Luminous Red Galaxies (2006)
Tegmark, M, Eisenstein, D, Strauss, M, Weinberg, D, Blanton, M, Frieman, J, ...
We measure the large-scale real-space power spectrum P(k) using luminous red galaxies (LRGs) in the Sloan Digital Sky Survey (SDSS) and use this measurement to sharpen constraints on cosmological...
Conway, Edward, Maddox, Stephen J., Wild, Vivienne, Peacock, John A., Hawkins, Edward, Norberg, P., ...
We present an analysis of the relative bias between early- and late-type galaxies in the Two-degree Field Galaxy Redshift Survey (2dFGRS) – as defined by the η parameter of Madgwick et al., which...
Conway, Edward, Maddox, Stephen J., Wild, Vivienne, Peacock, John A., Hawkins, Edward, Norberg, P., ...
We present an analysis of the relative bias between early- and late-type galaxies in the Two-degree Field Galaxy Redshift Survey (2dFGRS) – as defined by the η parameter of Madgwick et...
Conway, Edward, Maddox, Stephen J., Wild, Vivienne, Peacock, John A., Hawkins, Edward, Norberg, P., ...
We present an analysis of the relative bias between early- and late-type galaxies in the Two-degree Field Galaxy Redshift Survey (2dFGRS) – as defined by the η parameter of Madgwick et al., which...
The nature of the relative bias between galaxies of different spectral type in 2dFGRS (2004)
Conway, E., Maddox, S., Wild, V., Peacock, J. A., Hawkins, E., Norberg, P., ...
We present an analysis of the relative bias between early- and late-type galaxies in the Two-degree Field Galaxy Redshift Survey (2dFGRS). Our analysis examines the joint counts in cells between...
Galaxy ecology : groups and low-density environments in the SDSS and 2dFGRS. (2004)
Baugh, C., Bower, R., Cole, S., Eke, V., Baldry, I. K., Balogh, M., ...
We analyse the observed correlation between galaxy environment and Hα emission-line strength, using volume-limited samples and group catalogues of 24 968 galaxies at 0.05
The 2dF Galaxy Redshift Survey: the luminosity function of cluster galaxies (2002)
De Propris, Roberto, Colless, M., Driver, S., Couch, W., Peacock, J., Baldry, I., ...
We have determined the composite luminosity function (LF) for galaxies in 60 clusters from the 2dF Galaxy Redshift Survey. The LF spans the range $-22.5
Hawkins, E., Maddox, S., Cole, S., Lahav, O., Madgwick, D., Norberg, P., ...
We present a detailed analysis of the two-point correlation function, from the 2dF Galaxy Redshift Survey (2dFGRS). We estimate the redshift-space correlation function, xi(s), from which we measure...
Studying large-scale structure with the 2dF Galaxy Redshift Survey (2002)
Peacock, J. A., Colless, M., Baldry, I., Baugh, C., Bland-Hawthorn, J., Bridges, T. J., ...
The 2dF Galaxy Redshift Survey is the first to observe more than 100,000 redshifts. This allows precise measurements of many of the key statistics of galaxy clustering, in particular redshift-space...